Variations in Venus' Cloud Top SO2 and SO Gas Density with Latitude and Time of Day

Kandis Lea Jessup; Frank Mills; E. Marcq; J-L. Berteaux; Tony Roman; Yuk L Yung

doi:epsc2013/sessionprogramme

Variations in Venus' Cloud Top SO2 and SO Gas Density with Latitude and Time of Day

Kandis Lea Jessup
, Frank Mills
, E. Marcq
, J-L. Berteaux
, Tony Roman
, Yuk L Yung

Research output: Contribution to journal › Meeting Abstract

Abstract

Venus upper atmospheric H2SO4 clouds are formed from SO2 gas via the sulfur-oxidation cycle, beginning with SO2 photolysis; followed by the formation of SO3 via photochemical SO2 oxidation, which then reacts with H2O forming H2SO4. Thus, photochemical processing of SO2 is intimately linked to the global-scale cloud and haze layers, which are composed primarily of concentrated sulfuric acid.

Original language	English
Pages (from-to)	3pp
Journal	European Planetary Science Congress 2013
DOIs	https://doi.org/epsc2013/sessionprogramme
Publication status	Published - 2013
Event	European Planetary Science Congress 2013 - University College London Duration: 1 Jan 2013 → …

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title = "Variations in Venus' Cloud Top SO2 and SO Gas Density with Latitude and Time of Day",

abstract = "Venus upper atmospheric H2SO4 clouds are formed from SO2 gas via the sulfur-oxidation cycle, beginning with SO2 photolysis; followed by the formation of SO3 via photochemical SO2 oxidation, which then reacts with H2O forming H2SO4. Thus, photochemical processing of SO2 is intimately linked to the global-scale cloud and haze layers, which are composed primarily of concentrated sulfuric acid.",

author = "Jessup, \{Kandis Lea\} and Frank Mills and E. Marcq and J-L. Berteaux and Tony Roman and Yung, \{Yuk L\}",

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journal = "European Planetary Science Congress 2013",

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T1 - Variations in Venus' Cloud Top SO2 and SO Gas Density with Latitude and Time of Day

AU - Jessup, Kandis Lea

AU - Mills, Frank

AU - Marcq, E.

AU - Berteaux, J-L.

AU - Roman, Tony

AU - Yung, Yuk L

PY - 2013

Y1 - 2013

N2 - Venus upper atmospheric H2SO4 clouds are formed from SO2 gas via the sulfur-oxidation cycle, beginning with SO2 photolysis; followed by the formation of SO3 via photochemical SO2 oxidation, which then reacts with H2O forming H2SO4. Thus, photochemical processing of SO2 is intimately linked to the global-scale cloud and haze layers, which are composed primarily of concentrated sulfuric acid.

AB - Venus upper atmospheric H2SO4 clouds are formed from SO2 gas via the sulfur-oxidation cycle, beginning with SO2 photolysis; followed by the formation of SO3 via photochemical SO2 oxidation, which then reacts with H2O forming H2SO4. Thus, photochemical processing of SO2 is intimately linked to the global-scale cloud and haze layers, which are composed primarily of concentrated sulfuric acid.

U2 - epsc2013/sessionprogramme

DO - epsc2013/sessionprogramme

M3 - Meeting Abstract

SP - 3pp

JO - European Planetary Science Congress 2013

JF - European Planetary Science Congress 2013

T2 - European Planetary Science Congress 2013

Y2 - 1 January 2013

ER -

Variations in Venus' Cloud Top SO2 and SO Gas Density with Latitude and Time of Day

Abstract

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