Skip to Main content Skip to Navigation
Conference papers

Insights on Venus’Cloud Top Chemistry, Convective Activity and Topographyfrom HST

Abstract : Based on the HSTobserved LST and latitude albedo variations we conclude that topography impacts the vertical distribution of Venus’ unidentified absorber(s) through both large and small-scale mixing processes. As this (these) species have a direct impact on Venus’ radiative balance, climate and cloud super-rotation, we strongly advocate for future observations that can uniquely and contemporaneously characterize Venus’ cloud top albedo and chemistry relative to Venus’ underlying surface topography and zonal cloud motions
Document type :
Conference papers
Complete list of metadata

Cited literature [14 references]  Display  Hide  Download
Contributor : Catherine Cardon Connect in order to contact the contributor
Submitted on : Thursday, September 26, 2019 - 6:07:10 PM
Last modification on : Friday, December 3, 2021 - 11:42:51 AM
Long-term archiving on: : Monday, February 10, 2020 - 8:42:51 AM


Publisher files allowed on an open archive


  • HAL Id : insu-02298461, version 1


Kandis-Lea Jessup, Emmanuel Marcq, Jean-Loup Bertaux, Franklin P. Mills, Sanjay Limaye, et al.. Insights on Venus’Cloud Top Chemistry, Convective Activity and Topographyfrom HST. EPSC-DPS Joint Meeting 2019, Sep 2019, Geneva, Switzerland. pp.EPSC-DPS2019-672-2. ⟨insu-02298461⟩



Les métriques sont temporairement indisponibles