The 1.10- and 1.18-micron nightside windows of Venus observed by SPICAV-IR aboard Venus Express

Details The 1.10- and 1.18-micron nightside windows of Venus observed by SPICAV-IR aboard Venus Express The 1.10- and 1.18-micron nightside windows of Venus observed by SPICAV-IR aboard Venus Express

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..544b&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.544

Physics

1

Scientific paper

We present here an analysis of the 1.10- and 1.18-μm nightside windows observed by the infrared channel of the SPICAV (Spectroscopy for the investigation of the characteristics of the atmosphere of Venus) instrument aboard Venus Express [3]. We investigated the influence of the various sources of opacity (CO2 and H2O linelists, CO2 far wing and "continuum" opacity) on the spectrum and of the associated uncertainties or unknowns. The results were used to propose a best representation of the CO2 and H2O opacity and to derive a best fit H2O mixing ratio.

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