A test case: new retrievals of ozone at the terminator on Mars

Authors :: Piccialli, Arianna
Vandaele, Ann Carine
Robert, Séverine
Daerden, Frank
Viscardy, Sébastien
Neary, Lori
Aoki, Shohei
Wilquet, Valérie
Lefèvre, Franck
Määttänen, Anni
Montmessin, Franck
Belgian Institute for Space Aeronomy / Institut d'Aéronomie Spatiale de Belgique (BIRA-IASB)
Fonds National de la Recherche Scientifique [Bruxelles] (FNRS)
PLANETO - LATMOS
Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS)
Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
Source :: European Planetary Science Congress 2017, European Planetary Science Congress 2017, Sep 2017, Riga, Latvia. pp.EPSC2017-530
Publication Year :: 2017
Publisher :: HAL CCSD, 2017.
Abstract: International audience; ASIMUT, the BIRA-IASB radiative transfer code, was modified in order to take into account the changes in the atmospheric composition and structure across the martian day/night terminator.Here, we will discuss the impact of this implementation on the retrievals of ozone profiles derived from SPICAM solar occultations in the ultraviolet.

Subjects :: [SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP]

Language :: English
Database :: OpenAIRE
Journal :: European Planetary Science Congress 2017, European Planetary Science Congress 2017, Sep 2017, Riga, Latvia. pp.EPSC2017-530
Accession number :: edsair.dedup.wf.001..53fb39ed0205b47b34dea10667367085

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