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Instrumental requirements for the study of Venus' cloud top using the UV imaging spectrometer VeSUV

Marq, E and MontMessin, Franck and Lasue, J. and Bezard, B. and Jessup, Kandis and Lee, Yeon Joo and Wilson, C.F. and Lustrement, Benjamin and Rouanet, Nicolas and Guignan, G. (2021) Instrumental requirements for the study of Venus' cloud top using the UV imaging spectrometer VeSUV. Advances in Space Research, 68 (1), pp. 275-291. Elsevier. doi: 10.1016/j.asr.2021.03.012. ISSN 0273-1177.

Full text not available from this repository.

Official URL: https://linkinghub.elsevier.com/retrieve/pii/S0273117721002192

Abstract

Ultraviolet spectral imaging has been a powerful tool to investigate the cloud top of Venus, allowing for measurement of several minor gases (especially SO2, SO, O3), of cloud top aerosol's microphysical properties and of atmospheric dynamics through tracking of the unevenly distributed UV absorber. After a brief review of recent UV instruments that orbited around Venus, we present the results of a state-of-the-art radiative transfer model from Marcq et al. (2020) to derive the spectral resolution and Signal-to-Noise ratio (SNR) required to derive abundances of these gases, retrieve optical properties of the aerosols beyond our current knowledge. This leads us to propose a two-channel UV hyperspectral push-broom imager called VeSUV (standing for Venusian Spectroscopy in UV) whose technical characteristics will improve on existing measurements by a factor of at least 2, and which is well suited to the integration into the payload of future low Venus orbit platforms such as the proposed EnVision mission to ESA M5 call.

Item URL in elib:https://elib.dlr.de/146138/
Document Type:Article
Title:Instrumental requirements for the study of Venus' cloud top using the UV imaging spectrometer VeSUV
Authors:
AuthorsInstitution or Email of AuthorsAuthor's ORCID iD
Marq, ELATMOS, Université de Versailles Saint-Quentin-en-Yvelines, Guyancourt, FranceUNSPECIFIED
MontMessin, FranckLATMOSUNSPECIFIED
Lasue, J.Université de Toulouse & CNRSUNSPECIFIED
Bezard, B.LESIA, Observatoire de Paris (CNRS-UMR 8109), 5 place Jules Janssen, 92195 Meudon, FranceUNSPECIFIED
Jessup, KandisSWRI, Boulder, CO, USAUNSPECIFIED
Lee, Yeon Jooyeon.lee (at) dlr.dehttps://orcid.org/0000-0002-4571-0669
Wilson, C.F.Physics Department, Oxford University, Oxford, UKUNSPECIFIED
Lustrement, BenjaminLATMOS, Guyancourt, FranceUNSPECIFIED
Rouanet, NicolasLATMOS/IPSL, UVSQ, Université Paris-Saclay, Sorbonne Université, CNRS, Guyancourt, FranceUNSPECIFIED
Guignan, G.LATMOS/IPSL, Sorbonne Université, UVSQ, CNRS, Paris, FranceUNSPECIFIED
Date:2021
Journal or Publication Title:Advances in Space Research
Refereed publication:Yes
Open Access:No
Gold Open Access:No
In SCOPUS:Yes
In ISI Web of Science:Yes
Volume:68
DOI :10.1016/j.asr.2021.03.012
Page Range:pp. 275-291
Publisher:Elsevier
ISSN:0273-1177
Status:Published
Keywords:Venus, UV spectroscopy
HGF - Research field:Aeronautics, Space and Transport
HGF - Program:Space
HGF - Program Themes:Space Exploration
DLR - Research area:Raumfahrt
DLR - Program:R EW - Space Exploration
DLR - Research theme (Project):R - Project PLATO - PMC and Science
Location: Berlin-Adlershof
Institutes and Institutions:Institute of Planetary Research > Extrasolar Planets and Atmospheres
Deposited By: Cabrera Perez, Juan
Deposited On:24 Nov 2021 13:37
Last Modified:24 Nov 2021 13:37

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