Venus coordinated campaign: Difference between revisions
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Spectrographic mapping of atmosphere and surface | 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 ) | 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 | 2 - 5 µm R ~ 1000 - 2000 | ||
Revision as of 11:19, 20 May 2010
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.
The attached Google docs can be completed and modified according to the campaign progress.
Map (under construction)
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.
Coordination
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.
In-orbit observations
Venus Express
Instruments
400px|thumb|right|Instrumentation of Venus Express, Credit: ESA
- 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
The Project
The Venus Climate Orbiter mission (PLANET-C), one of the future planetary missions of Japan, aims at understanding the atmospheric circulation of Venus. Meteorological information will be obtained by globally mapping clouds and minor constituents successively with 4 cameras at ultraviolet and infrared wavelengths, detecting lightning with a high-speed imager, and observing the vertical structure of the atmosphere with radio science technique. The equatorial elongated orbit with westward revolution fits the observations of the movement and temporal variation of the Venusian atmosphere which rotates westward. The systematic, continuous imaging observations will provide us with an unprecedented large dataset of the Venusian atmospheric dynamics. Additional targets of the mission are the exploration of the ground surface and the observation of zodiacal light. The mission will complement the ESA's Venus Express, which also explores the Venusian environment with different approaches.
extract of: http://www.stp.isas.jaxa.jp/venus/top_english.html
The project, a link to JAXA
Instruments
350px|thumb|right|Instrumentation of Akatsuki, Credit: JAXA
- IR1: 1-micron Camera
1.01µm cloud (day-night), surface (nightside)
- IR2: 2-micron Camera
1.73, 2.26, 2.32 (near-IR) 2.02 (CO2), 1.65µm
- UVI: Ultraviolet Imager
283, 365 nm SO2 - UV absorber (dayside)
- LIR: Longwave Infrared Camera
10 µm cloud top (day/nightside)
- LAC: Lightning and Airglow Camera
Filters 777, 557, 553, 558, 630 nm O2/O airglow (night) lightning (night)
More about the Akatsuki Instruments
