Scientific objectives and instrumental requirements of the IR spectrometer VenSpec-H onboard EnVision
Séverine Robert
(1)
,
Justin Erwin
(1)
,
Roderick de Cock
(1)
,
Ian Thomas
(1)
,
Nuno Pereira
(1)
,
Lars Jacobs
(1)
,
Sophie Berkenbosch
(1)
,
David Bolsée
(1)
,
Filip Vanhellemont
(1)
,
Eddy Neefs
(1)
,
Shohei Aoki
(2)
,
Bruno Bézard
(3)
,
Emmanuel Marcq
(4)
,
Giulia Alemanno
(5)
,
Joern Helbert
(5)
,
Ann Vandaele
(1)
1
BIRA-IASB -
Belgian Institute for Space Aeronomy / Institut d'Aéronomie Spatiale de Belgique
2 UTokyo - The University of Tokyo
3 LESIA - Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics
4 SYSTEME SOLAIRE - LATMOS
5 DLR - Deutsches Zentrum für Luft- und Raumfahrt [Köln]
2 UTokyo - The University of Tokyo
3 LESIA - Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics
4 SYSTEME SOLAIRE - LATMOS
5 DLR - Deutsches Zentrum für Luft- und Raumfahrt [Köln]
Bruno Bézard
- Fonction : Auteur
- PersonId : 738795
- IdHAL : bruno-bezard
- ORCID : 0000-0002-5433-5661
- IdRef : 119468514
Emmanuel Marcq
- Fonction : Auteur
- PersonId : 175261
- IdHAL : emmanuel-marcq
- ORCID : 0000-0002-1924-641X
- IdRef : 119981246
Résumé
Onboard the spacecraft, there will be a suite of three spectrometers, VenSpec. One of these is called VenSpec-H where the H stands for high spectral resolution. Its scientific objectives consist in measuring variations of minor species’ abundances in the atmosphere of Venus. H2O, SO2, CO and OCS will be measured to characterize the potentially ongoing volcanic activity
