Observation of mesospheric CO in Venus using VIRTIS-H aboard Venus Express

Details Observation of mesospheric CO in Venus using VIRTIS-H aboard Venus Express Observation of mesospheric CO in Venus using VIRTIS-H aboard Venus Express

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..423e&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.423

Physics

Scientific paper

The thermal emission of the dark side of Venus is used to investigate
the distribution of CO above the clouds using the VIRTIS-H instrument
aboard Venus Express. The objective is to study the latitudinal
variations of CO, in particular in the polar regions.

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