Variability of SO2 at Venus' cloud top during the July 2009 brightening event as seen by SPICAV-UV

Details Variability of SO2 at Venus' cloud top during the July 2009 brightening event as seen by SPICAV-UV Variability of SO2 at Venus' cloud top during the July 2009 brightening event as seen by SPICAV-UV

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..537m&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.537

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Scientific paper

This paper applies the methods used by Marcq et al. [5] to derive observable SO2 column densities using SPICAV-UV in nadir mode on Venus Express to newer data immediately before and after the brightening event seen from Earth from 2009/07/19 to 2009/07/26 in the visible range. This event appears to have been followed by a global depletion in visible SO2 content lasting at last 6 Earth months. Various explanations are proposed to explain the observations, stressing the need for simultaneous measurements of other minor species in order to discriminate between competing hypotheses.

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