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Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=275 2010-07-07T08:16:39Z

<p>Wikiadmin: /* VEx Files */</p> <hr /> <div>This wiki is provided as a tool to share information and schedules for the 2010 coordinated ground-based campaign of Venus. Please feel free to complete and modify the attached tables according to the campaign progress and your proposed observations. <br /> __TOC__<br /> <br /> ==Tools of the Venus coordinated campaign==<br /> ===Table===<br /> <br /> <br /> A list of proposed and actual observations : pre-conjunction (July 2010-Oct. 29, 2010), post conjunction (Oct. 29, 2010 - Feb. 2011)<br /> * [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination table]<br /> <br /> ===Map of observatory sites and telescopes ===<br /> <br /> Sites and telescopes used for ground-based observations, with a link to their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> ==Instrumentation of the study of Venus==<br /> === Ground-based instruments ===<br /> <br /> * Sunspot Astronomy &amp; Visitor Center<br /> APO 3.5-m<br /> <br /> ARCES<br /> <br /> * Observatorio SOAR<br /> Soar Telescope<br /> <br /> * Observatoire du Pic du Midi de Bigorre<br /> Bernard-Lyot 2-m<br /> <br /> * Osservatorio Astronomico della Regione Autonoma Valle d'Aosta<br /> <br /> * South African Astronomical Observatory<br /> Southern African Large Telescope (SALT)<br /> <br /> * Hanle Observatory<br /> HCT<br /> <br /> * National Central University Lulin Observatory<br /> LOT Cassegrain/ SLT R-C/ 4 TAOS robotic<br /> <br /> * Naroyo Observatory<br /> Naroyo 1.6-m<br /> <br /> * Siding Spring Observatory<br /> Anglo-Australian 3.9-m<br /> <br /> * Mount John University Observatory<br /> 1 m McLellan<br /> <br /> MOA 1.8-m<br /> <br /> 0.6-m Optical Craftsmen <br /> <br /> 0.6-m Boller &amp; Chivens<br /> <br /> * Mauna Kea Observatory<br /> IRTF <br /> <br /> Keck 10-m<br /> <br /> CFHT 3.6-m<br /> <br /> SUBARU<br /> <br /> JCMT<br /> <br /> * Haleakala Observatory<br /> AEOS<br /> <br /> * THIS Tuneable Heterodyne Infrared Spectrometer<br /> used at the:<br /> <br /> - McMath-Pierce Solar Telescope on Kitt Peak in Arizona<br /> <br /> - IRTF on Mauna Kea Hawaii<br /> <br /> * HIPWAC Heterodyne Instrument for Planetary Wind And Composition<br /> used at the:<br /> <br /> - IRTF<br /> <br /> === Venus Express instruments ===<br /> <br /> [[File:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> - VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> - VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> ==== VEx Files ====<br /> <br /> * SOIR Files:<br /> :[[File:SOIR_observation_list_until_Sep2010.xls‎]]<br /> <br /> This file lists all SOIR observations made from the beginning of Venus operations (April 2006) <br /> until September 2010. <br /> <br /> For further details, contact the SOIR Principal Investigator: Ann-Carine Vandaele &lt;A-C.Vandaele@aeronomie.be&gt;<br /> <br /> :[[File:SOIR_MTP56-MTP70.xls|SOIR_MTP56-MTP70.xls]]<br /> <br /> This file desctibes SOIR solar occultation opportunities in the period 30/7/2010 - 25/8/2011. SOIR occultations allow measurement of gas abundances and temperatures in the 80-150 km altitude region. <br /> <br /> For further details, contact SOIR Principal Investigator: Ann-Carine Vandaele &lt;A-C.Vandaele@aeronomie.be&gt;.<br /> <br /> * VeRa Files:<br /> :[[File:VeRa_OCC_Seasons_1-9.xls‎ |VeRa_OCC_Seasons_1-9.xls‎ ]]<br /> <br /> This file descibes all VeRa radio <br /> occultations carried out in the period 1/7/2006 - 2/6/2010. <br /> <br /> For further information contact the VeRa team: Martin Paetzold &lt;Martin.Paetzold@uni-koeln.de&gt;, Bernd Hauesler &lt;Bernd.Haeusler@unibw.de&gt;, and Silvia Tellmann &lt;tellmann@geo.uni-koeln.de&gt;<br /> <br /> :[[File:VeRa_Occultations_seasons_10-12.txt‎ ]]<br /> <br /> This file describes the future opportunities for Radio occultations in the upcoming occultation seasons in January 2011 - January 2012. <br /> File kindly provided by Stefan Remus, ESAC. <br /> <br /> For further information contact the VeRa team: Martin Paetzold <br /> &lt;Martin.Paetzold@uni-koeln.de&gt;, Bernd Hauesler <br /> &lt;Bernd.Haeusler@unibw.de&gt;, and Silvia Tellmann &lt;tellmann@geo.uni-koeln.de&gt;.<br /> <br /> === Akatsuki instruments ===<br /> <br /> [[File:Akatsuki_instruments.jpg|400px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> <br /> [http://www.jaxa.jp/countdown/f17/index_e.html Visit the Akatsuki Website]<br /> <br /> Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time) !<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about VCO/Akatsuki mission]<br /> <br /> * '''IR1''' : 1-micron Camera<br /> Low stratus, vapor, active volcanism<br /> <br /> 1.01 µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''' : 2-micron Camera<br /> Low stratus, trace gasses, zodiacal light<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65 µm<br /> <br /> * '''UVI''' : Ultraviolet Imager<br /> Cloud-top ultraviolet absorber, SO2<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''' : Longwave Infrared Camera<br /> Cloud-top temperature distribution<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''' : Lightning and Airglow Camera<br /> Lightening flash, high-stratus airglow emission<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> == Coordination meetings / meeting sessions==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/ « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris, June 28-29, 2010]<br /> * [http://www.venus.wisc.edu/workshop/ 2010 VEXAG International Workshop: Venus, Our Closest Earth-like Planet, Madison (USA), 30 August - 2 September 2010]<br /> <br /> <br /> == Other links==<br /> * [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=41012 Coordinated Ground-based Venus Observation Campaign]<br /> (Between 23 May and 9 June 2007)<br /> * [http://www.rssd.esa.int/index.php?project=VENUS Venus Ground-Based image Active Archive]<br /> <br /> The Venus ground-based image Active Archive (VAA) allows you to upload and retrieve ground-based Venus observations obtained in infrared, visual or ultraviolet light. The aim of this archive is to complement the ongoing Venus Express (VEX) spacecraft observations of Venus with worldwide ground-based images to allow for continuous monitoring of the planet.</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=274 2010-07-07T08:15:09Z

<p>Wikiadmin: /* VEx Files */</p> <hr /> <div>This wiki is provided as a tool to share information and schedules for the 2010 coordinated ground-based campaign of Venus. Please feel free to complete and modify the attached tables according to the campaign progress and your proposed observations. <br /> __TOC__<br /> <br /> ==Tools of the Venus coordinated campaign==<br /> ===Table===<br /> <br /> <br /> A list of proposed and actual observations : pre-conjunction (July 2010-Oct. 29, 2010), post conjunction (Oct. 29, 2010 - Feb. 2011)<br /> * [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination table]<br /> <br /> ===Map of observatory sites and telescopes ===<br /> <br /> Sites and telescopes used for ground-based observations, with a link to their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> ==Instrumentation of the study of Venus==<br /> === Ground-based instruments ===<br /> <br /> * Sunspot Astronomy &amp; Visitor Center<br /> APO 3.5-m<br /> <br /> ARCES<br /> <br /> * Observatorio SOAR<br /> Soar Telescope<br /> <br /> * Observatoire du Pic du Midi de Bigorre<br /> Bernard-Lyot 2-m<br /> <br /> * Osservatorio Astronomico della Regione Autonoma Valle d'Aosta<br /> <br /> * South African Astronomical Observatory<br /> Southern African Large Telescope (SALT)<br /> <br /> * Hanle Observatory<br /> HCT<br /> <br /> * National Central University Lulin Observatory<br /> LOT Cassegrain/ SLT R-C/ 4 TAOS robotic<br /> <br /> * Naroyo Observatory<br /> Naroyo 1.6-m<br /> <br /> * Siding Spring Observatory<br /> Anglo-Australian 3.9-m<br /> <br /> * Mount John University Observatory<br /> 1 m McLellan<br /> <br /> MOA 1.8-m<br /> <br /> 0.6-m Optical Craftsmen <br /> <br /> 0.6-m Boller &amp; Chivens<br /> <br /> * Mauna Kea Observatory<br /> IRTF <br /> <br /> Keck 10-m<br /> <br /> CFHT 3.6-m<br /> <br /> SUBARU<br /> <br /> JCMT<br /> <br /> * Haleakala Observatory<br /> AEOS<br /> <br /> * THIS Tuneable Heterodyne Infrared Spectrometer<br /> used at the:<br /> <br /> - McMath-Pierce Solar Telescope on Kitt Peak in Arizona<br /> <br /> - IRTF on Mauna Kea Hawaii<br /> <br /> * HIPWAC Heterodyne Instrument for Planetary Wind And Composition<br /> used at the:<br /> <br /> - IRTF<br /> <br /> === Venus Express instruments ===<br /> <br /> [[File:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> - VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> - VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> ==== VEx Files ====<br /> <br /> * SOIR Files:<br /> :[[File:SOIR_observation_list_until_Sep2010.xls‎]]<br /> <br /> This file lists all SOIR observations made from the beginning of Venus operations (April 2006) <br /> until August 2010. <br /> <br /> For further details, contact the SOIR Principal Investigator: Ann-Carine Vandaele &lt;A-C.Vandaele@aeronomie.be&gt;<br /> <br /> :[[File:SOIR_MTP56-MTP70.xls|SOIR_MTP56-MTP70.xls]]<br /> <br /> This file desctibes SOIR solar occultation opportunities in the period 30/7/2010 - 25/8/2011. SOIR occultations allow measurement of gas abundances and temperatures in the 80-150 km altitude region. <br /> <br /> For further details, contact SOIR Principal Investigator: Ann-Carine Vandaele &lt;A-C.Vandaele@aeronomie.be&gt;.<br /> <br /> * VeRa Files:<br /> :[[File:VeRa_OCC_Seasons_1-9.xls‎ |VeRa_OCC_Seasons_1-9.xls‎ ]]<br /> <br /> This file descibes all VeRa radio <br /> occultations carried out in the period 1/7/2006 - 2/6/2010. <br /> <br /> For further information contact the VeRa team: Martin Paetzold &lt;Martin.Paetzold@uni-koeln.de&gt;, Bernd Hauesler &lt;Bernd.Haeusler@unibw.de&gt;, and Silvia Tellmann &lt;tellmann@geo.uni-koeln.de&gt;<br /> <br /> :[[File:VeRa_Occultations_seasons_10-12.txt‎ ]]<br /> <br /> This file describes the future opportunities for Radio occultations in the upcoming occultation seasons in January 2011 - January 2012. <br /> File kindly provided by Stefan Remus, ESAC. <br /> <br /> For further information contact the VeRa team: Martin Paetzold <br /> &lt;Martin.Paetzold@uni-koeln.de&gt;, Bernd Hauesler <br /> &lt;Bernd.Haeusler@unibw.de&gt;, and Silvia Tellmann &lt;tellmann@geo.uni-koeln.de&gt;.<br /> <br /> === Akatsuki instruments ===<br /> <br /> [[File:Akatsuki_instruments.jpg|400px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> <br /> [http://www.jaxa.jp/countdown/f17/index_e.html Visit the Akatsuki Website]<br /> <br /> Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time) !<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about VCO/Akatsuki mission]<br /> <br /> * '''IR1''' : 1-micron Camera<br /> Low stratus, vapor, active volcanism<br /> <br /> 1.01 µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''' : 2-micron Camera<br /> Low stratus, trace gasses, zodiacal light<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65 µm<br /> <br /> * '''UVI''' : Ultraviolet Imager<br /> Cloud-top ultraviolet absorber, SO2<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''' : Longwave Infrared Camera<br /> Cloud-top temperature distribution<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''' : Lightning and Airglow Camera<br /> Lightening flash, high-stratus airglow emission<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> == Coordination meetings / meeting sessions==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/ « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris, June 28-29, 2010]<br /> * [http://www.venus.wisc.edu/workshop/ 2010 VEXAG International Workshop: Venus, Our Closest Earth-like Planet, Madison (USA), 30 August - 2 September 2010]<br /> <br /> <br /> == Other links==<br /> * [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=41012 Coordinated Ground-based Venus Observation Campaign]<br /> (Between 23 May and 9 June 2007)<br /> * [http://www.rssd.esa.int/index.php?project=VENUS Venus Ground-Based image Active Archive]<br /> <br /> The Venus ground-based image Active Archive (VAA) allows you to upload and retrieve ground-based Venus observations obtained in infrared, visual or ultraviolet light. The aim of this archive is to complement the ongoing Venus Express (VEX) spacecraft observations of Venus with worldwide ground-based images to allow for continuous monitoring of the planet.</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=File:SOIR_observation_list_until_Sep2010.xls&diff=273 2010-07-07T08:14:13Z

<p>Wikiadmin: </p> <hr /> <div></div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=272 2010-07-06T13:50:20Z

<p>Wikiadmin: /* Other links */</p> <hr /> <div>This wiki is provided as a tool to share information and schedules for the 2010 coordinated ground-based campaign of Venus. Please feel free to complete and modify the attached tables according to the campaign progress and your proposed observations. <br /> __TOC__<br /> <br /> ==Tools of the Venus coordinated campaign==<br /> ===Table===<br /> <br /> <br /> A list of proposed and actual observations : pre-conjunction (July 2010-Oct. 29, 2010), post conjunction (Oct. 29, 2010 - Feb. 2011)<br /> * [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination table]<br /> <br /> ===Map of observatory sites and telescopes ===<br /> <br /> Sites and telescopes used for ground-based observations, with a link to their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> ==Instrumentation of the study of Venus==<br /> === Ground-based instruments ===<br /> <br /> * Sunspot Astronomy &amp; Visitor Center<br /> APO 3.5-m<br /> <br /> ARCES<br /> <br /> * Observatorio SOAR<br /> Soar Telescope<br /> <br /> * Observatoire du Pic du Midi de Bigorre<br /> Bernard-Lyot 2-m<br /> <br /> * Osservatorio Astronomico della Regione Autonoma Valle d'Aosta<br /> <br /> * South African Astronomical Observatory<br /> Southern African Large Telescope (SALT)<br /> <br /> * Hanle Observatory<br /> HCT<br /> <br /> * National Central University Lulin Observatory<br /> LOT Cassegrain/ SLT R-C/ 4 TAOS robotic<br /> <br /> * Naroyo Observatory<br /> Naroyo 1.6-m<br /> <br /> * Siding Spring Observatory<br /> Anglo-Australian 3.9-m<br /> <br /> * Mount John University Observatory<br /> 1 m McLellan<br /> <br /> MOA 1.8-m<br /> <br /> 0.6-m Optical Craftsmen <br /> <br /> 0.6-m Boller &amp; Chivens<br /> <br /> * Mauna Kea Observatory<br /> IRTF <br /> <br /> Keck 10-m<br /> <br /> CFHT 3.6-m<br /> <br /> SUBARU<br /> <br /> JCMT<br /> <br /> * Haleakala Observatory<br /> AEOS<br /> <br /> * THIS Tuneable Heterodyne Infrared Spectrometer<br /> used at the:<br /> <br /> - McMath-Pierce Solar Telescope on Kitt Peak in Arizona<br /> <br /> - IRTF on Mauna Kea Hawaii<br /> <br /> * HIPWAC Heterodyne Instrument for Planetary Wind And Composition<br /> used at the:<br /> <br /> - IRTF<br /> <br /> === Venus Express instruments ===<br /> <br /> [[File:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> - VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> - VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> ==== VEx Files ====<br /> <br /> * SOIR Files:<br /> :[[File:SOIR_observation_list_until_Aug2010.xls‎|SOIR_observation_list_until_Aug2010.xls‎]]<br /> <br /> This file lists all SOIR observations made from the beginning of Venus operations (April 2006) <br /> until August 2010. <br /> <br /> For further details, contact the SOIR Principal Investigator: Ann-Carine Vandaele &lt;A-C.Vandaele@aeronomie.be&gt;<br /> <br /> :[[File:SOIR_MTP56-MTP70.xls|SOIR_MTP56-MTP70.xls]]<br /> <br /> This file desctibes SOIR solar occultation opportunities in the period 30/7/2010 - 25/8/2011. SOIR occultations allow measurement of gas abundances and temperatures in the 80-150 km altitude region. <br /> <br /> For further details, contact SOIR Principal Investigator: Ann-Carine Vandaele &lt;A-C.Vandaele@aeronomie.be&gt;.<br /> <br /> * VeRa Files:<br /> :[[File:VeRa_OCC_Seasons_1-9.xls‎ |VeRa_OCC_Seasons_1-9.xls‎ ]]<br /> <br /> This file descibes all VeRa radio <br /> occultations carried out in the period 1/7/2006 - 2/6/2010. <br /> <br /> For further information contact the VeRa team: Martin Paetzold &lt;Martin.Paetzold@uni-koeln.de&gt;, Bernd Hauesler &lt;Bernd.Haeusler@unibw.de&gt;, and Silvia Tellmann &lt;tellmann@geo.uni-koeln.de&gt;<br /> <br /> :[[File:VeRa_Occultations_seasons_10-12.txt‎ ]]<br /> <br /> This file describes the future opportunities for Radio occultations in the upcoming occultation seasons in January 2011 - January 2012. <br /> File kindly provided by Stefan Remus, ESAC. <br /> <br /> For further information contact the VeRa team: Martin Paetzold <br /> &lt;Martin.Paetzold@uni-koeln.de&gt;, Bernd Hauesler <br /> &lt;Bernd.Haeusler@unibw.de&gt;, and Silvia Tellmann &lt;tellmann@geo.uni-koeln.de&gt;.<br /> <br /> === Akatsuki instruments ===<br /> <br /> [[File:Akatsuki_instruments.jpg|400px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> <br /> [http://www.jaxa.jp/countdown/f17/index_e.html Visit the Akatsuki Website]<br /> <br /> Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time) !<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about VCO/Akatsuki mission]<br /> <br /> * '''IR1''' : 1-micron Camera<br /> Low stratus, vapor, active volcanism<br /> <br /> 1.01 µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''' : 2-micron Camera<br /> Low stratus, trace gasses, zodiacal light<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65 µm<br /> <br /> * '''UVI''' : Ultraviolet Imager<br /> Cloud-top ultraviolet absorber, SO2<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''' : Longwave Infrared Camera<br /> Cloud-top temperature distribution<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''' : Lightning and Airglow Camera<br /> Lightening flash, high-stratus airglow emission<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> == Coordination meetings / meeting sessions==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/ « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris, June 28-29, 2010]<br /> * [http://www.venus.wisc.edu/workshop/ 2010 VEXAG International Workshop: Venus, Our Closest Earth-like Planet, Madison (USA), 30 August - 2 September 2010]<br /> <br /> <br /> == Other links==<br /> * [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=41012 Coordinated Ground-based Venus Observation Campaign]<br /> (Between 23 May and 9 June 2007)<br /> * [http://www.rssd.esa.int/index.php?project=VENUS Venus Ground-Based image Active Archive]<br /> <br /> The Venus ground-based image Active Archive (VAA) allows you to upload and retrieve ground-based Venus observations obtained in infrared, visual or ultraviolet light. The aim of this archive is to complement the ongoing Venus Express (VEX) spacecraft observations of Venus with worldwide ground-based images to allow for continuous monitoring of the planet.</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=271 2010-07-06T13:49:47Z

<p>Wikiadmin: /* Other links */</p> <hr /> <div>This wiki is provided as a tool to share information and schedules for the 2010 coordinated ground-based campaign of Venus. Please feel free to complete and modify the attached tables according to the campaign progress and your proposed observations. <br /> __TOC__<br /> <br /> ==Tools of the Venus coordinated campaign==<br /> ===Table===<br /> <br /> <br /> A list of proposed and actual observations : pre-conjunction (July 2010-Oct. 29, 2010), post conjunction (Oct. 29, 2010 - Feb. 2011)<br /> * [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination table]<br /> <br /> ===Map of observatory sites and telescopes ===<br /> <br /> Sites and telescopes used for ground-based observations, with a link to their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> ==Instrumentation of the study of Venus==<br /> === Ground-based instruments ===<br /> <br /> * Sunspot Astronomy &amp; Visitor Center<br /> APO 3.5-m<br /> <br /> ARCES<br /> <br /> * Observatorio SOAR<br /> Soar Telescope<br /> <br /> * Observatoire du Pic du Midi de Bigorre<br /> Bernard-Lyot 2-m<br /> <br /> * Osservatorio Astronomico della Regione Autonoma Valle d'Aosta<br /> <br /> * South African Astronomical Observatory<br /> Southern African Large Telescope (SALT)<br /> <br /> * Hanle Observatory<br /> HCT<br /> <br /> * National Central University Lulin Observatory<br /> LOT Cassegrain/ SLT R-C/ 4 TAOS robotic<br /> <br /> * Naroyo Observatory<br /> Naroyo 1.6-m<br /> <br /> * Siding Spring Observatory<br /> Anglo-Australian 3.9-m<br /> <br /> * Mount John University Observatory<br /> 1 m McLellan<br /> <br /> MOA 1.8-m<br /> <br /> 0.6-m Optical Craftsmen <br /> <br /> 0.6-m Boller &amp; Chivens<br /> <br /> * Mauna Kea Observatory<br /> IRTF <br /> <br /> Keck 10-m<br /> <br /> CFHT 3.6-m<br /> <br /> SUBARU<br /> <br /> JCMT<br /> <br /> * Haleakala Observatory<br /> AEOS<br /> <br /> * THIS Tuneable Heterodyne Infrared Spectrometer<br /> used at the:<br /> <br /> - McMath-Pierce Solar Telescope on Kitt Peak in Arizona<br /> <br /> - IRTF on Mauna Kea Hawaii<br /> <br /> * HIPWAC Heterodyne Instrument for Planetary Wind And Composition<br /> used at the:<br /> <br /> - IRTF<br /> <br /> === Venus Express instruments ===<br /> <br /> [[File:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> - VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> - VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> ==== VEx Files ====<br /> <br /> * SOIR Files:<br /> :[[File:SOIR_observation_list_until_Aug2010.xls‎|SOIR_observation_list_until_Aug2010.xls‎]]<br /> <br /> This file lists all SOIR observations made from the beginning of Venus operations (April 2006) <br /> until August 2010. <br /> <br /> For further details, contact the SOIR Principal Investigator: Ann-Carine Vandaele &lt;A-C.Vandaele@aeronomie.be&gt;<br /> <br /> :[[File:SOIR_MTP56-MTP70.xls|SOIR_MTP56-MTP70.xls]]<br /> <br /> This file desctibes SOIR solar occultation opportunities in the period 30/7/2010 - 25/8/2011. SOIR occultations allow measurement of gas abundances and temperatures in the 80-150 km altitude region. <br /> <br /> For further details, contact SOIR Principal Investigator: Ann-Carine Vandaele &lt;A-C.Vandaele@aeronomie.be&gt;.<br /> <br /> * VeRa Files:<br /> :[[File:VeRa_OCC_Seasons_1-9.xls‎ |VeRa_OCC_Seasons_1-9.xls‎ ]]<br /> <br /> This file descibes all VeRa radio <br /> occultations carried out in the period 1/7/2006 - 2/6/2010. <br /> <br /> For further information contact the VeRa team: Martin Paetzold &lt;Martin.Paetzold@uni-koeln.de&gt;, Bernd Hauesler &lt;Bernd.Haeusler@unibw.de&gt;, and Silvia Tellmann &lt;tellmann@geo.uni-koeln.de&gt;<br /> <br /> :[[File:VeRa_Occultations_seasons_10-12.txt‎ ]]<br /> <br /> This file describes the future opportunities for Radio occultations in the upcoming occultation seasons in January 2011 - January 2012. <br /> File kindly provided by Stefan Remus, ESAC. <br /> <br /> For further information contact the VeRa team: Martin Paetzold <br /> &lt;Martin.Paetzold@uni-koeln.de&gt;, Bernd Hauesler <br /> &lt;Bernd.Haeusler@unibw.de&gt;, and Silvia Tellmann &lt;tellmann@geo.uni-koeln.de&gt;.<br /> <br /> === Akatsuki instruments ===<br /> <br /> [[File:Akatsuki_instruments.jpg|400px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> <br /> [http://www.jaxa.jp/countdown/f17/index_e.html Visit the Akatsuki Website]<br /> <br /> Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time) !<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about VCO/Akatsuki mission]<br /> <br /> * '''IR1''' : 1-micron Camera<br /> Low stratus, vapor, active volcanism<br /> <br /> 1.01 µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''' : 2-micron Camera<br /> Low stratus, trace gasses, zodiacal light<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65 µm<br /> <br /> * '''UVI''' : Ultraviolet Imager<br /> Cloud-top ultraviolet absorber, SO2<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''' : Longwave Infrared Camera<br /> Cloud-top temperature distribution<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''' : Lightning and Airglow Camera<br /> Lightening flash, high-stratus airglow emission<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> == Coordination meetings / meeting sessions==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/ « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris, June 28-29, 2010]<br /> * [http://www.venus.wisc.edu/workshop/ 2010 VEXAG International Workshop: Venus, Our Closest Earth-like Planet, Madison (USA), 30 August - 2 September 2010]<br /> <br /> <br /> == Other links==<br /> * [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=41012 Coordinated Ground-based Venus Observation Campaign]<br /> 2007<br /> * [http://www.rssd.esa.int/index.php?project=VENUS Venus Ground-Based image Active Archive]<br /> <br /> The Venus ground-based image Active Archive (VAA) allows you to upload and retrieve ground-based Venus observations obtained in infrared, visual or ultraviolet light. The aim of this archive is to complement the ongoing Venus Express (VEX) spacecraft observations of Venus with worldwide ground-based images to allow for continuous monitoring of the planet.</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=270 2010-07-06T13:48:16Z

<p>Wikiadmin: /* Other links */</p> <hr /> <div>This wiki is provided as a tool to share information and schedules for the 2010 coordinated ground-based campaign of Venus. Please feel free to complete and modify the attached tables according to the campaign progress and your proposed observations. <br /> __TOC__<br /> <br /> ==Tools of the Venus coordinated campaign==<br /> ===Table===<br /> <br /> <br /> A list of proposed and actual observations : pre-conjunction (July 2010-Oct. 29, 2010), post conjunction (Oct. 29, 2010 - Feb. 2011)<br /> * [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination table]<br /> <br /> ===Map of observatory sites and telescopes ===<br /> <br /> Sites and telescopes used for ground-based observations, with a link to their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> ==Instrumentation of the study of Venus==<br /> === Ground-based instruments ===<br /> <br /> * Sunspot Astronomy &amp; Visitor Center<br /> APO 3.5-m<br /> <br /> ARCES<br /> <br /> * Observatorio SOAR<br /> Soar Telescope<br /> <br /> * Observatoire du Pic du Midi de Bigorre<br /> Bernard-Lyot 2-m<br /> <br /> * Osservatorio Astronomico della Regione Autonoma Valle d'Aosta<br /> <br /> * South African Astronomical Observatory<br /> Southern African Large Telescope (SALT)<br /> <br /> * Hanle Observatory<br /> HCT<br /> <br /> * National Central University Lulin Observatory<br /> LOT Cassegrain/ SLT R-C/ 4 TAOS robotic<br /> <br /> * Naroyo Observatory<br /> Naroyo 1.6-m<br /> <br /> * Siding Spring Observatory<br /> Anglo-Australian 3.9-m<br /> <br /> * Mount John University Observatory<br /> 1 m McLellan<br /> <br /> MOA 1.8-m<br /> <br /> 0.6-m Optical Craftsmen <br /> <br /> 0.6-m Boller &amp; Chivens<br /> <br /> * Mauna Kea Observatory<br /> IRTF <br /> <br /> Keck 10-m<br /> <br /> CFHT 3.6-m<br /> <br /> SUBARU<br /> <br /> JCMT<br /> <br /> * Haleakala Observatory<br /> AEOS<br /> <br /> * THIS Tuneable Heterodyne Infrared Spectrometer<br /> used at the:<br /> <br /> - McMath-Pierce Solar Telescope on Kitt Peak in Arizona<br /> <br /> - IRTF on Mauna Kea Hawaii<br /> <br /> * HIPWAC Heterodyne Instrument for Planetary Wind And Composition<br /> used at the:<br /> <br /> - IRTF<br /> <br /> === Venus Express instruments ===<br /> <br /> [[File:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> - VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> - VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> ==== VEx Files ====<br /> <br /> * SOIR Files:<br /> :[[File:SOIR_observation_list_until_Aug2010.xls‎|SOIR_observation_list_until_Aug2010.xls‎]]<br /> <br /> This file lists all SOIR observations made from the beginning of Venus operations (April 2006) <br /> until August 2010. <br /> <br /> For further details, contact the SOIR Principal Investigator: Ann-Carine Vandaele &lt;A-C.Vandaele@aeronomie.be&gt;<br /> <br /> :[[File:SOIR_MTP56-MTP70.xls|SOIR_MTP56-MTP70.xls]]<br /> <br /> This file desctibes SOIR solar occultation opportunities in the period 30/7/2010 - 25/8/2011. SOIR occultations allow measurement of gas abundances and temperatures in the 80-150 km altitude region. <br /> <br /> For further details, contact SOIR Principal Investigator: Ann-Carine Vandaele &lt;A-C.Vandaele@aeronomie.be&gt;.<br /> <br /> * VeRa Files:<br /> :[[File:VeRa_OCC_Seasons_1-9.xls‎ |VeRa_OCC_Seasons_1-9.xls‎ ]]<br /> <br /> This file descibes all VeRa radio <br /> occultations carried out in the period 1/7/2006 - 2/6/2010. <br /> <br /> For further information contact the VeRa team: Martin Paetzold &lt;Martin.Paetzold@uni-koeln.de&gt;, Bernd Hauesler &lt;Bernd.Haeusler@unibw.de&gt;, and Silvia Tellmann &lt;tellmann@geo.uni-koeln.de&gt;<br /> <br /> :[[File:VeRa_Occultations_seasons_10-12.txt‎ ]]<br /> <br /> This file describes the future opportunities for Radio occultations in the upcoming occultation seasons in January 2011 - January 2012. <br /> File kindly provided by Stefan Remus, ESAC. <br /> <br /> For further information contact the VeRa team: Martin Paetzold <br /> &lt;Martin.Paetzold@uni-koeln.de&gt;, Bernd Hauesler <br /> &lt;Bernd.Haeusler@unibw.de&gt;, and Silvia Tellmann &lt;tellmann@geo.uni-koeln.de&gt;.<br /> <br /> === Akatsuki instruments ===<br /> <br /> [[File:Akatsuki_instruments.jpg|400px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> <br /> [http://www.jaxa.jp/countdown/f17/index_e.html Visit the Akatsuki Website]<br /> <br /> Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time) !<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about VCO/Akatsuki mission]<br /> <br /> * '''IR1''' : 1-micron Camera<br /> Low stratus, vapor, active volcanism<br /> <br /> 1.01 µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''' : 2-micron Camera<br /> Low stratus, trace gasses, zodiacal light<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65 µm<br /> <br /> * '''UVI''' : Ultraviolet Imager<br /> Cloud-top ultraviolet absorber, SO2<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''' : Longwave Infrared Camera<br /> Cloud-top temperature distribution<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''' : Lightning and Airglow Camera<br /> Lightening flash, high-stratus airglow emission<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> == Coordination meetings / meeting sessions==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/ « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris, June 28-29, 2010]<br /> * [http://www.venus.wisc.edu/workshop/ 2010 VEXAG International Workshop: Venus, Our Closest Earth-like Planet, Madison (USA), 30 August - 2 September 2010]<br /> <br /> <br /> == Other links==<br /> * [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=41012 Coordinated Ground-based Venus Observation Campaign]<br /> * [http://www.rssd.esa.int/index.php?project=VENUS Venus Ground-Based image Active Archive]<br /> <br /> The Venus ground-based image Active Archive (VAA) allows you to upload and retrieve ground-based Venus observations obtained in infrared, visual or ultraviolet light. The aim of this archive is to complement the ongoing Venus Express (VEX) spacecraft observations of Venus with worldwide ground-based images to allow for continuous monitoring of the planet.</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=269 2010-07-06T13:05:52Z

<p>Wikiadmin: /* Other links */</p> <hr /> <div>This wiki is provided as a tool to share information and schedules for the 2010 coordinated ground-based campaign of Venus. Please feel free to complete and modify the attached tables according to the campaign progress and your proposed observations. <br /> __TOC__<br /> <br /> ==Tools of the Venus coordinated campaign==<br /> ===Table===<br /> <br /> <br /> A list of proposed and actual observations : pre-conjunction (July 2010-Oct. 29, 2010), post conjunction (Oct. 29, 2010 - Feb. 2011)<br /> * [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination table]<br /> <br /> ===Map of observatory sites and telescopes ===<br /> <br /> Sites and telescopes used for ground-based observations, with a link to their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> ==Instrumentation of the study of Venus==<br /> === Ground-based instruments ===<br /> <br /> * Sunspot Astronomy &amp; Visitor Center<br /> APO 3.5-m<br /> <br /> ARCES<br /> <br /> * Observatorio SOAR<br /> Soar Telescope<br /> <br /> * Observatoire du Pic du Midi de Bigorre<br /> Bernard-Lyot 2-m<br /> <br /> * Osservatorio Astronomico della Regione Autonoma Valle d'Aosta<br /> <br /> * South African Astronomical Observatory<br /> Southern African Large Telescope (SALT)<br /> <br /> * Hanle Observatory<br /> HCT<br /> <br /> * National Central University Lulin Observatory<br /> LOT Cassegrain/ SLT R-C/ 4 TAOS robotic<br /> <br /> * Naroyo Observatory<br /> Naroyo 1.6-m<br /> <br /> * Siding Spring Observatory<br /> Anglo-Australian 3.9-m<br /> <br /> * Mount John University Observatory<br /> 1 m McLellan<br /> <br /> MOA 1.8-m<br /> <br /> 0.6-m Optical Craftsmen <br /> <br /> 0.6-m Boller &amp; Chivens<br /> <br /> * Mauna Kea Observatory<br /> IRTF <br /> <br /> Keck 10-m<br /> <br /> CFHT 3.6-m<br /> <br /> SUBARU<br /> <br /> JCMT<br /> <br /> * Haleakala Observatory<br /> AEOS<br /> <br /> * THIS Tuneable Heterodyne Infrared Spectrometer<br /> used at the:<br /> <br /> - McMath-Pierce Solar Telescope on Kitt Peak in Arizona<br /> <br /> - IRTF on Mauna Kea Hawaii<br /> <br /> * HIPWAC Heterodyne Instrument for Planetary Wind And Composition<br /> used at the:<br /> <br /> - IRTF<br /> <br /> === Venus Express instruments ===<br /> <br /> [[File:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> - VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> - VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> ==== VEx Files ====<br /> <br /> * SOIR Files:<br /> :[[File:SOIR_observation_list_until_Aug2010.xls‎|SOIR_observation_list_until_Aug2010.xls‎]]<br /> <br /> This file lists all SOIR observations made from the beginning of Venus operations (April 2006) <br /> until August 2010. <br /> <br /> For further details, contact the SOIR Principal Investigator: Ann-Carine Vandaele &lt;A-C.Vandaele@aeronomie.be&gt;<br /> <br /> :[[File:SOIR_MTP56-MTP70.xls|SOIR_MTP56-MTP70.xls]]<br /> <br /> This file desctibes SOIR solar occultation opportunities in the period 30/7/2010 - 25/8/2011. SOIR occultations allow measurement of gas abundances and temperatures in the 80-150 km altitude region. <br /> <br /> For further details, contact SOIR Principal Investigator: Ann-Carine Vandaele &lt;A-C.Vandaele@aeronomie.be&gt;.<br /> <br /> * VeRa Files:<br /> :[[File:VeRa_OCC_Seasons_1-9.xls‎ |VeRa_OCC_Seasons_1-9.xls‎ ]]<br /> <br /> This file descibes all VeRa radio <br /> occultations carried out in the period 1/7/2006 - 2/6/2010. <br /> <br /> For further information contact the VeRa team: Martin Paetzold &lt;Martin.Paetzold@uni-koeln.de&gt;, Bernd Hauesler &lt;Bernd.Haeusler@unibw.de&gt;, and Silvia Tellmann &lt;tellmann@geo.uni-koeln.de&gt;<br /> <br /> :[[File:VeRa_Occultations_seasons_10-12.txt‎ ]]<br /> <br /> This file describes the future opportunities for Radio occultations in the upcoming occultation seasons in January 2011 - January 2012. <br /> File kindly provided by Stefan Remus, ESAC. <br /> <br /> For further information contact the VeRa team: Martin Paetzold <br /> &lt;Martin.Paetzold@uni-koeln.de&gt;, Bernd Hauesler <br /> &lt;Bernd.Haeusler@unibw.de&gt;, and Silvia Tellmann &lt;tellmann@geo.uni-koeln.de&gt;.<br /> <br /> === Akatsuki instruments ===<br /> <br /> [[File:Akatsuki_instruments.jpg|400px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> <br /> [http://www.jaxa.jp/countdown/f17/index_e.html Visit the Akatsuki Website]<br /> <br /> Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time) !<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about VCO/Akatsuki mission]<br /> <br /> * '''IR1''' : 1-micron Camera<br /> Low stratus, vapor, active volcanism<br /> <br /> 1.01 µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''' : 2-micron Camera<br /> Low stratus, trace gasses, zodiacal light<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65 µm<br /> <br /> * '''UVI''' : Ultraviolet Imager<br /> Cloud-top ultraviolet absorber, SO2<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''' : Longwave Infrared Camera<br /> Cloud-top temperature distribution<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''' : Lightning and Airglow Camera<br /> Lightening flash, high-stratus airglow emission<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> == Coordination meetings / meeting sessions==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/ « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris, June 28-29, 2010]<br /> * [http://www.venus.wisc.edu/workshop/ 2010 VEXAG International Workshop: Venus, Our Closest Earth-like Planet, Madison (USA), 30 August - 2 September 2010]<br /> <br /> <br /> == Other links==<br /> * [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=41012 Coordinated Ground-based Venus Observation Campaign]<br /> * [http://www.rssd.esa.int/index.php?project=VENUS Venus Ground-Based image Active Archive]<br /> <br /> The Venus ground-based image Active Archive (VAA) allows you to upload and retrieve ground-based Venus observations obtained in infrared, visual or ultraviolet light. The aim of this archive is to complement the ongoing Venus Express (VEX) spacecraft observations of Venus with worldwide ground-based images to allow for continuous monitoring of the planet. <br /> <br /> * [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=38833 Venus Amateur Observing Project]</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus-atm:About&diff=268 2010-07-06T09:37:05Z

<p>Wikiadmin: </p> <hr /> <div>This page has been designed to allow scientists to communicate and coordinate their work on Venus. <br /> Indeed, it would be great for science if we put synergies between the different aspects of scientific studies.</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus-atm:About&diff=267 2010-07-06T09:33:45Z

<p>Wikiadmin: Created page with 'This page has been designed to allow scientists to communicate and coordinate their work on Venus. Indeed, science would benefit greatly if we put synergies between the differen…'</p> <hr /> <div>This page has been designed to allow scientists to communicate and coordinate their work on Venus. <br /> Indeed, science would benefit greatly if we put synergies between the different aspects of scientific studies.</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=File:Logovenus-atm.jpg&diff=266 2010-07-06T08:32:02Z

<p>Wikiadmin: </p> <hr /> <div></div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=File:Logo.jpg&diff=265 2010-07-06T08:22:02Z

<p>Wikiadmin: </p> <hr /> <div></div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=227 2010-05-28T14:44:55Z

<p>Wikiadmin: /* Ground-based coordination meetings / meeting sessions */</p> <hr /> <div>This wiki is provided as a tool to share information and schedules for the 2010 coordinated ground-based campaign of Venus. Please feel free to complete and modify the attached tables according to the campaign progress and your proposed observations. <br /> __TOC__<br /> <br /> ==Tools of the Venus coordinated campaign==<br /> ===Table===<br /> <br /> <br /> A list of proposed and actual observations : pre-conjunction (July 2010-Oct. 29, 2010), post conjunction (Oct. 29, 2010 - Feb. 2011)<br /> * [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination table]<br /> <br /> ===Map of observatory sites and telescopes ===<br /> <br /> Sites and telescopes used for ground-based observations, with a link to their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> ==Instrumentation of the study of Venus==<br /> === Ground-based instruments ===<br /> <br /> * Sunspot Astronomy &amp; Visitor Center<br /> APO 3.5-m<br /> <br /> ARCES<br /> <br /> * Observatorio SOAR<br /> Soar Telescope<br /> <br /> * Observatoire du Pic du Midi de Bigorre<br /> Bernard-Lyot 2-m<br /> <br /> * Osservatorio Astronomico della Regione Autonoma Valle d'Aosta<br /> Telescope?<br /> <br /> * South African Astronomical Observatory<br /> Southern African Large Telescope (SALT)<br /> <br /> * Hanle Observatory<br /> HCT<br /> <br /> * National Central University Lulin Observatory<br /> LOT Cassegrain/ SLT R-C/ 4 TAOS robotic<br /> <br /> * Naroyo Observatory<br /> Naroyo 1.6-m<br /> <br /> * Siding Spring Observatory<br /> Anglo-Australian 3.9-m<br /> <br /> * Mount John University Observatory<br /> 1 m McLellan<br /> <br /> MOA 1.8-m<br /> <br /> 0.6-m Optical Craftsmen <br /> <br /> 0.6-m Boller &amp; Chivens<br /> <br /> * Mauna Kea Observatory<br /> IRTF<br /> <br /> Keck 10-m<br /> <br /> CFHT 3.6-m<br /> <br /> SUBARU<br /> <br /> JCMT<br /> <br /> * Haleakala Observatory<br /> AEOS<br /> <br /> === Venus Express instruments ===<br /> <br /> [[Fichier:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> - VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> - VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> === Akatsuki instruments ===<br /> <br /> [[Fichier:Akatsuki_instruments.jpg|400px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> <br /> [http://www.jaxa.jp/countdown/f17/index_e.html Visit the Akatsuki Website]<br /> <br /> Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time) !<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about VCO/Akatsuki mission]<br /> <br /> * '''IR1''' : 1-micron Camera<br /> Low stratus, vapor, active volcanism<br /> <br /> 1.01 µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''' : 2-micron Camera<br /> Low stratus, trace gasses, zodiacal light<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65 µm<br /> <br /> * '''UVI''' : Ultraviolet Imager<br /> Cloud-top ultraviolet absorber, SO2<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''' : Longwave Infrared Camera<br /> Cloud-top temperature distribution<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''' : Lightning and Airglow Camera<br /> Lightening flash, high-stratus airglow emission<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> == Coordination meetings / meeting sessions==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/ « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris, June 28-29, 2010]</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=226 2010-05-28T14:29:09Z

<p>Wikiadmin: /* Table */</p> <hr /> <div>This wiki is provided as a tool to share information and schedules for the 2010 coordinated ground-based campaign of Venus. Please feel free to complete and modify the attached tables according to the campaign progress and your proposed observations. <br /> __TOC__<br /> <br /> ==Tools of the Venus coordinated campaign==<br /> ===Table===<br /> <br /> <br /> A list of proposed and actual observations : pre-conjunction (July 2010-Oct. 29, 2010), post conjunction (Oct. 29, 2010 - Feb. 2011)<br /> * [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination table]<br /> <br /> ===Map of observatory sites and telescopes ===<br /> <br /> Sites and telescopes used for ground-based observations, with a link to their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> ==Instrumentation of the study of Venus==<br /> === Ground-based instruments ===<br /> <br /> * Sunspot Astronomy &amp; Visitor Center<br /> APO 3.5-m<br /> <br /> ARCES<br /> <br /> * Observatorio SOAR<br /> Soar Telescope<br /> <br /> * Observatoire du Pic du Midi de Bigorre<br /> Bernard-Lyot 2-m<br /> <br /> * Osservatorio Astronomico della Regione Autonoma Valle d'Aosta<br /> Telescope?<br /> <br /> * South African Astronomical Observatory<br /> Southern African Large Telescope (SALT)<br /> <br /> * Hanle Observatory<br /> HCT<br /> <br /> * National Central University Lulin Observatory<br /> LOT Cassegrain/ SLT R-C/ 4 TAOS robotic<br /> <br /> * Naroyo Observatory<br /> Naroyo 1.6-m<br /> <br /> * Siding Spring Observatory<br /> Anglo-Australian 3.9-m<br /> <br /> * Mount John University Observatory<br /> 1 m McLellan<br /> <br /> MOA 1.8-m<br /> <br /> 0.6-m Optical Craftsmen <br /> <br /> 0.6-m Boller &amp; Chivens<br /> <br /> * Mauna Kea Observatory<br /> IRTF<br /> <br /> Keck 10-m<br /> <br /> CFHT 3.6-m<br /> <br /> SUBARU<br /> <br /> JCMT<br /> <br /> * Haleakala Observatory<br /> AEOS<br /> <br /> === Venus Express instruments ===<br /> <br /> [[Fichier:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> - VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> - VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> === Akatsuki instruments ===<br /> <br /> [[Fichier:Akatsuki_instruments.jpg|400px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> <br /> [http://www.jaxa.jp/countdown/f17/index_e.html Visit the Akatsuki Website]<br /> <br /> Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time) !<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about VCO/Akatsuki mission]<br /> <br /> * '''IR1''' : 1-micron Camera<br /> Low stratus, vapor, active volcanism<br /> <br /> 1.01 µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''' : 2-micron Camera<br /> Low stratus, trace gasses, zodiacal light<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65 µm<br /> <br /> * '''UVI''' : Ultraviolet Imager<br /> Cloud-top ultraviolet absorber, SO2<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''' : Longwave Infrared Camera<br /> Cloud-top temperature distribution<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''' : Lightning and Airglow Camera<br /> Lightening flash, high-stratus airglow emission<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> == Ground-based coordination meetings / meeting sessions==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/ « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris, June 28-29, 2010]</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=225 2010-05-28T14:28:30Z

<p>Wikiadmin: /* Table */</p> <hr /> <div>This wiki is provided as a tool to share information and schedules for the 2010 coordinated ground-based campaign of Venus. Please feel free to complete and modify the attached tables according to the campaign progress and your proposed observations. <br /> __TOC__<br /> <br /> ==Tools of the Venus coordinated campaign==<br /> ===Table===<br /> <br /> * [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination table]<br /> <br /> A list of proposed and actual observations : pre-conjunction (July 2010-Oct. 29, 2010), post conjunction (Oct. 29, 2010 - Feb. 2011)<br /> <br /> ===Map of observatory sites and telescopes ===<br /> <br /> Sites and telescopes used for ground-based observations, with a link to their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> ==Instrumentation of the study of Venus==<br /> === Ground-based instruments ===<br /> <br /> * Sunspot Astronomy &amp; Visitor Center<br /> APO 3.5-m<br /> <br /> ARCES<br /> <br /> * Observatorio SOAR<br /> Soar Telescope<br /> <br /> * Observatoire du Pic du Midi de Bigorre<br /> Bernard-Lyot 2-m<br /> <br /> * Osservatorio Astronomico della Regione Autonoma Valle d'Aosta<br /> Telescope?<br /> <br /> * South African Astronomical Observatory<br /> Southern African Large Telescope (SALT)<br /> <br /> * Hanle Observatory<br /> HCT<br /> <br /> * National Central University Lulin Observatory<br /> LOT Cassegrain/ SLT R-C/ 4 TAOS robotic<br /> <br /> * Naroyo Observatory<br /> Naroyo 1.6-m<br /> <br /> * Siding Spring Observatory<br /> Anglo-Australian 3.9-m<br /> <br /> * Mount John University Observatory<br /> 1 m McLellan<br /> <br /> MOA 1.8-m<br /> <br /> 0.6-m Optical Craftsmen <br /> <br /> 0.6-m Boller &amp; Chivens<br /> <br /> * Mauna Kea Observatory<br /> IRTF<br /> <br /> Keck 10-m<br /> <br /> CFHT 3.6-m<br /> <br /> SUBARU<br /> <br /> JCMT<br /> <br /> * Haleakala Observatory<br /> AEOS<br /> <br /> === Venus Express instruments ===<br /> <br /> [[Fichier:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> - VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> - VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> === Akatsuki instruments ===<br /> <br /> [[Fichier:Akatsuki_instruments.jpg|400px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> <br /> [http://www.jaxa.jp/countdown/f17/index_e.html Visit the Akatsuki Website]<br /> <br /> Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time) !<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about VCO/Akatsuki mission]<br /> <br /> * '''IR1''' : 1-micron Camera<br /> Low stratus, vapor, active volcanism<br /> <br /> 1.01 µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''' : 2-micron Camera<br /> Low stratus, trace gasses, zodiacal light<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65 µm<br /> <br /> * '''UVI''' : Ultraviolet Imager<br /> Cloud-top ultraviolet absorber, SO2<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''' : Longwave Infrared Camera<br /> Cloud-top temperature distribution<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''' : Lightning and Airglow Camera<br /> Lightening flash, high-stratus airglow emission<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> == Ground-based coordination meetings / meeting sessions==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/ « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris, June 28-29, 2010]</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=224 2010-05-28T14:27:37Z

<p>Wikiadmin: </p> <hr /> <div>This wiki is provided as a tool to share information and schedules for the 2010 coordinated ground-based campaign of Venus. Please feel free to complete and modify the attached tables according to the campaign progress and your proposed observations. <br /> __TOC__<br /> <br /> ==Tools of the Venus coordinated campaign==<br /> ===Table===<br /> <br /> [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination table]<br /> <br /> A list of proposed and actual observations : pre-conjunction (July 2010-Oct. 29, 2010), post conjunction (Oct. 29, 2010 - Feb. 2011)<br /> <br /> ===Map of observatory sites and telescopes ===<br /> <br /> Sites and telescopes used for ground-based observations, with a link to their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> ==Instrumentation of the study of Venus==<br /> === Ground-based instruments ===<br /> <br /> * Sunspot Astronomy &amp; Visitor Center<br /> APO 3.5-m<br /> <br /> ARCES<br /> <br /> * Observatorio SOAR<br /> Soar Telescope<br /> <br /> * Observatoire du Pic du Midi de Bigorre<br /> Bernard-Lyot 2-m<br /> <br /> * Osservatorio Astronomico della Regione Autonoma Valle d'Aosta<br /> Telescope?<br /> <br /> * South African Astronomical Observatory<br /> Southern African Large Telescope (SALT)<br /> <br /> * Hanle Observatory<br /> HCT<br /> <br /> * National Central University Lulin Observatory<br /> LOT Cassegrain/ SLT R-C/ 4 TAOS robotic<br /> <br /> * Naroyo Observatory<br /> Naroyo 1.6-m<br /> <br /> * Siding Spring Observatory<br /> Anglo-Australian 3.9-m<br /> <br /> * Mount John University Observatory<br /> 1 m McLellan<br /> <br /> MOA 1.8-m<br /> <br /> 0.6-m Optical Craftsmen <br /> <br /> 0.6-m Boller &amp; Chivens<br /> <br /> * Mauna Kea Observatory<br /> IRTF<br /> <br /> Keck 10-m<br /> <br /> CFHT 3.6-m<br /> <br /> SUBARU<br /> <br /> JCMT<br /> <br /> * Haleakala Observatory<br /> AEOS<br /> <br /> === Venus Express instruments ===<br /> <br /> [[Fichier:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> - VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> - VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> === Akatsuki instruments ===<br /> <br /> [[Fichier:Akatsuki_instruments.jpg|400px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> <br /> [http://www.jaxa.jp/countdown/f17/index_e.html Visit the Akatsuki Website]<br /> <br /> Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time) !<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about VCO/Akatsuki mission]<br /> <br /> * '''IR1''' : 1-micron Camera<br /> Low stratus, vapor, active volcanism<br /> <br /> 1.01 µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''' : 2-micron Camera<br /> Low stratus, trace gasses, zodiacal light<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65 µm<br /> <br /> * '''UVI''' : Ultraviolet Imager<br /> Cloud-top ultraviolet absorber, SO2<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''' : Longwave Infrared Camera<br /> Cloud-top temperature distribution<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''' : Lightning and Airglow Camera<br /> Lightening flash, high-stratus airglow emission<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> == Ground-based coordination meetings / meeting sessions==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/ « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris, June 28-29, 2010]</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=223 2010-05-28T14:09:02Z

<p>Wikiadmin: </p> <hr /> <div>This wiki is provided as a tool to share information and schedules for the 2010 coordinated ground-based campaign of Venus. Please feel free to complete and modify the attached tables according to the campaign progress and your proposed observations. <br /> __TOC__<br /> <br /> ==Tools of the Venus coordinated campaign==<br /> ===Table===<br /> <br /> [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination table]<br /> <br /> A list of proposed and actual observations : pre-conjunction (July 2010-Oct. 29, 2010), post conjunction (Oct. 29, 2010 - Feb. 2011)<br /> <br /> ===Map of observatory sites and telescopes ===<br /> <br /> Sites and telescopes used for ground-based observations, with a link to their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> == Ground-based instruments ==<br /> <br /> * Sunspot Astronomy &amp; Visitor Center<br /> APO 3.5-m<br /> <br /> ARCES<br /> <br /> * Observatorio SOAR<br /> Soar Telescope<br /> <br /> * Observatoire du Pic du Midi de Bigorre<br /> Bernard-Lyot 2-m<br /> <br /> * Osservatorio Astronomico della Regione Autonoma Valle d'Aosta<br /> Telescope?<br /> <br /> * South African Astronomical Observatory<br /> Southern African Large Telescope (SALT)<br /> <br /> * Hanle Observatory<br /> HCT<br /> <br /> * National Central University Lulin Observatory<br /> LOT Cassegrain/ SLT R-C/ 4 TAOS robotic<br /> <br /> * Naroyo Observatory<br /> Naroyo 1.6-m<br /> <br /> * Siding Spring Observatory<br /> Anglo-Australian 3.9-m<br /> <br /> * Mount John University Observatory<br /> 1 m McLellan<br /> <br /> MOA 1.8-m<br /> <br /> 0.6-m Optical Craftsmen <br /> <br /> 0.6-m Boller &amp; Chivens<br /> <br /> * Mauna Kea Observatory<br /> IRTF<br /> <br /> Keck 10-m<br /> <br /> CFHT 3.6-m<br /> <br /> SUBARU<br /> <br /> JCMT<br /> <br /> * Haleakala Observatory<br /> AEOS<br /> <br /> == Venus Express instruments ==<br /> <br /> [[Fichier:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> - VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> - VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> == Akatsuki instruments ==<br /> <br /> [[Fichier:Akatsuki_instruments.jpg|400px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> <br /> [http://www.jaxa.jp/countdown/f17/index_e.html Visit the Akatsuki Website]<br /> <br /> Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time) !<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about VCO/Akatsuki mission]<br /> <br /> * '''IR1''' : 1-micron Camera<br /> Low stratus, vapor, active volcanism<br /> <br /> 1.01 µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''' : 2-micron Camera<br /> Low stratus, trace gasses, zodiacal light<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65 µm<br /> <br /> * '''UVI''' : Ultraviolet Imager<br /> Cloud-top ultraviolet absorber, SO2<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''' : Longwave Infrared Camera<br /> Cloud-top temperature distribution<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''' : Lightning and Airglow Camera<br /> Lightening flash, high-stratus airglow emission<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> == Ground-based coordination meetings / meeting sessions==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/ « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris, June 28-29, 2010]</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=222 2010-05-28T13:52:47Z

<p>Wikiadmin: </p> <hr /> <div>This wiki is provided as a tool to share information and schedules for the 2010 coordinated ground-based campaign of Venus. Please feel free to complete and modify the attached tables according to the campaign progress and your proposed observations. <br /> __TOC__<br /> <br /> ==Table==<br /> <br /> [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination table]<br /> <br /> A list of proposed and actual observations : pre-conjunction (July 2010-Oct. 29, 2010), post conjunction (Oct. 29, 2010 - Feb. 2011)<br /> <br /> ==Map of observatory sites and telescopes ==<br /> <br /> Sites and telescopes used for ground-based observations, with a link to their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> == Ground-based instruments ==<br /> <br /> * Sunspot Astronomy &amp; Visitor Center<br /> APO 3.5-m<br /> <br /> ARCES<br /> <br /> * Observatorio SOAR<br /> Soar Telescope<br /> <br /> * Observatoire du Pic du Midi de Bigorre<br /> Bernard-Lyot 2-m<br /> <br /> * Osservatorio Astronomico della Regione Autonoma Valle d'Aosta<br /> Telescope?<br /> <br /> * South African Astronomical Observatory<br /> Southern African Large Telescope (SALT)<br /> <br /> * Hanle Observatory<br /> HCT<br /> <br /> * National Central University Lulin Observatory<br /> LOT Cassegrain/ SLT R-C/ 4 TAOS robotic<br /> <br /> * Naroyo Observatory<br /> Naroyo 1.6-m<br /> <br /> * Siding Spring Observatory<br /> Anglo-Australian 3.9-m<br /> <br /> * Mount John University Observatory<br /> 1 m McLellan<br /> <br /> MOA 1.8-m<br /> <br /> 0.6-m Optical Craftsmen <br /> <br /> 0.6-m Boller &amp; Chivens<br /> <br /> * Mauna Kea Observatory<br /> IRTF<br /> <br /> Keck 10-m<br /> <br /> CFHT 3.6-m<br /> <br /> SUBARU<br /> <br /> JCMT<br /> <br /> * Haleakala Observatory<br /> AEOS<br /> <br /> == Venus Express instruments ==<br /> <br /> [[Fichier:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> - VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> - VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> == Akatsuki instruments ==<br /> <br /> [[Fichier:Akatsuki_instruments.jpg|400px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> <br /> [http://www.jaxa.jp/countdown/f17/index_e.html Visit the Akatsuki Website]<br /> <br /> Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time) !<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about VCO/Akatsuki mission]<br /> <br /> * '''IR1''' : 1-micron Camera<br /> Low stratus, vapor, active volcanism<br /> <br /> 1.01 µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''' : 2-micron Camera<br /> Low stratus, trace gasses, zodiacal light<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65 µm<br /> <br /> * '''UVI''' : Ultraviolet Imager<br /> Cloud-top ultraviolet absorber, SO2<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''' : Longwave Infrared Camera<br /> Cloud-top temperature distribution<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''' : Lightning and Airglow Camera<br /> Lightening flash, high-stratus airglow emission<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> == Ground-based coordination meetings / meeting sessions==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/ « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris, June 28-29, 2010]</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=221 2010-05-26T09:50:15Z

<p>Wikiadmin: /* Ground-based instruments */</p> <hr /> <div>This wiki is provided as a tool to share information and schedules for the 2010 coordinated ground-based campaign of Venus. Please feel free to complete and modify the attached tables according to the campaign progress and your proposed observations. <br /> __TOC__<br /> <br /> ==Table==<br /> <br /> [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination table]<br /> <br /> A list of proposed and actual observations : pre-conjunction (July 2010-Oct. 29, 2010), post conjunction (Oct. 29, 2010 - Feb. 2011)<br /> <br /> ==Map of observatory sites and telescopes ==<br /> <br /> Sites and telescopes used for ground-based observations, with a link to their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> == Ground-based instruments ==<br /> <br /> * Sunspot Astronomy &amp; Visitor Center<br /> APO 3.5-m<br /> <br /> ARCES<br /> <br /> * Observatorio SOAR<br /> Soar Telescope<br /> <br /> * Observatoire du Pic du Midi de Bigorre<br /> Bernard-Lyot 2-m<br /> <br /> * Osservatorio Astronomico della Regione Autonoma Valle d'Aosta<br /> Telescope?<br /> <br /> * South African Astronomical Observatory<br /> Southern African Large Telescope (SALT)<br /> <br /> * Hanle Observatory<br /> HCT<br /> <br /> * National Central University Lulin Observatory<br /> LOT Cassegrain/ SLT R-C/ 4 TAOS robotic<br /> <br /> * Naroyo Observatory<br /> Naroyo 1.6-m<br /> <br /> * Siding Spring Observatory<br /> Anglo-Australian 3.9-m<br /> <br /> * Mount John University Observatory<br /> 1 m McLellan<br /> <br /> MOA 1.8-m<br /> <br /> 0.6-m Optical Craftsmen <br /> <br /> 0.6-m Boller &amp; Chivens<br /> <br /> * Mauna Kea Observatory<br /> IRTF<br /> <br /> Keck 10-m<br /> <br /> CFHT 3.6-m<br /> <br /> SUBARU<br /> <br /> JCMT<br /> <br /> * Haleakala Observatory<br /> AEOS<br /> <br /> == Venus Express instruments ==<br /> <br /> [[Fichier:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> - VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> - VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> == Akatsuki instruments ==<br /> <br /> [[Fichier:Akatsuki_instruments.jpg|400px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> <br /> [http://www.jaxa.jp/countdown/f17/index_e.html Visit the Akatsuki Website]<br /> <br /> Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time) !<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about VCO/Akatsuki mission]<br /> <br /> * '''IR1''' : 1-micron Camera<br /> Low stratus, vapor, active volcanism<br /> <br /> 1.01 µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''' : 2-micron Camera<br /> Low stratus, trace gasses, zodiacal light<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65 µm<br /> <br /> * '''UVI''' : Ultraviolet Imager<br /> Cloud-top ultraviolet absorber, SO2<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''' : Longwave Infrared Camera<br /> Cloud-top temperature distribution<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''' : Lightning and Airglow Camera<br /> Lightening flash, high-stratus airglow emission<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> == Ground-based coordination meetings / meeting sessions==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/ « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris Observatory, June 28-29, 2010]</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=220 2010-05-26T09:48:18Z

<p>Wikiadmin: /* Ground-based instruments */</p> <hr /> <div>This wiki is provided as a tool to share information and schedules for the 2010 coordinated ground-based campaign of Venus. Please feel free to complete and modify the attached tables according to the campaign progress and your proposed observations. <br /> __TOC__<br /> <br /> ==Table==<br /> <br /> [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination table]<br /> <br /> A list of proposed and actual observations : pre-conjunction (July 2010-Oct. 29, 2010), post conjunction (Oct. 29, 2010 - Feb. 2011)<br /> <br /> ==Map of observatory sites and telescopes ==<br /> <br /> Sites and telescopes used for ground-based observations, with a link to their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> == Ground-based instruments ==<br /> <br /> * '''Sunspot Astronomy &amp; Visitor Center'''<br /> APO 3.5-m<br /> <br /> ARCES<br /> <br /> * '''Observatorio SOAR'''<br /> Soar Telescope<br /> <br /> * '''Observatoire du Pic du Midi de Bigorre'''<br /> Bernard-Lyot 2-m<br /> <br /> * '''Osservatorio Astronomico della Regione Autonoma Valle d'Aosta'''<br /> Telescope?<br /> <br /> * '''South African Astronomical Observatory'''<br /> Southern African Large Telescope (SALT)<br /> <br /> * '''Hanle Observatory'''<br /> HCT<br /> <br /> * '''National Central University Lulin Observatory'''<br /> LOT Cassegrain/ SLT R-C/ 4 TAOS robotic<br /> <br /> * '''Naroyo Observatory'''<br /> Naroyo 1.6-m<br /> <br /> * '''Siding Spring Observatory'''<br /> Anglo-Australian 3.9-m<br /> <br /> * '''Mount John University Observatory'''<br /> 1 m McLellan<br /> <br /> MOA 1.8-m<br /> <br /> 0.6-m Optical Craftsmen <br /> <br /> 0.6-m Boller &amp; Chivens<br /> <br /> * '''Mauna Kea Observatory'''<br /> IRTF<br /> <br /> Keck 10-m<br /> <br /> CFHT 3.6-m<br /> <br /> SUBARU<br /> <br /> JCMT<br /> <br /> * '''Haleakala Observatory'''<br /> AEOS<br /> <br /> == Venus Express instruments ==<br /> <br /> [[Fichier:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> - VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> - VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> == Akatsuki instruments ==<br /> <br /> [[Fichier:Akatsuki_instruments.jpg|400px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> <br /> [http://www.jaxa.jp/countdown/f17/index_e.html Visit the Akatsuki Website]<br /> <br /> Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time) !<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about VCO/Akatsuki mission]<br /> <br /> * '''IR1''' : 1-micron Camera<br /> Low stratus, vapor, active volcanism<br /> <br /> 1.01 µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''' : 2-micron Camera<br /> Low stratus, trace gasses, zodiacal light<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65 µm<br /> <br /> * '''UVI''' : Ultraviolet Imager<br /> Cloud-top ultraviolet absorber, SO2<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''' : Longwave Infrared Camera<br /> Cloud-top temperature distribution<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''' : Lightning and Airglow Camera<br /> Lightening flash, high-stratus airglow emission<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> == Ground-based coordination meetings / meeting sessions==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/ « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris Observatory, June 28-29, 2010]</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=219 2010-05-26T09:27:44Z

<p>Wikiadmin: /* Ground-based instruments */</p> <hr /> <div>This wiki is provided as a tool to share information and schedules for the 2010 coordinated ground-based campaign of Venus. Please feel free to complete and modify the attached tables according to the campaign progress and your proposed observations. <br /> __TOC__<br /> <br /> ==Table==<br /> <br /> [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination table]<br /> <br /> A list of proposed and actual observations : pre-conjunction (July 2010-Oct. 29, 2010), post conjunction (Oct. 29, 2010 - Feb. 2011)<br /> <br /> ==Map of observatory sites and telescopes ==<br /> <br /> Sites and telescopes used for ground-based observations, with a link to their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> == Ground-based instruments ==<br /> <br /> * Sunspot Astronomy &amp; Visitor Center<br /> APO 3.5-m<br /> <br /> ARCES<br /> <br /> * Observatorio SOAR<br /> Soar Telescope<br /> <br /> * Observatoire du Pic du Midi de Bigorre<br /> Bernard-Lyot 2-m<br /> <br /> * Osservatorio Astronomico della Regione Autonoma Valle d'Aosta<br /> Telescope?<br /> <br /> * South African Astronomical Observatory<br /> Southern African Large Telescope (SALT)<br /> <br /> * Hanle Observatory<br /> HCT<br /> <br /> * National Central University Lulin Observatory<br /> LOT Cassegrain/ SLT R-C/ 4 TAOS robotic<br /> <br /> * Naroyo Observatory<br /> Naroyo 1.6-m<br /> <br /> * Siding Spring Observatory<br /> Anglo-Australian 3.9-m<br /> <br /> * Mount John University Observatory<br /> 1 m McLellan<br /> <br /> MOA 1.8-m<br /> <br /> 0.6-m Optical Craftsmen <br /> <br /> 0.6-m Boller &amp; Chivens<br /> <br /> * Mauna Kea Observatory<br /> IRTF<br /> <br /> Keck 10-m<br /> <br /> CFHT 3.6-m<br /> <br /> SUBARU<br /> <br /> JCMT<br /> <br /> * Haleakala Observatory<br /> AEOS<br /> <br /> == Venus Express instruments ==<br /> <br /> [[Fichier:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> - VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> - VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> == Akatsuki instruments ==<br /> <br /> [[Fichier:Akatsuki_instruments.jpg|400px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> <br /> [http://www.jaxa.jp/countdown/f17/index_e.html Visit the Akatsuki Website]<br /> <br /> Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time) !<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about VCO/Akatsuki mission]<br /> <br /> * '''IR1''' : 1-micron Camera<br /> Low stratus, vapor, active volcanism<br /> <br /> 1.01 µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''' : 2-micron Camera<br /> Low stratus, trace gasses, zodiacal light<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65 µm<br /> <br /> * '''UVI''' : Ultraviolet Imager<br /> Cloud-top ultraviolet absorber, SO2<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''' : Longwave Infrared Camera<br /> Cloud-top temperature distribution<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''' : Lightning and Airglow Camera<br /> Lightening flash, high-stratus airglow emission<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> == Ground-based coordination meetings / meeting sessions==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/ « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris Observatory, June 28-29, 2010]</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=218 2010-05-26T09:23:57Z

<p>Wikiadmin: /* Ground-based instruments */</p> <hr /> <div>This wiki is provided as a tool to share information and schedules for the 2010 coordinated ground-based campaign of Venus. Please feel free to complete and modify the attached tables according to the campaign progress and your proposed observations. <br /> __TOC__<br /> <br /> ==Table==<br /> <br /> [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination table]<br /> <br /> A list of proposed and actual observations : pre-conjunction (July 2010-Oct. 29, 2010), post conjunction (Oct. 29, 2010 - Feb. 2011)<br /> <br /> ==Map of observatory sites and telescopes ==<br /> <br /> Sites and telescopes used for ground-based observations, with a link to their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> == Ground-based instruments ==<br /> <br /> * Sunspot Astronomy &amp; Visitor Center<br /> APO 3.5-m<br /> <br /> ARCES<br /> <br /> * Observatorio SOAR<br /> Soar Telescope<br /> <br /> * Observatoire du Pic du Midi de Bigorre<br /> Bernard-Lyot 2-m<br /> <br /> * Osservatorio Astronomico della Regione Autonoma Valle d'Aosta<br /> Telescope?<br /> <br /> * South African Astronomical Observatory<br /> Southern African Large Telescope (SALT)<br /> <br /> * Hanle Observatory<br /> HCT<br /> <br /> * National Central University Lulin Observatory<br /> LOT Cassegrain/ SLT R-C/ 4 TAOS robotic<br /> <br /> * Naroyo Observatory<br /> Naroyo 1.6-m<br /> <br /> * Siding Spring Observatory<br /> Anglo-Australian 3.9-m<br /> <br /> * Mount John University Observatory<br /> 1 m McLellan<br /> <br /> MOA 1.8-m<br /> <br /> 0.6-m Optical Craftsmen <br /> <br /> 0.6-m Boller &amp; Chivens<br /> <br /> * Mauna Kea Observatory<br /> IRTF<br /> <br /> Keck 10-m<br /> <br /> CFHT 3.6-m<br /> <br /> SUBARU<br /> <br /> JCMT<br /> <br /> == Venus Express instruments ==<br /> <br /> [[Fichier:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> - VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> - VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> == Akatsuki instruments ==<br /> <br /> [[Fichier:Akatsuki_instruments.jpg|400px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> <br /> [http://www.jaxa.jp/countdown/f17/index_e.html Visit the Akatsuki Website]<br /> <br /> Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time) !<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about VCO/Akatsuki mission]<br /> <br /> * '''IR1''' : 1-micron Camera<br /> Low stratus, vapor, active volcanism<br /> <br /> 1.01 µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''' : 2-micron Camera<br /> Low stratus, trace gasses, zodiacal light<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65 µm<br /> <br /> * '''UVI''' : Ultraviolet Imager<br /> Cloud-top ultraviolet absorber, SO2<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''' : Longwave Infrared Camera<br /> Cloud-top temperature distribution<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''' : Lightning and Airglow Camera<br /> Lightening flash, high-stratus airglow emission<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> == Ground-based coordination meetings / meeting sessions==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/ « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris Observatory, June 28-29, 2010]</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=217 2010-05-26T09:21:48Z

<p>Wikiadmin: /* Ground-based instruments */</p> <hr /> <div>This wiki is provided as a tool to share information and schedules for the 2010 coordinated ground-based campaign of Venus. Please feel free to complete and modify the attached tables according to the campaign progress and your proposed observations. <br /> __TOC__<br /> <br /> ==Table==<br /> <br /> [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination table]<br /> <br /> A list of proposed and actual observations : pre-conjunction (July 2010-Oct. 29, 2010), post conjunction (Oct. 29, 2010 - Feb. 2011)<br /> <br /> ==Map of observatory sites and telescopes ==<br /> <br /> Sites and telescopes used for ground-based observations, with a link to their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> == Ground-based instruments ==<br /> <br /> * Sunspot Astronomy &amp; Visitor Center<br /> APO 3.5-m<br /> <br /> ARCES<br /> <br /> * Siding Spring Observatory<br /> Anglo-Australian 3.9-m<br /> <br /> * Observatorio SOAR<br /> Soar Telescope<br /> <br /> * Observatoire du Pic du Midi de Bigorre<br /> Bernard-Lyot 2-m<br /> <br /> * Osservatorio Astronomico della Regione Autonoma Valle d'Aosta<br /> Telescope?<br /> <br /> * South African Astronomical Observatory<br /> Southern African Large Telescope (SALT)<br /> <br /> * Hanle Observatory<br /> HCT<br /> <br /> * National Central University Lulin Observatory<br /> LOT Cassegrain/ SLT R-C/ 4 TAOS robotic<br /> <br /> * Naroyo Observatory<br /> Naroyo 1.6-m<br /> <br /> * Mount John University Observatory<br /> 1 m McLellan<br /> <br /> MOA 1.8-m<br /> <br /> 0.6-m Optical Craftsmen <br /> <br /> 0.6-m Boller &amp; Chivens<br /> <br /> * Mauna Kea Observatory<br /> IRTF<br /> <br /> Keck 10-m<br /> <br /> CFHT 3.6-m<br /> <br /> SUBARU<br /> <br /> JCMT<br /> <br /> == Venus Express instruments ==<br /> <br /> [[Fichier:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> - VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> - VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> == Akatsuki instruments ==<br /> <br /> [[Fichier:Akatsuki_instruments.jpg|400px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> <br /> [http://www.jaxa.jp/countdown/f17/index_e.html Visit the Akatsuki Website]<br /> <br /> Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time) !<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about VCO/Akatsuki mission]<br /> <br /> * '''IR1''' : 1-micron Camera<br /> Low stratus, vapor, active volcanism<br /> <br /> 1.01 µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''' : 2-micron Camera<br /> Low stratus, trace gasses, zodiacal light<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65 µm<br /> <br /> * '''UVI''' : Ultraviolet Imager<br /> Cloud-top ultraviolet absorber, SO2<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''' : Longwave Infrared Camera<br /> Cloud-top temperature distribution<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''' : Lightning and Airglow Camera<br /> Lightening flash, high-stratus airglow emission<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> == Ground-based coordination meetings / meeting sessions==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/ « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris Observatory, June 28-29, 2010]</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=216 2010-05-26T09:18:49Z

<p>Wikiadmin: /* Ground-based instruments */</p> <hr /> <div>This wiki is provided as a tool to share information and schedules for the 2010 coordinated ground-based campaign of Venus. Please feel free to complete and modify the attached tables according to the campaign progress and your proposed observations. <br /> __TOC__<br /> <br /> ==Table==<br /> <br /> [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination table]<br /> <br /> A list of proposed and actual observations : pre-conjunction (July 2010-Oct. 29, 2010), post conjunction (Oct. 29, 2010 - Feb. 2011)<br /> <br /> ==Map of observatory sites and telescopes ==<br /> <br /> Sites and telescopes used for ground-based observations, with a link to their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> == Ground-based instruments ==<br /> <br /> * Sunspot Astronomy &amp; Visitor Center<br /> APO 3.5-m<br /> <br /> ARCES<br /> <br /> * Siding Spring Observatory<br /> Anglo-Australian 3.9-m<br /> <br /> * Observatorio SOAR<br /> Soar Telescope<br /> <br /> * Observatoire du Pic du Midi de Bigorre<br /> Bernard-Lyot 2-m<br /> <br /> * Osservatorio Astronomico della Regione Autonoma Valle d'Aosta<br /> Telescope?<br /> <br /> * South African Astronomical Observatory<br /> Southern African Large Telescope (SALT)<br /> <br /> * Hanle Observatory<br /> HCT<br /> <br /> * National Central University Lulin Observatory<br /> LOT Cassegrain/ SLT R-C/ 4 TAOS robotic<br /> <br /> * Naroyo Observatory<br /> Naroyo 1.6-m<br /> <br /> * Mount John University Observatory<br /> 1 m McLellan<br /> <br /> MOA 1.8-m<br /> <br /> 0.6-m Optical Craftsmen <br /> <br /> 0.6-m Boller &amp; Chivens<br /> <br /> == Venus Express instruments ==<br /> <br /> [[Fichier:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> - VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> - VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> == Akatsuki instruments ==<br /> <br /> [[Fichier:Akatsuki_instruments.jpg|400px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> <br /> [http://www.jaxa.jp/countdown/f17/index_e.html Visit the Akatsuki Website]<br /> <br /> Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time) !<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about VCO/Akatsuki mission]<br /> <br /> * '''IR1''' : 1-micron Camera<br /> Low stratus, vapor, active volcanism<br /> <br /> 1.01 µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''' : 2-micron Camera<br /> Low stratus, trace gasses, zodiacal light<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65 µm<br /> <br /> * '''UVI''' : Ultraviolet Imager<br /> Cloud-top ultraviolet absorber, SO2<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''' : Longwave Infrared Camera<br /> Cloud-top temperature distribution<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''' : Lightning and Airglow Camera<br /> Lightening flash, high-stratus airglow emission<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> == Ground-based coordination meetings / meeting sessions==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/ « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris Observatory, June 28-29, 2010]</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=215 2010-05-26T09:04:42Z

<p>Wikiadmin: /* Ground-based instruments */</p> <hr /> <div>This wiki is provided as a tool to share information and schedules for the 2010 coordinated ground-based campaign of Venus. Please feel free to complete and modify the attached tables according to the campaign progress and your proposed observations. <br /> __TOC__<br /> <br /> ==Table==<br /> <br /> [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination table]<br /> <br /> A list of proposed and actual observations : pre-conjunction (July 2010-Oct. 29, 2010), post conjunction (Oct. 29, 2010 - Feb. 2011)<br /> <br /> ==Map of observatory sites and telescopes ==<br /> <br /> Sites and telescopes used for ground-based observations, with a link to their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> == Ground-based instruments ==<br /> <br /> * Sunspot Astronomy &amp; Visitor Center<br /> APO 3.5-m<br /> <br /> ARCES<br /> <br /> * Siding Spring Observatory<br /> Anglo-Australian 3.9-m<br /> <br /> * Observatorio SOAR<br /> Soar Telescope<br /> <br /> * Observatoire du Pic du Midi de Bigorre<br /> Bernard-Lyot 2-m<br /> <br /> * Osservatorio Astronomico della Regione Autonoma Valle d'Aosta<br /> Telescope?<br /> <br /> * South African Astronomical Observatory<br /> Southern African Large Telescope (SALT)<br /> <br /> * Hanle Observatory<br /> HCT<br /> <br /> * National Central University Lulin Observatory<br /> LOT Cassegrain/ SLT R-C/ 4 TAOS robotic<br /> <br /> == Venus Express instruments ==<br /> <br /> [[Fichier:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> - VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> - VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> == Akatsuki instruments ==<br /> <br /> [[Fichier:Akatsuki_instruments.jpg|400px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> <br /> [http://www.jaxa.jp/countdown/f17/index_e.html Visit the Akatsuki Website]<br /> <br /> Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time) !<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about VCO/Akatsuki mission]<br /> <br /> * '''IR1''' : 1-micron Camera<br /> Low stratus, vapor, active volcanism<br /> <br /> 1.01 µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''' : 2-micron Camera<br /> Low stratus, trace gasses, zodiacal light<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65 µm<br /> <br /> * '''UVI''' : Ultraviolet Imager<br /> Cloud-top ultraviolet absorber, SO2<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''' : Longwave Infrared Camera<br /> Cloud-top temperature distribution<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''' : Lightning and Airglow Camera<br /> Lightening flash, high-stratus airglow emission<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> == Ground-based coordination meetings / meeting sessions==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/ « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris Observatory, June 28-29, 2010]</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=214 2010-05-26T09:04:06Z

<p>Wikiadmin: /* Ground-based instruments */</p> <hr /> <div>This wiki is provided as a tool to share information and schedules for the 2010 coordinated ground-based campaign of Venus. Please feel free to complete and modify the attached tables according to the campaign progress and your proposed observations. <br /> __TOC__<br /> <br /> ==Table==<br /> <br /> [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination table]<br /> <br /> A list of proposed and actual observations : pre-conjunction (July 2010-Oct. 29, 2010), post conjunction (Oct. 29, 2010 - Feb. 2011)<br /> <br /> ==Map of observatory sites and telescopes ==<br /> <br /> Sites and telescopes used for ground-based observations, with a link to their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> == Ground-based instruments ==<br /> <br /> * Sunspot Astronomy &amp; Visitor Center<br /> APO 3.5-m<br /> <br /> ARCES<br /> <br /> * Siding Spring Observatory<br /> Anglo-Australian 3.9-m<br /> <br /> * Observatorio SOAR<br /> Soar Telescope<br /> <br /> * Observatoire du Pic du Midi de Bigorre<br /> Bernard-Lyot 2-m<br /> <br /> * Osservatorio Astronomico della Regione Autonoma Valle d'Aosta<br /> Telescope?<br /> <br /> * South African Astronomical Observatory<br /> Southern African Large Telescope (SALT)<br /> <br /> * Hanle Observatory<br /> HCT<br /> <br /> *<br /> <br /> == Venus Express instruments ==<br /> <br /> [[Fichier:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> - VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> - VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> == Akatsuki instruments ==<br /> <br /> [[Fichier:Akatsuki_instruments.jpg|400px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> <br /> [http://www.jaxa.jp/countdown/f17/index_e.html Visit the Akatsuki Website]<br /> <br /> Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time) !<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about VCO/Akatsuki mission]<br /> <br /> * '''IR1''' : 1-micron Camera<br /> Low stratus, vapor, active volcanism<br /> <br /> 1.01 µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''' : 2-micron Camera<br /> Low stratus, trace gasses, zodiacal light<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65 µm<br /> <br /> * '''UVI''' : Ultraviolet Imager<br /> Cloud-top ultraviolet absorber, SO2<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''' : Longwave Infrared Camera<br /> Cloud-top temperature distribution<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''' : Lightning and Airglow Camera<br /> Lightening flash, high-stratus airglow emission<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> == Ground-based coordination meetings / meeting sessions==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/ « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris Observatory, June 28-29, 2010]</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=213 2010-05-25T15:15:23Z

<p>Wikiadmin: /* Ground-based coordination meetings / meeting sessions */</p> <hr /> <div>This wiki is provided as a tool to share information and schedules for the 2010 coordinated ground-based campaign of Venus. Please feel free to complete and modify the attached tables according to the campaign progress and your proposed observations. <br /> __TOC__<br /> <br /> ==Table==<br /> <br /> [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination table]<br /> <br /> A list of proposed and actual observations : pre-conjunction (July 2010-Oct. 29, 2010), post conjunction (Oct. 29, 2010 - Feb. 2011)<br /> <br /> ==Map of observatory sites and telescopes ==<br /> <br /> Sites and telescopes used for ground-based observations, with a link to their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> == Ground-based instruments ==<br /> <br /> == Venus Express instruments ==<br /> <br /> [[Fichier:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> - VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> - VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> == Akatsuki instruments ==<br /> <br /> [[Fichier:Akatsuki_instruments.jpg|400px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> <br /> [http://www.jaxa.jp/countdown/f17/index_e.html Visit the Akatsuki Website]<br /> <br /> Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time) !<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about VCO/Akatsuki mission]<br /> <br /> * '''IR1''' : 1-micron Camera<br /> Low stratus, vapor, active volcanism<br /> <br /> 1.01 µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''' : 2-micron Camera<br /> Low stratus, trace gasses, zodiacal light<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65 µm<br /> <br /> * '''UVI''' : Ultraviolet Imager<br /> Cloud-top ultraviolet absorber, SO2<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''' : Longwave Infrared Camera<br /> Cloud-top temperature distribution<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''' : Lightning and Airglow Camera<br /> Lightening flash, high-stratus airglow emission<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> == Ground-based coordination meetings / meeting sessions==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/ « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris Observatory, June 28-29, 2010]</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=212 2010-05-25T15:07:18Z

<p>Wikiadmin: /* Table */</p> <hr /> <div>This wiki is provided as a tool to share information and schedules for the 2010 coordinated ground-based campaign of Venus. Please feel free to complete and modify the attached tables according to the campaign progress and your proposed observations. <br /> __TOC__<br /> <br /> ==Table==<br /> <br /> [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination table]<br /> <br /> A list of proposed and actual observations : pre-conjunction (July 2010-Oct. 29, 2010), post conjunction (Oct. 29, 2010 - Feb. 2011)<br /> <br /> ==Map of observatory sites and telescopes ==<br /> <br /> Sites and telescopes used for ground-based observations, with a link to their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> == Ground-based instruments ==<br /> <br /> == Venus Express instruments ==<br /> <br /> [[Fichier:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> - VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> - VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> == Akatsuki instruments ==<br /> <br /> [[Fichier:Akatsuki_instruments.jpg|400px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> <br /> [http://www.jaxa.jp/countdown/f17/index_e.html Visit the Akatsuki Website]<br /> <br /> Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time) !<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about VCO/Akatsuki mission]<br /> <br /> * '''IR1''' : 1-micron Camera<br /> Low stratus, vapor, active volcanism<br /> <br /> 1.01 µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''' : 2-micron Camera<br /> Low stratus, trace gasses, zodiacal light<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65 µm<br /> <br /> * '''UVI''' : Ultraviolet Imager<br /> Cloud-top ultraviolet absorber, SO2<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''' : Longwave Infrared Camera<br /> Cloud-top temperature distribution<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''' : Lightning and Airglow Camera<br /> Lightening flash, high-stratus airglow emission<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> == Ground-based coordination meetings / meeting sessions==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/International « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris Observatory, June 28-29, 2010]</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=211 2010-05-25T15:06:39Z

<p>Wikiadmin: /* Akatsuki instruments */</p> <hr /> <div>This wiki is provided as a tool to share information and schedules for the 2010 coordinated ground-based campaign of Venus. Please feel free to complete and modify the attached tables according to the campaign progress and your proposed observations. <br /> __TOC__<br /> <br /> ==Table==<br /> <br /> [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination]<br /> <br /> A list of proposed and actual observations : pre-conjunction (July 2010-Oct. 29, 2010), post conjunction (Oct. 29, 2010 - Feb. 2011)<br /> <br /> ==Map of observatory sites and telescopes ==<br /> <br /> Sites and telescopes used for ground-based observations, with a link to their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> == Ground-based instruments ==<br /> <br /> == Venus Express instruments ==<br /> <br /> [[Fichier:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> - VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> - VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> == Akatsuki instruments ==<br /> <br /> [[Fichier:Akatsuki_instruments.jpg|400px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> <br /> [http://www.jaxa.jp/countdown/f17/index_e.html Visit the Akatsuki Website]<br /> <br /> Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time) !<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about VCO/Akatsuki mission]<br /> <br /> * '''IR1''' : 1-micron Camera<br /> Low stratus, vapor, active volcanism<br /> <br /> 1.01 µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''' : 2-micron Camera<br /> Low stratus, trace gasses, zodiacal light<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65 µm<br /> <br /> * '''UVI''' : Ultraviolet Imager<br /> Cloud-top ultraviolet absorber, SO2<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''' : Longwave Infrared Camera<br /> Cloud-top temperature distribution<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''' : Lightning and Airglow Camera<br /> Lightening flash, high-stratus airglow emission<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> == Ground-based coordination meetings / meeting sessions==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/International « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris Observatory, June 28-29, 2010]</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=210 2010-05-25T14:55:08Z

<p>Wikiadmin: /* Venus Express instruments */</p> <hr /> <div>This wiki is provided as a tool to share information and schedules for the 2010 coordinated ground-based campaign of Venus. Please feel free to complete and modify the attached tables according to the campaign progress and your proposed observations. <br /> __TOC__<br /> <br /> ==Table==<br /> <br /> [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination]<br /> <br /> A list of proposed and actual observations : pre-conjunction (July 2010-Oct. 29, 2010), post conjunction (Oct. 29, 2010 - Feb. 2011)<br /> <br /> ==Map of observatory sites and telescopes ==<br /> <br /> Sites and telescopes used for ground-based observations, with a link to their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> == Ground-based instruments ==<br /> <br /> == Venus Express instruments ==<br /> <br /> [[Fichier:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> - VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> - VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> == Akatsuki instruments ==<br /> <br /> [[Fichier:Akatsuki_instruments.jpg|400px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> <br /> [http://www.jaxa.jp/countdown/f17/index_e.html Visit the Akatsuki Website]<br /> <br /> Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time) !<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about VCO/Akatsuki mission]<br /> <br /> * '''IR1''' : 1-micron Camera<br /> Low stratus, vapor, active volcanism<br /> <br /> 1.01µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''' : 2-micron Camera<br /> Low stratus, trace gasses, zodiacal light<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65µm<br /> <br /> * '''UVI''' : Ultraviolet Imager<br /> Cloud-top ultraviolet absorber, SO2<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''' : Longwave Infrared Camera<br /> Cloud-top temperature distribution<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''' : Lightning and Airglow Camera<br /> Lightening flash, high-stratus airglow emission<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> == Ground-based coordination meetings / meeting sessions==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/International « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris Observatory, June 28-29, 2010]</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=209 2010-05-25T14:49:06Z

<p>Wikiadmin: /* Akatsuki instruments */</p> <hr /> <div>This wiki is provided as a tool to share information and schedules for the 2010 coordinated ground-based campaign of Venus. Please feel free to complete and modify the attached tables according to the campaign progress and your proposed observations. <br /> __TOC__<br /> <br /> ==Table==<br /> <br /> [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination]<br /> <br /> A list of proposed and actual observations : pre-conjunction (July 2010-Oct. 29, 2010), post conjunction (Oct. 29, 2010 - Feb. 2011)<br /> <br /> ==Map of observatory sites and telescopes ==<br /> <br /> Sites and telescopes used for ground-based observations, with a link to their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> == Ground-based instruments ==<br /> <br /> == Venus Express instruments ==<br /> <br /> [[Fichier:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> == Akatsuki instruments ==<br /> <br /> [[Fichier:Akatsuki_instruments.jpg|400px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> <br /> [http://www.jaxa.jp/countdown/f17/index_e.html Visit the Akatsuki Website]<br /> <br /> Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time) !<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about VCO/Akatsuki mission]<br /> <br /> * '''IR1''' : 1-micron Camera<br /> Low stratus, vapor, active volcanism<br /> <br /> 1.01µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''' : 2-micron Camera<br /> Low stratus, trace gasses, zodiacal light<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65µm<br /> <br /> * '''UVI''' : Ultraviolet Imager<br /> Cloud-top ultraviolet absorber, SO2<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''' : Longwave Infrared Camera<br /> Cloud-top temperature distribution<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''' : Lightning and Airglow Camera<br /> Lightening flash, high-stratus airglow emission<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> == Ground-based coordination meetings / meeting sessions==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/International « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris Observatory, June 28-29, 2010]</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=208 2010-05-25T14:34:07Z

<p>Wikiadmin: /* Akatsuki instruments */</p> <hr /> <div>This wiki is provided as a tool to share information and schedules for the 2010 coordinated ground-based campaign of Venus. Please feel free to complete and modify the attached tables according to the campaign progress and your proposed observations. <br /> __TOC__<br /> <br /> ==Table==<br /> <br /> [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination]<br /> <br /> A list of proposed and actual observations : pre-conjunction (July 2010-Oct. 29, 2010), post conjunction (Oct. 29, 2010 - Feb. 2011)<br /> <br /> ==Map of observatory sites and telescopes ==<br /> <br /> Sites and telescopes used for ground-based observations, with a link to their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> == Ground-based instruments ==<br /> <br /> == Venus Express instruments ==<br /> <br /> [[Fichier:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> == Akatsuki instruments ==<br /> <br /> [[Fichier:Akatsuki_instruments.jpg|400px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> <br /> [http://www.jaxa.jp/countdown/f17/index_e.html Visit the Akatsuki Website]<br /> <br /> Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time) !<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about VCO/Akatsuki mission]<br /> <br /> * '''IR1''' : 1-micron Camera<br /> <br /> 1.01µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''' : 2-micron Camera<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65µm<br /> <br /> * '''UVI''' : Ultraviolet Imager<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''' : Longwave Infrared Camera<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''' : Lightning and Airglow Camera<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> == Ground-based coordination meetings / meeting sessions==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/International « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris Observatory, June 28-29, 2010]</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=207 2010-05-25T14:33:17Z

<p>Wikiadmin: /* Akatsuki instruments */</p> <hr /> <div>This wiki is provided as a tool to share information and schedules for the 2010 coordinated ground-based campaign of Venus. Please feel free to complete and modify the attached tables according to the campaign progress and your proposed observations. <br /> __TOC__<br /> <br /> ==Table==<br /> <br /> [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination]<br /> <br /> A list of proposed and actual observations : pre-conjunction (July 2010-Oct. 29, 2010), post conjunction (Oct. 29, 2010 - Feb. 2011)<br /> <br /> ==Map of observatory sites and telescopes ==<br /> <br /> Sites and telescopes used for ground-based observations, with a link to their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> == Ground-based instruments ==<br /> <br /> == Venus Express instruments ==<br /> <br /> [[Fichier:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> == Akatsuki instruments ==<br /> <br /> [[Fichier:Akatsuki_instruments.jpg|400px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> <br /> [http://www.jaxa.jp/countdown/f17/index_e.html Visit the Akatsuki Website]<br /> <br /> Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time) !<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about VCO/Akatsuki mission]<br /> <br /> * '''IR1''': 1-micron Camera<br /> <br /> 1.01µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''': 2-micron Camera<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65µm<br /> <br /> * '''UVI''': Ultraviolet Imager<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''': Longwave Infrared Camera<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''': Lightning and Airglow Camera<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> == Ground-based coordination meetings / meeting sessions==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/International « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris Observatory, June 28-29, 2010]</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=206 2010-05-25T14:29:16Z

<p>Wikiadmin: /* Akatsuki instruments */</p> <hr /> <div>This wiki is provided as a tool to share information and schedules for the 2010 coordinated ground-based campaign of Venus. Please feel free to complete and modify the attached tables according to the campaign progress and your proposed observations. <br /> __TOC__<br /> <br /> ==Table==<br /> <br /> [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination]<br /> <br /> A list of proposed and actual observations : pre-conjunction (July 2010-Oct. 29, 2010), post conjunction (Oct. 29, 2010 - Feb. 2011)<br /> <br /> ==Map of observatory sites and telescopes ==<br /> <br /> Sites and telescopes used for ground-based observations, with a link to their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> == Ground-based instruments ==<br /> <br /> == Venus Express instruments ==<br /> <br /> [[Fichier:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> == Akatsuki instruments ==<br /> [http://www.jaxa.jp/countdown/f17/index_e.html Visit the Akatsuki Website]<br /> <br /> [[Fichier:Akatsuki_instruments.jpg|400px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> <br /> Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time) !<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about VCO/Akatsuki mission]<br /> <br /> * '''IR1''': 1-micron Camera<br /> <br /> 1.01µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''': 2-micron Camera<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65µm<br /> <br /> * '''UVI''': Ultraviolet Imager<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''': Longwave Infrared Camera<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''': Lightning and Airglow Camera<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> == Ground-based coordination meetings / meeting sessions==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/International « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris Observatory, June 28-29, 2010]</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=205 2010-05-25T14:28:57Z

<p>Wikiadmin: /* Akatsuki instruments */</p> <hr /> <div>This wiki is provided as a tool to share information and schedules for the 2010 coordinated ground-based campaign of Venus. Please feel free to complete and modify the attached tables according to the campaign progress and your proposed observations. <br /> __TOC__<br /> <br /> ==Table==<br /> <br /> [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination]<br /> <br /> A list of proposed and actual observations : pre-conjunction (July 2010-Oct. 29, 2010), post conjunction (Oct. 29, 2010 - Feb. 2011)<br /> <br /> ==Map of observatory sites and telescopes ==<br /> <br /> Sites and telescopes used for ground-based observations, with a link to their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> == Ground-based instruments ==<br /> <br /> == Venus Express instruments ==<br /> <br /> [[Fichier:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> == Akatsuki instruments ==<br /> [http://www.jaxa.jp/countdown/f17/index_e.html Visit the Akatsuki Website]<br /> <br /> [[Fichier:Akatsuki_instruments.jpg|300px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> <br /> Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time) !<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about VCO/Akatsuki mission]<br /> <br /> * '''IR1''': 1-micron Camera<br /> <br /> 1.01µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''': 2-micron Camera<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65µm<br /> <br /> * '''UVI''': Ultraviolet Imager<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''': Longwave Infrared Camera<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''': Lightning and Airglow Camera<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> == Ground-based coordination meetings / meeting sessions==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/International « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris Observatory, June 28-29, 2010]</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=204 2010-05-25T14:28:13Z

<p>Wikiadmin: /* Akatsuki instruments */</p> <hr /> <div>This wiki is provided as a tool to share information and schedules for the 2010 coordinated ground-based campaign of Venus. Please feel free to complete and modify the attached tables according to the campaign progress and your proposed observations. <br /> __TOC__<br /> <br /> ==Table==<br /> <br /> [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination]<br /> <br /> A list of proposed and actual observations : pre-conjunction (July 2010-Oct. 29, 2010), post conjunction (Oct. 29, 2010 - Feb. 2011)<br /> <br /> ==Map of observatory sites and telescopes ==<br /> <br /> Sites and telescopes used for ground-based observations, with a link to their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> == Ground-based instruments ==<br /> <br /> == Venus Express instruments ==<br /> <br /> [[Fichier:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> == Akatsuki instruments ==<br /> [http://www.jaxa.jp/countdown/f17/index_e.html Visit the Akatsuki Website]<br /> <br /> Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time) !<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about VCO/Akatsuki mission]<br /> <br /> [[Fichier:Akatsuki_instruments.jpg|300px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> <br /> * '''IR1''': 1-micron Camera<br /> <br /> 1.01µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''': 2-micron Camera<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65µm<br /> <br /> * '''UVI''': Ultraviolet Imager<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''': Longwave Infrared Camera<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''': Lightning and Airglow Camera<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> == Ground-based coordination meetings / meeting sessions==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/International « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris Observatory, June 28-29, 2010]</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=203 2010-05-25T14:24:29Z

<p>Wikiadmin: /* Akatsuki instruments */</p> <hr /> <div>This wiki is provided as a tool to share information and schedules for the 2010 coordinated ground-based campaign of Venus. Please feel free to complete and modify the attached tables according to the campaign progress and your proposed observations. <br /> __TOC__<br /> <br /> ==Table==<br /> <br /> [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination]<br /> <br /> A list of proposed and actual observations : pre-conjunction (July 2010-Oct. 29, 2010), post conjunction (Oct. 29, 2010 - Feb. 2011)<br /> <br /> ==Map of observatory sites and telescopes ==<br /> <br /> Sites and telescopes used for ground-based observations, with a link to their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> == Ground-based instruments ==<br /> <br /> == Venus Express instruments ==<br /> <br /> [[Fichier:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> == Akatsuki instruments ==<br /> [http://www.jaxa.jp/countdown/f17/index_e.html Visit the Akatsuki Website]<br /> <br /> Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time) !<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about VCO/Akatsuki mission]<br /> <br /> [[Fichier:Akatsuki_instrumentation.gif|300px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> [[Fichier:Akatsuki_instruments.jpg|300px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> <br /> * '''IR1''': 1-micron Camera<br /> <br /> 1.01µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''': 2-micron Camera<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65µm<br /> <br /> * '''UVI''': Ultraviolet Imager<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''': Longwave Infrared Camera<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''': Lightning and Airglow Camera<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> == Ground-based coordination meetings / meeting sessions==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/International « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris Observatory, June 28-29, 2010]</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=File:Akatsuki_instruments.jpg&diff=202 2010-05-25T14:23:07Z

<p>Wikiadmin: </p> <hr /> <div></div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=201 2010-05-25T14:13:13Z

<p>Wikiadmin: /* Akatsuki instruments */</p> <hr /> <div>This wiki is provided as a tool to share information and schedules for the 2010 coordinated ground-based campaign of Venus. Please feel free to complete and modify the attached tables according to the campaign progress and your proposed observations. <br /> __TOC__<br /> <br /> ==Table==<br /> <br /> [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination]<br /> <br /> A list of proposed and actual observations : pre-conjunction (July 2010-Oct. 29, 2010), post conjunction (Oct. 29, 2010 - Feb. 2011)<br /> <br /> ==Map of observatory sites and telescopes ==<br /> <br /> Sites and telescopes used for ground-based observations, with a link to their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> == Ground-based instruments ==<br /> <br /> == Venus Express instruments ==<br /> <br /> [[Fichier:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> == Akatsuki instruments ==<br /> [http://www.jaxa.jp/countdown/f17/index_e.html Visit the Akatsuki Website]<br /> <br /> Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time) !<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about VCO/Akatsuki mission]<br /> <br /> [[Fichier:Akatsuki_instrumentation.gif|350px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> <br /> * '''IR1''': 1-micron Camera<br /> <br /> 1.01µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''': 2-micron Camera<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65µm<br /> <br /> * '''UVI''': Ultraviolet Imager<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''': Longwave Infrared Camera<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''': Lightning and Airglow Camera<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> == Ground-based coordination meetings / meeting sessions==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/International « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris Observatory, June 28-29, 2010]</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=200 2010-05-25T14:09:42Z

<p>Wikiadmin: /* Akatsuki instruments */</p> <hr /> <div>This wiki is provided as a tool to share information and schedules for the 2010 coordinated ground-based campaign of Venus. Please feel free to complete and modify the attached tables according to the campaign progress and your proposed observations. <br /> __TOC__<br /> <br /> ==Table==<br /> <br /> [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination]<br /> <br /> A list of proposed and actual observations : pre-conjunction (July 2010-Oct. 29, 2010), post conjunction (Oct. 29, 2010 - Feb. 2011)<br /> <br /> ==Map of observatory sites and telescopes ==<br /> <br /> Sites and telescopes used for ground-based observations, with a link to their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> == Ground-based instruments ==<br /> <br /> == Venus Express instruments ==<br /> <br /> [[Fichier:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> == Akatsuki instruments ==<br /> [http://www.jaxa.jp/projects/sat/planet_c/index_e.html Visit the Akatsuki Website]<br /> <br /> Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time) !<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about VCO/Akatsuki mission]<br /> <br /> [[Fichier:Akatsuki_instrumentation.gif|350px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> <br /> * '''IR1''': 1-micron Camera<br /> <br /> 1.01µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''': 2-micron Camera<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65µm<br /> <br /> * '''UVI''': Ultraviolet Imager<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''': Longwave Infrared Camera<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''': Lightning and Airglow Camera<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> == Ground-based coordination meetings / meeting sessions==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/International « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris Observatory, June 28-29, 2010]</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=199 2010-05-25T14:07:40Z

<p>Wikiadmin: /* Akatsuki instruments */</p> <hr /> <div>This wiki is provided as a tool to share information and schedules for the 2010 coordinated ground-based campaign of Venus. Please feel free to complete and modify the attached tables according to the campaign progress and your proposed observations. <br /> __TOC__<br /> <br /> ==Table==<br /> <br /> [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination]<br /> <br /> A list of proposed and actual observations : pre-conjunction (July 2010-Oct. 29, 2010), post conjunction (Oct. 29, 2010 - Feb. 2011)<br /> <br /> ==Map of observatory sites and telescopes ==<br /> <br /> Sites and telescopes used for ground-based observations, with a link to their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> == Ground-based instruments ==<br /> <br /> == Venus Express instruments ==<br /> <br /> [[Fichier:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> == Akatsuki instruments ==<br /> <br /> Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time) !<br /> <br /> [http://www.jaxa.jp/projects/sat/planet_c/index_e.html Visit the Akatsuki Website]<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about VCO/Akatsuki mission]<br /> <br /> [[Fichier:Akatsuki_instrumentation.gif|350px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> <br /> * '''IR1''': 1-micron Camera<br /> <br /> 1.01µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''': 2-micron Camera<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65µm<br /> <br /> * '''UVI''': Ultraviolet Imager<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''': Longwave Infrared Camera<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''': Lightning and Airglow Camera<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> == Ground-based coordination meetings / meeting sessions==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/International « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris Observatory, June 28-29, 2010]</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=198 2010-05-25T13:52:19Z

<p>Wikiadmin: /* Venus Express instruments = */</p> <hr /> <div>This wiki is provided as a tool to share information and schedules for the 2010 coordinated ground-based campaign of Venus. Please feel free to complete and modify the attached tables according to the campaign progress and your proposed observations. <br /> __TOC__<br /> <br /> ==Table==<br /> <br /> [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination]<br /> <br /> A list of proposed and actual observations : pre-conjunction (July 2010-Oct. 29, 2010), post conjunction (Oct. 29, 2010 - Feb. 2011)<br /> <br /> ==Map of observatory sites and telescopes ==<br /> <br /> Sites and telescopes used for ground-based observations, with a link to their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> == Ground-based instruments ==<br /> <br /> == Venus Express instruments ==<br /> <br /> [[Fichier:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> == Akatsuki instruments ==<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about VCO/Akatsuki mission]<br /> <br /> Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time) !<br /> <br /> [http://www.jaxa.jp/projects/sat/planet_c/index_e.html Visit the Akatsuki Website]<br /> <br /> [[Fichier:Akatsuki_instrumentation.gif|350px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> <br /> * '''IR1''': 1-micron Camera<br /> <br /> 1.01µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''': 2-micron Camera<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65µm<br /> <br /> * '''UVI''': Ultraviolet Imager<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''': Longwave Infrared Camera<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''': Lightning and Airglow Camera<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> == Ground-based coordination meetings / meeting sessions==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/International « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris Observatory, June 28-29, 2010]</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=197 2010-05-25T13:51:52Z

<p>Wikiadmin: /* Ground-based instruments = */</p> <hr /> <div>This wiki is provided as a tool to share information and schedules for the 2010 coordinated ground-based campaign of Venus. Please feel free to complete and modify the attached tables according to the campaign progress and your proposed observations. <br /> __TOC__<br /> <br /> ==Table==<br /> <br /> [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination]<br /> <br /> A list of proposed and actual observations : pre-conjunction (July 2010-Oct. 29, 2010), post conjunction (Oct. 29, 2010 - Feb. 2011)<br /> <br /> ==Map of observatory sites and telescopes ==<br /> <br /> Sites and telescopes used for ground-based observations, with a link to their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> == Ground-based instruments ==<br /> <br /> == Venus Express instruments ===<br /> <br /> [[Fichier:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> == Akatsuki instruments ==<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about VCO/Akatsuki mission]<br /> <br /> Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time) !<br /> <br /> [http://www.jaxa.jp/projects/sat/planet_c/index_e.html Visit the Akatsuki Website]<br /> <br /> [[Fichier:Akatsuki_instrumentation.gif|350px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> <br /> * '''IR1''': 1-micron Camera<br /> <br /> 1.01µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''': 2-micron Camera<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65µm<br /> <br /> * '''UVI''': Ultraviolet Imager<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''': Longwave Infrared Camera<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''': Lightning and Airglow Camera<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> == Ground-based coordination meetings / meeting sessions==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/International « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris Observatory, June 28-29, 2010]</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=193 2010-05-21T14:10:44Z

<p>Wikiadmin: /* Akatsuki */</p> <hr /> <div>This site is intended as a tool to share information, comments and schedules for preparing the 2010 coordinated campaign of ground-based observations in the context of Venus Express and coming launch of Akatsuki mission.<br /> <br /> The attached Google docs can be completed and modified according to the campaign progress. <br /> __TOC__<br /> <br /> <br /> ==Table==<br /> <br /> To prepare the campaign and coordinate telescope proposals with VEx MTPs, the attached table is under construction. Please do not hesitate to comment/modify and add more details on your plans.<br /> <br /> [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination]<br /> <br /> ==Map (under construction) ==<br /> <br /> To have a general view of the sites and telescopes which are used for ground-based observations of Venus, see this googlemap for an overview for all of the different observatories and their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> <br /> == In-orbit observations ==<br /> <br /> <br /> === Venus Express ===<br /> <br /> <br /> ==== Instruments ====<br /> <br /> [[Fichier:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> === Akatsuki ===<br /> <br /> * Goals: Akatsuki is designed to study Venus' climate using ultraviolet and infrared cameras. The spacecraft will follow orbit Venus following the westware rotation of the atmosphere, mapping the circulation and vertical structure of the planet's thick clouds. The mission will complement the ESA's Venus Express, which also explores the Venusian environment with different approaches.<br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about the project]<br /> <br /> * Accomplishments: The mission is in development.<br /> <br /> Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time)!<br /> <br /> [http://www.jaxa.jp/projects/sat/planet_c/index_e.html Visit the Akatsuki Website]<br /> <br /> ==== Instruments====<br /> [[Fichier:Akatsuki_instrumentation.gif|350px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> * '''IR1''': 1-micron Camera<br /> <br /> 1.01µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''': 2-micron Camera<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65µm<br /> <br /> * '''UVI''': Ultraviolet Imager<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''': Longwave Infrared Camera<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''': Lightning and Airglow Camera<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> ==Coming meetings==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/International « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris Observatory, June 28-29, 2010]</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=192 2010-05-21T14:07:58Z

<p>Wikiadmin: /* Akatsuki */</p> <hr /> <div>This site is intended as a tool to share information, comments and schedules for preparing the 2010 coordinated campaign of ground-based observations in the context of Venus Express and coming launch of Akatsuki mission.<br /> <br /> The attached Google docs can be completed and modified according to the campaign progress. <br /> __TOC__<br /> <br /> <br /> ==Table==<br /> <br /> To prepare the campaign and coordinate telescope proposals with VEx MTPs, the attached table is under construction. Please do not hesitate to comment/modify and add more details on your plans.<br /> <br /> [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination]<br /> <br /> ==Map (under construction) ==<br /> <br /> To have a general view of the sites and telescopes which are used for ground-based observations of Venus, see this googlemap for an overview for all of the different observatories and their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> <br /> == In-orbit observations ==<br /> <br /> <br /> === Venus Express ===<br /> <br /> <br /> ==== Instruments ====<br /> <br /> [[Fichier:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> === Akatsuki ===<br /> <br /> * Goals: Akatsuki is designed to study Venus' climate using ultraviolet and infrared cameras. The spacecraft will follow orbit Venus following the westware rotation of the atmosphere, mapping the circulation and vertical structure of the planet's thick clouds. The mission will complement the ESA's Venus Express, which also explores the Venusian environment with different approaches.<br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about the project]<br /> <br /> * Accomplishments: Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time)! The mission is in development.<br /> <br /> [http://www.jaxa.jp/projects/sat/planet_c/index_e.html Visit the Akatsuki Website]<br /> <br /> ==== Instruments====<br /> [[Fichier:Akatsuki_instrumentation.gif|350px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> * '''IR1''': 1-micron Camera<br /> <br /> 1.01µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''': 2-micron Camera<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65µm<br /> <br /> * '''UVI''': Ultraviolet Imager<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''': Longwave Infrared Camera<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''': Lightning and Airglow Camera<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> ==Coming meetings==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/International « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris Observatory, June 28-29, 2010]</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=191 2010-05-21T14:07:14Z

<p>Wikiadmin: /* Akatsuki */</p> <hr /> <div>This site is intended as a tool to share information, comments and schedules for preparing the 2010 coordinated campaign of ground-based observations in the context of Venus Express and coming launch of Akatsuki mission.<br /> <br /> The attached Google docs can be completed and modified according to the campaign progress. <br /> __TOC__<br /> <br /> <br /> ==Table==<br /> <br /> To prepare the campaign and coordinate telescope proposals with VEx MTPs, the attached table is under construction. Please do not hesitate to comment/modify and add more details on your plans.<br /> <br /> [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination]<br /> <br /> ==Map (under construction) ==<br /> <br /> To have a general view of the sites and telescopes which are used for ground-based observations of Venus, see this googlemap for an overview for all of the different observatories and their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> <br /> == In-orbit observations ==<br /> <br /> <br /> === Venus Express ===<br /> <br /> <br /> ==== Instruments ====<br /> <br /> [[Fichier:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> === Akatsuki ===<br /> <br /> * Goals: Akatsuki is designed to study Venus' climate using ultraviolet and infrared cameras. The spacecraft will follow orbit Venus following the westware rotation of the atmosphere, mapping the circulation and vertical structure of the planet's thick clouds. The mission will complement the ESA's Venus Express, which also explores the Venusian environment with different approaches.<br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about the project]<br /> <br /> * Accomplishments: Akatsuki successfully launched! The mission is in development.<br /> <br /> [http://www.jaxa.jp/projects/sat/planet_c/index_e.html Visit the Akatsuki Website]<br /> <br /> ==== Instruments====<br /> [[Fichier:Akatsuki_instrumentation.gif|350px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> * '''IR1''': 1-micron Camera<br /> <br /> 1.01µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''': 2-micron Camera<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65µm<br /> <br /> * '''UVI''': Ultraviolet Imager<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''': Longwave Infrared Camera<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''': Lightning and Airglow Camera<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> ==Coming meetings==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/International « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris Observatory, June 28-29, 2010]</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=190 2010-05-21T14:05:56Z

<p>Wikiadmin: /* Akatsuki */</p> <hr /> <div>This site is intended as a tool to share information, comments and schedules for preparing the 2010 coordinated campaign of ground-based observations in the context of Venus Express and coming launch of Akatsuki mission.<br /> <br /> The attached Google docs can be completed and modified according to the campaign progress. <br /> __TOC__<br /> <br /> <br /> ==Table==<br /> <br /> To prepare the campaign and coordinate telescope proposals with VEx MTPs, the attached table is under construction. Please do not hesitate to comment/modify and add more details on your plans.<br /> <br /> [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination]<br /> <br /> ==Map (under construction) ==<br /> <br /> To have a general view of the sites and telescopes which are used for ground-based observations of Venus, see this googlemap for an overview for all of the different observatories and their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> <br /> == In-orbit observations ==<br /> <br /> <br /> === Venus Express ===<br /> <br /> <br /> ==== Instruments ====<br /> <br /> [[Fichier:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> === Akatsuki ===<br /> <br /> * Goals: Akatsuki is designed to study Venus' climate using ultraviolet and infrared cameras. The spacecraft will follow orbit Venus following the westware rotation of the atmosphere, mapping the circulation and vertical structure of the planet's thick clouds. The mission will complement the ESA's Venus Express, which also explores the Venusian environment with different approaches.<br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about the project]<br /> <br /> * Accomplishments: Akatsuki successfully launched!<br /> <br /> [http://www.jaxa.jp/projects/sat/planet_c/index_e.html Visit the Akatsuki Website]<br /> <br /> ==== Instruments====<br /> [[Fichier:Akatsuki_instrumentation.gif|350px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> * '''IR1''': 1-micron Camera<br /> <br /> 1.01µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''': 2-micron Camera<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65µm<br /> <br /> * '''UVI''': Ultraviolet Imager<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''': Longwave Infrared Camera<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''': Lightning and Airglow Camera<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> ==Coming meetings==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/International « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris Observatory, June 28-29, 2010]</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=189 2010-05-21T14:05:03Z

<p>Wikiadmin: /* Akatsuki */</p> <hr /> <div>This site is intended as a tool to share information, comments and schedules for preparing the 2010 coordinated campaign of ground-based observations in the context of Venus Express and coming launch of Akatsuki mission.<br /> <br /> The attached Google docs can be completed and modified according to the campaign progress. <br /> __TOC__<br /> <br /> <br /> ==Table==<br /> <br /> To prepare the campaign and coordinate telescope proposals with VEx MTPs, the attached table is under construction. Please do not hesitate to comment/modify and add more details on your plans.<br /> <br /> [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination]<br /> <br /> ==Map (under construction) ==<br /> <br /> To have a general view of the sites and telescopes which are used for ground-based observations of Venus, see this googlemap for an overview for all of the different observatories and their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> <br /> == In-orbit observations ==<br /> <br /> <br /> === Venus Express ===<br /> <br /> <br /> ==== Instruments ====<br /> <br /> [[Fichier:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> === Akatsuki ===<br /> <br /> * Goals: Akatsuki is designed to study Venus' climate using ultraviolet and infrared cameras. The spacecraft will follow orbit Venus following the westware rotation of the atmosphere, mapping the circulation and vertical structure of the planet's thick clouds. The mission will complement the ESA's Venus Express, which also explores the Venusian environment with different approaches.<br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about the project]<br /> <br /> * Accomplishments: <br /> <br /> [http://www.jaxa.jp/projects/sat/planet_c/index_e.html Visit the Akatsuki Website]<br /> <br /> ==== Instruments====<br /> [[Fichier:Akatsuki_instrumentation.gif|350px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> * '''IR1''': 1-micron Camera<br /> <br /> 1.01µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''': 2-micron Camera<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65µm<br /> <br /> * '''UVI''': Ultraviolet Imager<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''': Longwave Infrared Camera<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''': Lightning and Airglow Camera<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> ==Coming meetings==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/International « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris Observatory, June 28-29, 2010]</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=188 2010-05-21T13:36:27Z

<p>Wikiadmin: </p> <hr /> <div>This site is intended as a tool to share information, comments and schedules for preparing the 2010 coordinated campaign of ground-based observations in the context of Venus Express and coming launch of Akatsuki mission.<br /> <br /> The attached Google docs can be completed and modified according to the campaign progress. <br /> __TOC__<br /> <br /> <br /> ==Table==<br /> <br /> To prepare the campaign and coordinate telescope proposals with VEx MTPs, the attached table is under construction. Please do not hesitate to comment/modify and add more details on your plans.<br /> <br /> [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination]<br /> <br /> ==Map (under construction) ==<br /> <br /> To have a general view of the sites and telescopes which are used for ground-based observations of Venus, see this googlemap for an overview for all of the different observatories and their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> <br /> == In-orbit observations ==<br /> <br /> <br /> === Venus Express ===<br /> <br /> <br /> ==== Instruments ====<br /> <br /> [[Fichier:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> === Akatsuki ===<br /> <br /> * Goals: Akatsuki is designed to study Venus' climate using ultraviolet and infrared cameras. The spacecraft will follow orbit Venus following the westware rotation of the atmosphere, mapping the circulation and vertical structure of the planet's thick clouds. The mission will complement the ESA's Venus Express, which also explores the Venusian environment with different approaches.<br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about the project]<br /> <br /> * Accomplishments: This mission is in development. <br /> <br /> [http://www.jaxa.jp/projects/sat/planet_c/index_e.html Visit the Akatsuki Website]<br /> <br /> ==== Instruments====<br /> [[Fichier:Akatsuki_instrumentation.gif|350px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> * '''IR1''': 1-micron Camera<br /> <br /> 1.01µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''': 2-micron Camera<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65µm<br /> <br /> * '''UVI''': Ultraviolet Imager<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''': Longwave Infrared Camera<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''': Lightning and Airglow Camera<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> ==Coming meetings==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/International « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris Observatory, June 28-29, 2010]</div>

Wikiadmin http://vmweblesia-site.obspm.fr/venus-atm-wiki//index.php?title=Venus_coordinated_campaign&diff=187 2010-05-21T13:35:20Z

<p>Wikiadmin: /* Coordination */</p> <hr /> <div>This site is intended as a tool to share information, comments and schedules for preparing the 2010 coordinated campaign of ground-based observations in the context of Venus Express and coming launch of Akatsuki mission.<br /> <br /> The attached Google docs can be completed and modified according to the campaign progress. <br /> __TOC__<br /> <br /> ==Map (under construction) ==<br /> <br /> To have a general view of the sites and telescopes which are used for ground-based observations of Venus, see this googlemap for an overview for all of the different observatories and their instruments.<br /> <br /> * [http://maps.google.com/maps/ms?ie=UTF8&amp;hl=fr&amp;msa=0&amp;msid=106784557914957315781.000481c7cd8ab690441fc&amp;ll=-11.178402,-54.492187&amp;spn=163.437297,68.554688&amp;z=2 2010 Venus Coordinated Campaign, Telescopes sites]<br /> <br /> ==Table==<br /> <br /> To prepare the campaign and coordinate telescope proposals with VEx MTPs, the attached table is under construction. Please do not hesitate to comment/modify and add more details on your plans.<br /> <br /> [http://spreadsheets.google.com/ccc?key=0Am6asZV0iMhhdGNENE56UU9WRVJodWZpMk81cE9aTWc&amp;hl=fr 2010 Venus Coordination]<br /> <br /> == In-orbit observations ==<br /> <br /> <br /> === Venus Express ===<br /> <br /> <br /> ==== Instruments ====<br /> <br /> [[Fichier:Instruments_of_venus_express.jpg|400px|thumb|right|Instrumentation of Venus Express, Credit: ESA]]<br /> <br /> * '''SPICAV/SOIR''' : Ultraviolet and Infrared Atmospheric Spectrometer <br /> Atmospheric spectrometry by star or Sun occultation<br /> <br /> UV 0.11 - 0.3 µm R ~ 300 <br /> <br /> IR 0.7 - 1.7 µm R ~ 1300<br /> <br /> SOIR 2.3 - 4.2 µm R ~ 15000<br /> <br /> * '''VeRa''' : Venus Radio Science Experiment <br /> Radio sounding of atmosphere<br /> <br /> * '''VIRTIS''' : Ultraviolet/Visible/Near-Infrared mapping spectrometer<br /> Spectrographic mapping of atmosphere and surface<br /> <br /> VIRTIS-M mapping spectrometer <br /> <br /> Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )<br /> <br /> VIRTIS-H High-res<br /> <br /> 2 - 5 µm R ~ 1000 - 2000<br /> <br /> * '''VMC''' : Venus Monitoring Camera<br /> Ultraviolet and visible imaging<br /> <br /> Filters :<br /> <br /> UV 0.365 µm<br /> <br /> Vis 0.513 µm<br /> <br /> Near - IR1 0.965 µm<br /> <br /> Near - IR2 1.010 µm<br /> <br /> [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33964&amp;fbodylongid=1441 More about the Venus Express Instruments]<br /> <br /> === Akatsuki ===<br /> <br /> * Goals: Akatsuki is designed to study Venus' climate using ultraviolet and infrared cameras. The spacecraft will follow orbit Venus following the westware rotation of the atmosphere, mapping the circulation and vertical structure of the planet's thick clouds. The mission will complement the ESA's Venus Express, which also explores the Venusian environment with different approaches.<br /> [http://www.stp.isas.jaxa.jp/venus/top_english.html More about the project]<br /> <br /> * Accomplishments: This mission is in development. <br /> <br /> [http://www.jaxa.jp/projects/sat/planet_c/index_e.html Visit the Akatsuki Website]<br /> <br /> ==== Instruments====<br /> [[Fichier:Akatsuki_instrumentation.gif|350px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA]]<br /> * '''IR1''': 1-micron Camera<br /> <br /> 1.01µm<br /> cloud (day-night), surface (nightside)<br /> <br /> * '''IR2''': 2-micron Camera<br /> <br /> 1.73, 2.26, 2.32 (near-IR)<br /> 2.02 (CO2), 1.65µm<br /> <br /> * '''UVI''': Ultraviolet Imager<br /> <br /> 283, 365 nm<br /> SO2 - UV absorber (dayside)<br /> <br /> * '''LIR''': Longwave Infrared Camera<br /> <br /> 10 µm<br /> cloud top (day/nightside)<br /> <br /> * '''LAC''': Lightning and Airglow Camera<br /> <br /> Filters <br /> 777, 557, 553, 558, 630 nm<br /> O2/O airglow (night)<br /> lightning (night)<br /> <br /> [http://www.stp.isas.jaxa.jp/venus/E_instrument.html More about the Akatsuki Instruments]<br /> <br /> ==Coming meetings==<br /> <br /> * [http://lesia.obspm.fr/venus2010/ Venus Conference, Aussois (France), 20-26 June 2010]<br /> * [http://www.lesia.obspm.fr/venus-atm/International « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris Observatory, June 28-29, 2010]</div>

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