Photochemical Distribution of Venusian Sulphur and Halogen Species AND Why Vulcanism cannot be the source for Venusian SO 2 above 80km . C. D. Parkinson Brecht, S. W. Bougher , F. Mills, M. Allen, X. Zhang and Y. L. Yung DPS 2010 (Poster 10.4).
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Photochemical Distribution of VenusianSulphurand Halogen SpeciesANDWhy Vulcanism cannot be the source for Venusian SO2 above 80km
C. D. Parkinson
Brecht, S. W. Bougher, F. Mills, M. Allen,
X. Zhang and Y. L. Yung
DPS 2010 (Poster 10.4)
Blue shaded area shows parameter space where model predicts SO2
mixing ratios between 0.01 and 1 ppm at 100 km
Golden line = max values of SO2 (67 ppb) from microwave measurements of Sandor et al (2010)
No change in SO2 above 80 km due to pulse in lower atmosphere
Vulcanism not the source of SO2 above this point