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- W131966579 abstract "The NASA mission MESSENGER fly-byed planet Venus on June 2007 on its route to Mercury. This chance was took to produce coordinated observations between Messenger and ESA Venus Express spacecrafts. This work shows spectra in the wavelength range between 320 and 1450nm retrieved with the instrument MASCS (Mercury Atmospheric and Surface Composition Spectrometer). Spectra are calibrated in absolute reflectivity (diffuse reflection by Venus clouds) and wavelength, and they are navigated in order to retrieve their position in the planet’s disk. Comparing synthetic spectra with these ones for each viewing geometry we will obtain information on the vertical distribution of cloud particulates between 60 and 75km height, approximately, as well as the SO2 abundance, among others. This will be combined with almost simultaneous data gathered by the visible and infrared spectrograph VIRTIS onboard Venus Express spacecraft. The results of the atmospheric modeling will be presented elsewhere." @default.
- W131966579 created "2016-06-24" @default.
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- W131966579 date "2010-01-01" @default.
- W131966579 modified "2023-09-25" @default.
- W131966579 title "Venus Spectrophotometry During the MESSENGER Mission Fly-By" @default.
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- W131966579 doi "https://doi.org/10.1007/978-3-642-11250-8_125" @default.
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