Results 1 to 10 of about 25,262 (186)

Meteoric Metal Chemistry in the Martian Atmosphere [PDF]

Journal of Geophysical Research: Planets, 2018
AbstractRecent measurements by the Imaging Ultraviolet Spectrograph (IUVS) instrument on NASA's Mars Atmosphere and Volatile EvolutioN mission show that a persistent layer of Mg+ ions occurs around 90 km in the Martian atmosphere but that neutral Mg atoms are not detectable.
J. M. C. Plane, J. D. Carrillo‐Sanchez, T. P. Mangan, M. M. J. Crismani, N. M. Schneider, A. Määttänen   +5 more
openaire   +6 more sources

Impact sculpting of the early martian atmosphere [PDF]

Science Advances
Intense bombardment of solar system planets in the immediate aftermath of protoplanetary disk dissipation has played a key role in their atmospheric evolution. During this epoch, energetic collisions will have removed substantial masses of gas from rocky planet atmospheres.
Shorttle, Oliver, Saeidfirozeh, Homa, Rimmer, Paul Brandon, Laitl, Vojtĕch, Kubelík, Petr, Petera, Lukáš, Ferus, Martin   +6 more
openaire   +7 more sources

Bow shock oscillations of Mars under weakly disturbed solar wind conditions [PDF]

Nature Communications
Bow shock, where the solar wind first encounters the Martian environment, reflects the complex interplay between the solar wind and Martian upper atmosphere and crustal fields.
Long Cheng, Yuming Wang, Yingjuan Ma, Robert Lillis, Jasper Halekas, Benoit Langlais, Tielong Zhang, Aibing Zhang, Guoqiang Wang, Sudong Xiao, Zhuxuan Zou, Yutian Chi, Xinjun Hao, Yiren Li, Zonghao Pan, Kai Liu   +15 more
doaj   +2 more sources

Effects of Charged Martian Dust on Martian Atmosphere Remote Sensing

Remote Sensing, 2022
In this paper, the extinction property and optical depth of charged Martian dust at infrared band 3 THz–300 THz are studied using the Mie scattering theory.
Xuebang Gao, Li Xie, Xuqiang Dou, Jun Zhou   +3 more
doaj   +2 more sources

Discovery of a wind-driven diamagnetic current system in the Martian magnetosphere [PDF]

Scientific Reports
Magnetic fields around Mars shape the pathways of energy input into, and ion escape from, the Martian atmosphere, thereby potentially affecting the atmospheric evolution of Mars.
Yuki Harada, Robert J. Lillis, Matthew O. Fillingim, Shun Imajo, Takuto Minami, Yingjuan Ma, Jacob R. Gruesbeck, Gina A. DiBraccio, Jared R. Espley   +8 more
doaj   +2 more sources

Properties and models of the Martian bow shock

地球与行星物理论评, 2021
Mars does not have a global magnetic field of the internal origin, thus, the solar wind plasma can interact directly with the upper atmosphere and the ionosphere and be shocked with the mass-loading and magnetic pileup processes.
Yifan Li, Jiding Wen, Yuan Pan, Haibo Lin, Jianpeng Guo   +4 more
doaj   +1 more source

Methodology of estimation the parameters permissible values of the aerodynamic and inertial asymmetry of the martian probe

Космические аппараты и технологии, 2023
A technique for estimating small permissible values of the parameters of the aerodynamic and inertial asymmetry of an unguided space probe in the rarefied layers of the Martian atmosphere is considered.
I. Bakry
doaj   +1 more source

What Is the Radiation Impact of Extreme Solar Energetic Particle Events on Mars?

Space Weather, 2023
Solar Energetic Particles (SEP) are one of the major sources of the Martian radiation environment. It is important to understand the SEP‐induced Martian radiation environment for future human habitats on Mars.
Jian Zhang, Jingnan Guo, Mikhail I. Dobynde   +2 more
doaj   +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, Shuanggen Jin, Jiandong Liu, Yawen Li   +3 more
doaj   +1 more source

THE MARTIAN ATMOSPHERIC BOUNDARY LAYER [PDF]

Reviews of Geophysics, 2011
The planetary boundary layer (PBL) represents the part of the atmosphere that is strongly influenced by the presence of the underlying surface and mediates the key interactions between the atmosphere and the surface. On Mars, this represents the lowest 10 km of the atmosphere during the daytime.
Petrosyan, A., Galperin, B., Larsen, S. E., Lewis, S., Määttänen, Anni, Read, P. L., Rennó, N., Rogberg, L. P. H. T., Savijärvi, H., Siili, T., Spiga, A., Toigo, A., Vazquez, L.   +12 more
openaire   +3 more sources