Results 41 to 50 of about 722,187 (326)
Gravity waves and high‐altitude CO2 ice cloud formation in the Martian atmosphere [PDF]
, 2015 We present the first general circulation model simulations that quantify and reproduce patches of extremely cold air required for CO2 condensation and cloud formation in the Martian mesosphere.
Erdal Yiğit, A. Medvedev, P. Hartogh
semanticscholar +1 more source
Martian Proton Aurora Brightening Reveals Atmospheric Ion Loss Intensifying
Geophysical Research Letters, 2023 The Martian proton aurora is a distinct aurora phenomenon resulting from the direct deposition of solar wind energy into Mars' dayside atmosphere. What solar wind parameters influence the aurora activity in the short term is yet unknown, as are the ...
Fei He +12 more
doaj +1 more source
Improved general circulation models of the Martian atmosphere from the surface to above 80 km
, 1999 We describe a set of two “new generation” general circulation models of the Martian atmosphere derived from the models we originally developed in the early 1990s.
F. Forget +8 more
semanticscholar +1 more source
Thermospheric density responses to Martian dust storm in autumn based on MAVEN data
Geodesy and Geodynamics, 2022 The unique seasonal surface dust storms on Mars have a significant impact on the Martian atmosphere. However, due to the lack of observations, semi-empirical models are difficult to simulate the density changes in the thermosphere with the existence of ...
Peng Han +3 more
doaj
Earth – Mars Similarity Criteria for Martian Vehicles [PDF]
INCAS Bulletin, 2010 In order to select the most efficient kind of a martian exploring vehicle, the similarity criteria are deduced from the equilibrium movement in the terrestrial and martian conditions.
Octavian TRIFU, George SAVU
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Cloud trains associated with Martian Mountain Lee Waves on the eastern side of the Phlegra Montes
Earth, Planets and Space, 2023 Mountain lee waves have often been observed on the eastern side of the Phlegra Montes as wave trains visualized by water ice clouds in the Martian atmosphere. The seasonality and formation condition of these lee waves and associated cloud trains have not
Kazunori Ogohara, Maaya Ro
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Distribution of Dune Landform on Mars
Frontiers in Astronomy and Space Sciences, 2022 Dune landforms are widely distributed on Mars and contain abundant information about the Martian atmosphere and sedimentary environment. At present, the understanding of Martian dunes and their environmental significance still needs to be further ...
Li Chao, Dong Zhibao
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Earth, Planets and Space, 2021 The mass spectrum analyzer (MSA) will perform in situ observations of ions and magnetic fields around Phobos as part of the Martian Moons eXploration (MMX) mission to investigate the origin of the Martian moons and physical processes in the Martian ...
Shoichiro Yokota +16 more
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Evolution of the Martian Atmosphere [PDF]
Icarus, 1994 Carbon dioxide, nitrogen, and the nonradiogenic and radiogenic noble gases are tracked from primordial inventories to their present states in a revised model of atmospheric evolution on Mars. Elemental and isotopic abundances evolve by hydrodynamic escape, impact erosion, outgassing, sputtering, photochemical escape of nitrogen, and carbonate formation
openaire +2 more sources
Nucleation studies in the Martian atmosphere [PDF]
Journal of Geophysical Research: Planets, 2005 We developed models for unary nucleation of water and carbon dioxide in the Martian atmosphere. Both homogeneous and heterogeneous nucleation on dust particles were studied. Our models are based on classical theory. We compare results of different adsorption approaches.
Määttänen, Anni +6 more
openaire +3 more sources