Venus coordinated campaign

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)

• 2010 Venus Coordinated Campaign telescope sites

Coordination

Two tables to facilitate the coordination on Venus:

Link on: Coordination and Information

In-orbit observations

Venus Express

Instruments

• ASPERA : Analyser of Space Plasma and Energetic Atoms

Neutral and ionised plasma analysis

• MAG : Venus Express Magnetometer

Magnetic field measurements

• SPICAV/SOIR : Ultraviolet and Infrared Atmospheric Spectrometer

Atmospheric spectrometry by star or Sun occultation

• VeRa : Venus Radio Science Experiment

Radio sounding of atmosphere

• VIRTIS : Ultraviolet/Visible/Near-Infrared mapping spectrometer

Spectrographic mapping of atmosphere and surface

• VMC : Venus Monitoring Camera

Ultraviolet and visible imaging

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

Instrumentation and Techniques

• 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

777, 551, 553, 558, 630 nm O2/O airglow (night) lightning (night)

More about the Akatsuki Instruments

Future meetings

• International Venus Conference, Aussois (France)

20-26 June 2010