Results 51 to 60 of about 113,851 (260)

A Simple Subgrid‐Scale Model for Slope Winds on Mars

Earth and Space Science
Global Climate Models (GCMs) are useful tools for simulating the dynamics of Mars atmosphere on a planetary scale. However their coarse resolution (∼100 km) does not allow to capture small‐scale phenomena such as slope winds which can occur over scales ...
T. Pierron, F. Forget, E. Millour, A. Spiga, A. Martinez   +4 more
doaj   +1 more source

Turbulence in the Lower Atmosphere of Mars Enhanced by Transported Dust Particles [PDF]

, 2021
Aymeric Spiga
openalex   +1 more source

Quantification of Carbonates, Oxychlorines, and Chlorine Generated by Heterogeneous Electrochemistry Induced by Martian Dust Activity

Geophysical Research Letters, 2023
Heterogeneous electrochemistry induced by Martian dust activity is an important type of atmosphere‐surface interaction that affects geochemical processes at the Martian surface and in the Martian atmosphere.
Alian Wang, Andrew W. Jackson, Neil C. Sturchio, Jen Houghton, Chuck Y. C. Yan, Kevin S. Olsen, Quincy H. K. Qu   +6 more
doaj   +1 more source

Water ice clouds in a martian global climate model using data assimilation [PDF]

, 2011
The water cycle is one of the key seasonal cycles on Mars, and the radiative effects of water ice clouds have recently been shown to alter the thermal structure of the atmosphere.
Lewis, S. R., Mulholland, D. P., Patel, M. R., Steele, Liam   +3 more
core  

The upper atmosphere and ionosphere of Mars [PDF]

The topics discussed include the following: the dynamic atmosphere of Mars; possible similarities with Earth and Venus; the atmosphere and ionosphere of Mars; solar wind interactions; future approved missions; and possible future ...
Brace, Larry H.
core   +1 more source

Thermal tides in an assimilation of three years of Thermal Emission Spectromenter data from Mars Global Surveyor [PDF]

, 2008
Introduction. Thermal tides are particularly prominent in the Mars atmosphere with the result that temperature and wind fields have a strong dependence on local solar time (LT).
Lewis, S. R., Montabone, L., Wilson, R. J.   +2 more
core  

The atmosphere of Mars [PDF]

Effects of Mariner IV ionospheric data on Mars atmosphere composition ...
Johnson, F. S.
core   +1 more source

The impacts of coronal mass ejections on the space environments of Venus and Mars

地球与行星物理论评
Coronal mass ejections (CME) are solar transients, and their impacts on the planets within the solar system have attracted considerable attention. As neighboring planets within the solar system, Venus and Mars are also directly and indirectly affected by
Qi Xu, Lianghai Xie, Lei Li, Xiaojun Xu
doaj   +1 more source

Volatiles on Mars [PDF]

The long-term evolution of both the atmosphere and the surface of Mars can be understood by examining the history of volatiles in the Mars atmosphere, their non-atmospheric reservoirs, and the processes of exchange between the two.
Jakosky, Bruce M.
core   +1 more source

THz generation from laser-induced breakdown in pressurized molecular gases: on the way to terahertz remote sensing of the atmospheres of Mars and Venus

New Journal of Physics, 2020
The present paper studies the generation of terahertz (THz) radiation in CO _2 in comparison with atmospheric air at a wide range of pressures. We established experimentally and explained theoretically that for these gases there are optimal pressures at ...
Peter M Solyankin, Irina A Nikolaeva, Andrey A Angeluts, Daniil E Shipilo, Nikita V Minaev, Nikolay A Panov, Alexei V Balakin, Yiming Zhu, Olga G Kosareva, Alexander P Shkurinov   +9 more
doaj   +1 more source