Skip to Main content Skip to Navigation
Poster communications

Venus Emissivity Mapper – Investigating the Atmospheric Structure and Dynamics of Venus' Polar Region

Thomas Widemann 1 Emmanuel Marcq 2 C. Tsang 3 N. Mueller 4 D. Kappel 5 J. Helbert 5 M. D. Dyar 6 S. Smrekar 4
1 LESIA - Laboratoire d'études spatiales et d'instrumentation en astrophysique
2 IMPEC - LATMOS
LATMOS - Laboratoire Atmosphères, Milieux, Observations Spatiales
3 Department of Space Studies [Boulder]
4 JPL - Jet Propulsion Laboratory
5 DLR Institut für Planetenforschung
6 PSI - Planetary Science Institute [Tucson]
Abstract : VEM will map cloud particle modes and their temporal variations, and track cloud-level wind field in the polar vortices. VOX circular polar orbit geometry will provide an unprecedented simultaneous study of both polar regions
Document type :
Poster communications
Complete list of metadatas
https://hal-insu.archives-ouvertes.fr/insu-01672488
Contributor : Catherine Cardon <>
Submitted on : Monday, December 25, 2017 - 5:30:03 PM
Last modification on : Wednesday, September 23, 2020 - 4:36:42 AM

File

Vignette du document
Widemann-Venus.pdf
Files produced by the author(s)

Identifiers

Collections

INSU | CNRS | OBSPM | LATMOS | UPMC | UVSQ | LESIA | SORBONNE-UNIVERSITE | UNIV-PARIS7 | USPC | SU-SCIENCES | UNIV-PARIS | UP-SCIENCES | PSL

Citation

Thomas Widemann, Emmanuel Marcq, C. Tsang, N. Mueller, D. Kappel, et al.. Venus Emissivity Mapper – Investigating the Atmospheric Structure and Dynamics of Venus' Polar Region. 15th Meeting of the Venus Exploration and Analysis Group (VEXAG), Nov 2017, Laurel, Maryland, United States. pp.LPI Contribution No. 2061, 2017. ⟨insu-01672488⟩

Export

BibTeX TEI DC DCterms EndNote

Share

Metrics