Insights on Venus’Cloud Top Chemistry, Convective Activity and Topographyfrom HST - Archive ouverte HAL Access content directly
Conference Papers Year : 2018

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

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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
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Dates and versions

insu-02298461 , version 1 (26-09-2019)

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  • HAL Id : insu-02298461 , version 1

Cite

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⟩
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