The OH Venus nightglow: morphology and relation to ozone in the upper atmosphere

Details The OH Venus nightglow: morphology and relation to ozone in the upper atmosphere The OH Venus nightglow: morphology and relation to ozone in the upper atmosphere

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..896s&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.896

Computer Science

Scientific paper

An analysis of the spectral distribution of OH infrared nightglow spectra obtained with the VIRTIS spectral imager on board Venus Express will be presented. It will be compared with models of the intensity distribution among the Δv=1 and 2 bands and rotational lines calculated with recent quenching coefficients of OH* by CO2 molecules. The total intensity will be compared with that expected from the reaction of ozone with atomic hydrogen, based on the O3 abundance recently derived from stellar occultations.

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