Venus coordinated campaign: Difference between revisions
No edit summary |
|||
| Line 52: | Line 52: | ||
===== Current ===== | ===== Current ===== | ||
* VEx science operations, Jan. 2012 - April 2013, VSOC team : | * VEx science operations, Jan. 2012 - April 2013, VSOC team : | ||
[[File:VEX-SCIOPS-PO-016_1_F_VEX_3rd_P3_Extended_Overview_2011Nov03.pdf]] | |||
<br clear=all> | <br clear=all> | ||
Revision as of 00:03, 7 July 2012
This wiki is provided as a tool for sharing information and schedules for coordinated Venus observations in support of ESA/Venus Express, JAXA/Akatsuki and comparative climatology of the Earth and Venus. Last update July 6, 2012 - TW
What's New ?
July 6, 2012 - Schedule of 2012B ground-based Venus observations updated. Period July 2012-January 2013 encompasses Venus Express MTP 81-87 - T.W.
June 5-6, 2012 - the international campaign to observe the aureole of refracted sunlight in the transiting Venus' atmosphere on June 5-6, 2012 has involved several orbiting spacecraft/instrumentation. There has been a worldwide coordination between NASA's Hubble Space Telescope ACS/WFC3 moon observations, ESA's Venus Express science operations, JAXA's Hinode Solar Observatory/SOT, AURA's NSO/IBIS visible high resolution spectro-imagery, NASA's Solar Dynamical Observatory/HMI and the ground-based Venus Twilight Experiment coronographs. - See e.g. Science News@Analysis, Vol. 336, 11 May 2012 : Venus's Rare Sun Crossing May Aid Search for Exoplanets - T.W.
Mar. 5-7, 2012 - Third Europlanet strategic workshop – 4th JSPS/PHC/Sakura meeting - France, Observatoire de Paris and Institut d'Astrophysique, March 5-7, 2012 - Added link to presentations on the website. - T.W.
Nov. 21-22, 2011 - Third JSPS/PHC Sakura meeting, ISAS, Sagamihara Campus, November 21-22, 2011. Added meeting agenda and minutes. - T.W.
October 2011 - Added a DPS/EPSC virtual poster session section. New section for the 2012 transit of Venus coordination campaign. Added links to the VEXAG website and future meetings - T.W.
June 2011 - Added files 2010_Campaign_5.pdf and .jpg. Now includes coordination summary up to June-July 2011. - T.W.
June 2011 - now includes planning overview poster for Jan 2012 - April 2013. - C.W.
Nov. 21, 2010 - Scheduled ground-based observations updated. Includes MTP 63-64 planned campaign 25 Feb – 15 March 2011. - T.W.
Circumstances of Venus coordinated campaigns
Scheduled ground-based observations
Current
- Ground-based campaign in support of Venus-Express, Jul. 2012 - Jan. 2013
- Circumstances of Venus observation from Earth, 2010-2014
Archive
- Ground-based campaign, Jul. 2010 - Jan. 2012
- Editable Google spreadsheet for detailed observing circumstances
- 2010 | Detailed observing circumstances (Editable Google spreadsheet)
VEx - ground-based coordination files
Current
- VEx science operations, Jan. 2012 - April 2013, VSOC team :
File:VEX-SCIOPS-PO-016 1 F VEX 3rd P3 Extended Overview 2011Nov03.pdf
- SOIR Files:
In order to make it easier for all observers to have access to the observations date & time performed by SOIR on VEX, the SOIR team has built a web tool which allows the user to find past and near-future observations of SOIR corresponding to several search criteria. This tool can be accessed freely with no password needed through our web site at the following address : [1]
SOIR solar occultation opportunities in the period 1/1/2012-31/12/2012are described in the following file: File:SOIR MTP76-MTP86.xls.
For further details, contact the SOIR Principal Investigator: Ann-Carine Vandaele <A-C.Vandaele@aeronomie.be>
Archive
- Venus observing by NASA-ESA/Hubble Space Telescope : File:HST-soir overlap.txt
- VEx science operations, Jul. 2010 - Jan. 2012, VSOC team :
- VeRa Files:
This file descibes all VeRa radio occultations carried out in the period 1/7/2006 - 2/6/2010.
For further information contact the VeRa team: Martin Paetzold <Martin.Paetzold@uni-koeln.de>, Bernd Hauesler <Bernd.Haeusler@unibw.de>, and Silvia Tellmann <tellmann@geo.uni-koeln.de>
This file describes all opportunities for Radio occultations in occultation seasons in January 2011 - November 2012. File kindly provided by Stefan Remus, ESAC. Note that not all radio occultation opportunities are exploited.
For further information contact the VeRa team: Martin Paetzold <Martin.Paetzold@uni-koeln.de>, Bernd Hauesler <Bernd.Haeusler@unibw.de>, and Silvia Tellmann <tellmann@geo.uni-koeln.de>.
Coordination meetings / meeting sessions
Past and future workshops / Meeting sessions
- July 14-22, 2012 COSPAR session on Venus Exploration (M. Nakamura and H. Svedhem conveners)
- Science Conference on Comparative Climatology of the Terrestrial Planets, Boulder, June 25-28, 2012
- Japan Geoscience Union (JpGU) Meeting, 20-25 May, 2012, Makuhari Messe, Japan.
- Third Europlanet strategic workshop – 4th JSPS/PHC/Sakura meeting - France, Observatoire de Paris and Institut d'Astrophysique, March 5-7, 2012.
- January 25–26, 2012 - Meeting on Earth-based Balloon Platform for Planetary Observations, NASA Glenn Research Center, Cleveland, Ohio
- Third JSPS/PHC Sakura meeting, ISAS, Sagamihara Campus, November 21-22, 2011.
- Meeting agenda: File:3rdmeeting.pdf
- Meeting minutes/report: File:3rdSakuraReport.pdf
- VEx Science Working Team Meeting, 16-18 November 2011, Graz, Austria
- Atmospheric waves workshop, 9-10 November 2011, ESTEC, Noordwijk, NL
- VEXAG International Venus Workshop, Smithsonian Steven F. UdvarHazy Center, Dulles Airport, Washington DC 30 August - 1 September 2011
- Second JSPS/PHC Sakura meeting, University of Tokyo, Space science building, December 3, 2010.
- 2010 VEXAG International Workshop: Venus, Our Closest Earth-like Planet, Madison (USA), 30 August - 2 September 2010
- « After-Aussois Venus 2010 » workshop: 1st strategic workshop on Coordinated ground-based measurements and modeling of the Venus atmosphere, Paris, June 28-29, 2010
- Venus Conference, Aussois (France), 20-26 June 2010
- First JSPS/PHC Sakura meeting, ISAS, Sagamihara Campus, February 23-25, 2010.
EPSC/DPS Nantes Oct. 2011 - Venus virtual poster session
- Machado et al. 2011, Characterization of Venus' cloud top dynamics using ground-based Doppler spectroscopy
- Peralta et al. 2011, Solar Tides in the Winds of the Southern Polar Region of Venus using VIRTIS-M/VEx Images
- Sonnabend et al. 2011, Thermospheric/Mesospheric Temperatures on Venus : Comparison between Ground-based High-Resolution Spectroscopy of CO2 and other Techniques
- Stangier et al. 2011, Investigation of CO2 Absorption Features on Venus
 Machado et al. 2011 Characterization of Venus' cloud top dynamics using ground-based Doppler spectroscopy File:Machado-Nantes.pdf |
 Peralta et al. 2011 Solar Tides in the Winds of the Southern Polar Region of Venus using VIRTIS-M/VEx Images File:Peralta-Nantes.pdf |
 Sonnabend et al. 2011 Thermospheric/Mesospheric Temperatures on Venus : Comparison between Ground-based High-Resolution Spectroscopy of CO2 and other Techniques File:Sonnabend-Nantes.pdf |
 |
| File:Machado-Nantes.pdf | File:Peralta-Nantes.pdf | File:Sonnabend-Nantes.pdf | File:Stangier-Nantes.pdf |
Detailed instrumental characteristics
Ground-based facilities
Clickable map of observatory sites and telescope facilities, with a link to their instruments.
- Venus Coordinated Campaign, Telescopes sites (editable Google map)
<googlemap version="0.9" lat="5.266008" lon="81.5625" type="terrain" zoom="2" controls="large"> http://www.lesia.obspm.fr/venus-atm/2010venus.kml </googlemap>
- Sunspot Astronomy & Visitor Center
- Observatorio SOAR
- Observatoire du Pic du Midi de Bigorre
- Osservatorio Astronomico della Regione Autonoma Valle d'Aosta
- South African Astronomical Observatory
- Southern African Large Telescope (SALT)
- Hanle Observatory
- 4 TAOS robotic
- Naroyo Observatory
- Naroyo 1.6-m
- Siding Spring Observatory
- 1 m McLellan
- MOA 1.8-m
- 0.6-m Optical Craftsmen
- 0.6-m Boller & Chivens
- Mauna Kea Observatory
- Haleakala Observatory
- THIS Tuneable Heterodyne Infrared Spectrometer
used at the:
- - McMath-Pierce Solar Telescope on Kitt Peak in Arizona
- - IRTF on Mauna Kea Hawaii
- HIPWAC Heterodyne Instrument for Planetary Wind And Composition at IRTF
Venus Express instruments
- SPICAV/SOIR : Ultraviolet and Infrared Atmospheric Spectrometer
Atmospheric spectrometry by star or Sun occultation
UV 0.11 - 0.3 µm R ~ 300
IR 0.7 - 1.7 µm R ~ 1300
SOIR 2.3 - 4.2 µm R ~ 15000
- VeRa : Venus Radio Science Experiment
Radio sounding of atmosphere
- VIRTIS : Ultraviolet/Visible/Near-Infrared mapping spectrometer
Spectrographic mapping of atmosphere and surface
- VIRTIS-M mapping spectrometer
Vis 0.25 - 1.0 µm R ~ 100 - 200 ( IR 1 - 5 µm R ~ 100 - 200 )
- VIRTIS-H High-res
2 - 5 µm R ~ 1000 - 2000
- VMC : Venus Monitoring Camera
Ultraviolet and visible imaging
Filters :
UV 0.365 µm
Vis 0.513 µm
Near - IR1 0.965 µm
Near - IR2 1.010 µm
More about the Venus Express Instruments
Akatsuki instruments
Akatsuki successfully launched at 6:58:22 a.m. on May 21 (Japan Standard Time) !
More about VCO/Akatsuki mission
- IR1 : 1-micron Camera
Low stratus, vapor, active volcanism
1.01 µm cloud (day-night), surface (nightside)
- IR2 : 2-micron Camera
Low stratus, trace gasses, zodiacal light
1.73, 2.26, 2.32 (near-IR) 2.02 (CO2), 1.65 µm
- UVI : Ultraviolet Imager
Cloud-top ultraviolet absorber, SO2
283, 365 nm SO2 - UV absorber (dayside)
- LIR : Longwave Infrared Camera
Cloud-top temperature distribution
10 µm cloud top (day/nightside)
- LAC : Lightning and Airglow Camera
Lightening flash, high-stratus airglow emission
Filters 777, 557, 553, 558, 630 nm O2/O airglow (night) lightning (night)
More about the Akatsuki Instruments
Transit of Venus coordinated campaign, June 5-6, 2012
Planning
Venus Twilight / coronagraph experiment : Science background - collaborations - Tutorials for registered users https://venustex.oca.eu/foswiki/bin/view/Main/WebHome
Contact times for the transit can be found at: http://eclipse.gsfc.nasa.gov/transit/venus/city12-2.html
Annual mean cloud cover for June : http://xjubier.free.fr/en/site_pages/SolarEclipseWeather.html
Science references
Ehrenreich, D., Vidal-Madjar, A., Widemann, T., Gronoff, G., Tanga, P., Barthélemy, M., Lilensten, J., Lecavelier des Etangs, A. and Arnold, L. 2011, Transmission spectrum of Venus as a transiting exoplanet, accepted in Astronomy & Astrophysics.
Tanga, P., Widemann, T., Sicardy, B., Pasachoff, J., Arnaud, J., Comolli, L., Rondi, A., Rondi, S., Suetterlin, P. 2011, Solar light refraction by the Venus mesosphere during the 2004 transit, accepted in Icarus.
Pasachoff, J.M., G. Schneider, and T. Widemann 2011, High-Resolution Satellite Imaging of the 2004 Transit of Venus and Asymmetries In the Cytherean Atmosphere, Astronomical Journal, 141, 112.
Hedelt, P., R. Alonso, T. Brown, M. Collados Vera, H. Rauer, H. Schleicher, W. Schmidt, F. Schreier, and R. Titz 2011, Venus transit 2004 : Illustrating the capability of exoplanet transmission spectroscopy, A&A 533, A136.
Ambastha, A., Ravindra, B. and Gosain, S. 2006, H-alpha observations of 8 june, 2004 Venus transit, Solar Phys. 233:171-184.
De, S.S., De, B.K., Adhikari, S.K., Sarkar, B.K., Sarkar, S.K., Guha, A., Mandal, P.K., Mandal, S.K., Sardar, H.P. and Ray, M. 2006, The effect of recent Venus transit on Earth's atmosphere, Ann. Geophys. Vol. 49, N.6, Dec. 2006.
Other links
The Venus Exploration Analysis Group, established in 2005, is NASA's community-based forum designed to provide scientific input and technology development plans for planning and prioritizing the exploration of Venus over the next several decades
(Between 23 May and 9 June 2007 - ESA web site)
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 Venus Express (VEX) spacecraft observations of Venus with worldwide ground-based images to allow for continuous monitoring of the planet.
