Advancing Venus atmospheric modelling via coordinated HST-Akatsuki observations

Kandis Lea Jessup; T. Imamura; M. Nakamura; Frank Mills; E. Marcq; Sanjay Limaye; C. Wilson; Jean-Loup Bertaux; E. Young; T. Kremic

doi:meetings/lpsc2016/programAbstracts/view/

Advancing Venus atmospheric modelling via coordinated HST-Akatsuki observations

Kandis Lea Jessup, T. Imamura, M. Nakamura, Frank Mills, E. Marcq, Sanjay Limaye, C. Wilson, Jean-Loup Bertaux, E. Young, T. Kremic

Research output: Contribution to journal › Meeting Abstract

Abstract

Venus global-scale H2SO4 cloud and haze layers form via the combination of SO3 and H2O, and SO3 forms via oxidation of SO2. Sulfurbearing and sulfur-oxidized species, such as SO2, SO, S, OCS, H2SO4, are key traces of Venus H2SO4 cloud/haze formation process.

Original language	English
Pages (from-to)	2pp
Journal	47th Lunar and Planetary Science Conference
DOIs	https://doi.org/meetings/lpsc2016/programAbstracts/view/
Publication status	Published - 2016
Event	47th Lunar and Planetary Science Conference - The Woodlands, Texas, USA Duration: 1 Jan 2016 → …

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title = "Advancing Venus atmospheric modelling via coordinated HST-Akatsuki observations",

abstract = "Venus global-scale H2SO4 cloud and haze layers form via the combination of SO3 and H2O, and SO3 forms via oxidation of SO2. Sulfurbearing and sulfur-oxidized species, such as SO2, SO, S, OCS, H2SO4, are key traces of Venus H2SO4 cloud/haze formation process.",

author = "Jessup, {Kandis Lea} and T. Imamura and M. Nakamura and Frank Mills and E. Marcq and Sanjay Limaye and C. Wilson and Jean-Loup Bertaux and E. Young and T. Kremic",

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T1 - Advancing Venus atmospheric modelling via coordinated HST-Akatsuki observations

AU - Jessup, Kandis Lea

AU - Imamura, T.

AU - Nakamura, M.

AU - Mills, Frank

AU - Marcq, E.

AU - Limaye, Sanjay

AU - Wilson, C.

AU - Bertaux, Jean-Loup

AU - Young, E.

AU - Kremic, T.

PY - 2016

Y1 - 2016

N2 - Venus global-scale H2SO4 cloud and haze layers form via the combination of SO3 and H2O, and SO3 forms via oxidation of SO2. Sulfurbearing and sulfur-oxidized species, such as SO2, SO, S, OCS, H2SO4, are key traces of Venus H2SO4 cloud/haze formation process.

AB - Venus global-scale H2SO4 cloud and haze layers form via the combination of SO3 and H2O, and SO3 forms via oxidation of SO2. Sulfurbearing and sulfur-oxidized species, such as SO2, SO, S, OCS, H2SO4, are key traces of Venus H2SO4 cloud/haze formation process.

U2 - meetings/lpsc2016/programAbstracts/view/

DO - meetings/lpsc2016/programAbstracts/view/

M3 - Meeting Abstract

SP - 2pp

JO - 47th Lunar and Planetary Science Conference

JF - 47th Lunar and Planetary Science Conference

T2 - 47th Lunar and Planetary Science Conference

Y2 - 1 January 2016

ER -

Advancing Venus atmospheric modelling via coordinated HST-Akatsuki observations

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