Martian Temperature Profiles Measured by MAVEN and MRO from 20 to 160 km
| Autor: | Gröller, Hannes, Yelle, Roger V., Koskinen, Tommi T., Montmessin, Franck, Lacombe, Gaetan, Kass, David, Kleinböhl, Armin, Schofield, T., Mccleese, D. J., Schneider, Nick, Deighan, Justin, Jain, S.K., Jakosky, Bruce M. |
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| Přispěvatelé: | Lunar and Planetary Laboratory [Tucson] (LPL), University of Arizona, 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), Jet Propulsion Laboratory (JPL), NASA-California Institute of Technology (CALTECH), Laboratory for Atmospheric and Space Physics [Boulder] (LASP), University of Colorado [Boulder], Cardon, Catherine |
| Jazyk: | angličtina |
| Rok vydání: | 2016 |
| Předmět: |
Physics::Space Physics
[SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP] [SDU.ASTR.EP] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP] Astrophysics::Earth and Planetary Astrophysics Physics::Atmospheric and Oceanic Physics |
| Zdroj: | LPSC 2016 47th Lunar and Planetary Science Conference 47th Lunar and Planetary Science Conference, Mar 2016, The Woodlands, Texas, United States. pp.1811 |
| Popis: | International audience; We combined the temperature profile retrieved from the Imaging UltraViolet Spectrometer (IUVS) on Mars Atmosphere and Volatile EvolutioN (MAVEN) [1] and from the Mars Climate Sounder (MCS) on Mars Reconnaissance Orbiter (MRO) [2] to obtain a measured temperature profiles spanning the altitude range from the lower (~20 km) up to the upper (~160 km) atmosphere. A temperature profile that covers such a large altitude range will allow us to investigate coupling among atmospheric regions both for static structures controlled by radiative exchange and for propagating structures such as tides and waves. To construct the merged temperature profile we required IUVS and MCS measurements at similar locations (latitude, longitude, and local time). The latitude and local time distribution of the measurements is shown. |
| Databáze: | OpenAIRE |
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