Martian water ice clouds during the 2018 global dust storm as observed by the ACS-MIR channel onboard the Trace Gas Orbiter
Autor: | Aurélien Stcherbinine, Anna Fedorova, Andrew Patrakeev, Franck Montmessin, Alexander Trokhimovskiy, Oleg Korablev, Lucio Baggio, Alexei Shakun, Michael J. Wolff, Gaetan Lacombe, Mathieu Vincendon |
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Přispěvatelé: | PLANETO - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS), Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Space Science Institute [Boulder] (SSI), Space Research Institute of the Russian Academy of Sciences (IKI), Russian Academy of Sciences [Moscow] (RAS), IMPEC - LATMOS, Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS) |
Jazyk: | angličtina |
Rok vydání: | 2020 |
Předmět: |
010504 meteorology & atmospheric sciences
FOS: Physical sciences Atmospheric sciences 01 natural sciences law.invention global dust storm Orbiter Altitude Mars atmosphere Geochemistry and Petrology law Dust storm Earth and Planetary Sciences (miscellaneous) Astrophysics::Galaxy Astrophysics Physics::Atmospheric and Oceanic Physics 0105 earth and related environmental sciences Martian Earth and Planetary Astrophysics (astro-ph.EP) Storm solar occultation Atmosphere of Mars Effects of high altitude on humans Trace gas water ice clouds Geophysics ExoMars TGO 13. Climate action Space and Planetary Science IR spectroscopy [SDU]Sciences of the Universe [physics] Physics::Space Physics Environmental science Astrophysics::Earth and Planetary Astrophysics Astrophysics - Earth and Planetary Astrophysics |
Zdroj: | Journal of Geophysical Research. Planets Journal of Geophysical Research. Planets, Wiley-Blackwell, 2020, 125 (3), pp.e2019JE006300. ⟨10.1029/2019JE006300⟩ |
ISSN: | 2169-9097 2169-9100 |
DOI: | 10.1029/2019JE006300⟩ |
Popis: | The Atmospheric Chemistry Suite (ACS) instrument onboard the ExoMars Trace Gas Orbiter (TGO) ESA-Roscosmos mission began science operations in March 2018. ACS Mid InfraRed (MIR) channel notably provides solar occultation observations of the martian atmosphere in the 2.3 - 4.2 $\mu$m spectral range. Here we use these observations to characterize water ice clouds before and during the MY 34 Global Dust Storm (GDS). We developed a method to detect water ice clouds with mean particle size $\leq$ 2 $\mu$m, and applied it to observations gathered between $L_s=165^\circ$ and $L_s=243^\circ$. We observe a shift in water ice clouds maximum altitudes from about 60 km before the GDS to above 90 km during the storm. These very high altitude, small-sized ($r_\mathrm{eff} \leq 0.3$ $\mu$m) water ice clouds are more frequent during MY34 compared to non-GDS years at the same season. Particle size frequently decreases with altitude, both locally within a given profile and globally in the whole dataset. We observe that the maximum altitude at which a given size is observed can increase during the GDS by several tens of km for certain sizes. We notably notice some large water ice particles ($r_\mathrm{eff}\geq1.5$ $\mu$m) at surprisingly high altitudes during the GDS (50 - 70 km). These results suggest that GDS can significantly impact the formation and properties of high altitude water ice clouds as compared to the usual perihelion dust activity. |
Databáze: | OpenAIRE |
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