MAVEN IUVS in Stellar Occultation Mode: A First Look at Martian Atmospheric Density and Temperature Profiles - Archive ouverte HAL
Poster De Conférence Année : 2015

MAVEN IUVS in Stellar Occultation Mode: A First Look at Martian Atmospheric Density and Temperature Profiles

Résumé

We will present a first series of results obtained by IUVS using stellar occultation, which allows one to retrieve CO2 density and temperature from 30 to 150 km.

Domaines

Planétologie et astrophysique de la terre [astro-ph.EP]

Catherine Cardon  : Connectez-vous pour contacter le contributeur

https://hal.science/hal-01130627

Soumis le : jeudi 12 mars 2015-10:04:04

Dernière modification le : dimanche 6 octobre 2024-14:44:03

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Dates et versions

hal-01130627 , version 1 (12-03-2015)

Identifiants

Citer

Franck Montmessin, N. M. Schneider, A. I. Stewart, Justin Deighan, Roger Yelle, et al.. MAVEN IUVS in Stellar Occultation Mode: A First Look at Martian Atmospheric Density and Temperature Profiles. 46th Lunar and Planetary Science Conference, Mar 2015, The Woodlands, United States. 46, LPI Contribution No. 1832, p.2026, 2015. ⟨hal-01130627⟩

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INSU UPMC CNRS LATMOS UVSQ UNIV-PARIS-SACLAY SORBONNE-UNIVERSITE SU-SCIENCES GS-ENGINEERING GS-PHYSIQUE INSTITUT-SCIENCES-LUMIERE
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