Assimilation of data from the Solar Aureole imager and the Visible Spectrometer onboard the Huygens probe into a radiative transfer model of Titan's Atmosphere

Details Assimilation of data from the Solar Aureole imager and the Visible Spectrometer onboard the Huygens probe into a radiative transfer model of Titan's Atmosphere Assimilation of data from the Solar Aureole imager and the Visible Spectrometer onboard the Huygens probe into a radiative transfer model of Titan's Atmosphere

Nov 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001dps....33.5509g&link_type=abstract

American Astronomical Society, DPS Meeting #33, #55.09; Bulletin of the American Astronomical Society, Vol. 33, p.1140

Astronomy and Astrophysics

Astronomy

Scientific paper

During the descent of the Huygens probe through Titan's atmosphere in January 2005, the Descent Imager / Spectral Radiometer (DISR) will performe upward and downward looking measurements at various spectral ranges and spatial resolutions. Simulated data from two DISR subinstruments, the Solar Aureole imager and the Upward Looking Visible Spectrometer, have been assimilated into an inverse radiative transfer model to reconstruct the scattering phase function in the atmosphere in dependence on the altitude. Results are shown in the Figure. \leavevmode \epsfxsize=0.8\hsize \epsfbox{34.eps} This work was supported by the German Aerospace Center (DLR), contract number 50 OH 98044.

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