Computer Science
Scientific paper
Oct 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..189y&link_type=abstract
EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.189
Computer Science
Scientific paper
Venus Express and ground-based measurements of an inversion layer with enhanced concentrations of SO and SO2 in the mesosphere of Venus (Belyaev et al., 2008; 2010; Clancy et al. 2008) suggests a new source of gaseous sulfur that was not included in the previous models of Venus (see, e.g., Mills et al. 2007). A one-dimensional photochemistry-transport model is used to simulate the whole chemical system including oxygen-, hydrogen-, chlorine-, sulfur-, and nitrogen-bearing species (see schematic in Figure 1). The evaporation of aerosols composed of sulfuric acid (model A) or polysulfur (model B) above 90 km could provide a new source of gaseous sulfur species (Zhang et al. 2010; 2011). The implications of the new model are discussed in light of recent measurements (Sandor et al. 2011). Future measurements are needed to confirm the model predictions.
Belyaev Denis A.
Liang Mao-Chang
Mills Franklin P.
Yung Yuk L.
Zhang Xinyu
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