Conference papers
The Venus Emissivity Mapper concept
Jörn Helbert
1
Ingo Walter
2
Dennis Wendler
1
Thomas Widemann
3
Emmanuel Marcq
4
Gabriel Guignan
5
Sabrina Ferrari
6
Alessandro Maturilli
1
Nils Mueller
7
David Kappel
1
Judit Jaenchen
8
Mario d'Amore
1
Anko Boerner
8
M. Darby Dyar
9
Gabriele E. Arnold
8
Suzanne E. Smrekar
7
Emmanuel Marcq 4
Author IdHAL : emmanuel-marcq ORCID : https://orcid.org/0000-0002-1924-641X
Gabriel Guignan 5
Author IdHAL : gabriel-guignan
Sabrina Ferrari 6
Author
Alessandro Maturilli 1
Author
Anko Boerner 8
Author
M. Darby Dyar 9
Author
Gabriele E. Arnold 8
Author
Suzanne E. Smrekar 7
Author
1
DLR Institut für Planetenforschung (Berlin - Germany)
- DLR - Deutsches Zentrum für Luft- und Raumfahrt [Berlin] (Rutherfordstraße 2 12489 Berlin - Germany)
2
DLR Institute for Optical Sensorsystems (Germany)
- DLR - Deutsches Zentrum für Luft- und Raumfahrt [Berlin] (Rutherfordstraße 2 12489 Berlin - Germany)
3
LESIA - Laboratoire d'études spatiales et d'instrumentation en astrophysique (5, place Jules Janssen 92190 MEUDON - France)
- UPMC - Université Pierre et Marie Curie - Paris 6 (4 place Jussieu - 75005 Paris - France)
- INSU - CNRS - Institut national des sciences de l'Univers (INSU-CNRS 3 rue Michel-Ange, 75794 Paris Cedex 16 - France)
- Observatoire de Paris (61 Av de l'Observatoire 75014 PARIS - France)
- PSL - Université Paris sciences et lettres (60 rue Mazarine 75006 Paris - France)
- UPD7 - Université Paris Diderot - Paris 7 (5 rue Thomas-Mann - 75205 Paris cedex 13 - France)
- CNRS - Centre National de la Recherche Scientifique : UMR8109 (France)
4
PLANETO - LATMOS (France)
- LATMOS - Laboratoire Atmosphères, Milieux, Observations Spatiales (11 boulevard d'Alembert
Quartier des Garennes
78280 - Guyancourt - France)
- UVSQ - Université de Versailles Saint-Quentin-en-Yvelines : UMR8190 (55 avenue de Paris - 78035 Versailles cedex - France)
- UPMC - Université Pierre et Marie Curie - Paris 6 : UMR8190 (4 place Jussieu - 75005 Paris - France)
- INSU - CNRS - Institut national des sciences de l'Univers : UMR8190 (INSU-CNRS 3 rue Michel-Ange, 75794 Paris Cedex 16 - France)
- CNRS - Centre National de la Recherche Scientifique : UMR8190 (France)
5
LATMOS - Laboratoire Atmosphères, Milieux, Observations Spatiales (11 boulevard d'Alembert
Quartier des Garennes
78280 - Guyancourt - France)
- UVSQ - Université de Versailles Saint-Quentin-en-Yvelines : UMR8190 (55 avenue de Paris - 78035 Versailles cedex - France)
- UPMC - Université Pierre et Marie Curie - Paris 6 : UMR8190 (4 place Jussieu - 75005 Paris - France)
- INSU - CNRS - Institut national des sciences de l'Univers : UMR8190 (INSU-CNRS 3 rue Michel-Ange, 75794 Paris Cedex 16 - France)
- CNRS - Centre National de la Recherche Scientifique : UMR8190 (France)
6
Università degli Studi di Pavia (Strada Nuova, 65 - 27100 Pavia - Italy)
7
JPL - Jet Propulsion Laboratory (4800 Oak Grove Drive, Pasadena, CA 91109-8099, USA - United States)
- NASA (www.nasa.gov - United States)
- CALTECH - California Institute of Technology (1200 East California Blvd, Pasadena, California 91125 - United States)
8
DLR - Deutsches Zentrum für Luft- und Raumfahrt (Germany)
9
Department of Astronomy of the Mount Holyoke College (50 College Street, South Hadley, Massachusetts 01075 - United States)
- Mount Holyoke College (South Hadley, Massachusetts - United States)
Abstract : The Venus Emissivity Mapper (VEM) is the first flight instrument specially designed with a sole focus on mapping the surface of Venus using the narrow atmospheric windows around 1μm. VEM will provide a global map of surface composition as well as redox state of the surface, providing a comprehensive picture of surface-atmosphere interaction on Venus. In addition, continuous observation of the thermal emission of the Venus will provide tight constraints on current day volcanic activity. These capabilities are complemented by measurements of atmospheric water vapor abundance as well as cloud microphysics and dynamic. Atmospheric data will allow for the accurate correction of atmospheric interference on the surface measurements and represent highly valuable science on their own. A mission combining VEM with a high-resolution radar mapper such as the NASA VOX or the ESA EnVision mission proposals in a low circular orbit will provide key insights in the divergent evolution of Venus.
Document type :
Conference papers
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https://hal-insu.archives-ouvertes.fr/insu-01587304
Contributor : Catherine Cardon Connect in order to contact the contributor
Submitted on : Thursday, September 14, 2017 - 9:48:59 AM
Last modification on : Wednesday, November 17, 2021 - 12:29:15 PM
Contributor : Catherine Cardon Connect in order to contact the contributor
Submitted on : Thursday, September 14, 2017 - 9:48:59 AM
Last modification on : Wednesday, November 17, 2021 - 12:29:15 PM
Links full text
Identifiers
- HAL Id : insu-01587304, version 1
- DOI : 10.1117/12.2275666
Collections
INSU | CNRS | OBSPM | LATMOS | LESIA | UPMC | UVSQ | SORBONNE-UNIVERSITE | UNIV-PARIS7 | USPC | SU-SCIENCES | UNIV-PARIS | UP-SCIENCES | PSL | SU-TI | GS-ENGINEERING | INSTITUT-SCIENCES-LUMIERE
Citation
Jörn Helbert, Ingo Walter, Dennis Wendler, Thomas Widemann, Emmanuel Marcq, et al.. The Venus Emissivity Mapper concept. Proceeding SPIE 10403, Infrared Remote Sensing and Instrumentation XXV, Aug 2017, San Diego, United States. ⟨10.1117/12.2275666⟩. ⟨insu-01587304⟩
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