Results 11 to 20 of about 722,187 (326)
Strong Depletion of 13C in CO Induced by Photolysis of CO2 in the Martian Atmosphere, Calculated by a Photochemical Model [PDF]
The isotopic signature of atmospheric carbon offers a unique tracer for the history of the Martian atmosphere and the origin of organic matter on Mars. The photolysis of CO _2 is known to induce strong isotopic fractionation of the carbon between CO _2 ...
Tatsuya Yoshida+9 more
doaj +2 more sources
Dust tides and rapid meridional motions in the Martian atmosphere during major dust storms. [PDF]
The atmosphere of Mars is strongly affected by the spatial and temporal variability of airborne dust. However, global dust variability within a sol (Martian day) is still poorly understood.
Wu Z, Li T, Zhang X, Li J, Cui J.
europepmc +2 more sources
Properties and models of the Martian bow shock
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+4 more
doaj +1 more source
Isotopes of chlorine from HCl in the Martian atmosphere
Hydrogen chloride gas was recently discovered in the atmosphere of Mars during southern summer seasons. Its connection with potential chlorine reservoirs and the related atmospheric chemistry is now of particular interest and actively studied ...
A. Trokhimovskiy+9 more
semanticscholar +1 more source
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
Carbonate formation events in ALH 84001 trace the evolution of the Martian atmosphere. [PDF]
Shaheen R+4 more
europepmc +2 more sources
What Is the Radiation Impact of Extreme Solar Energetic Particle Events on Mars?
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+2 more
doaj +1 more source
THE MARTIAN ATMOSPHERIC BOUNDARY LAYER [PDF]
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.
Hannu Savijärvi+13 more
openaire +4 more sources
Nonmigrating tides in the Martian atmosphere as observed by MAVEN IUVS [PDF]
Daniel Lo+16 more
openalex +2 more sources
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+6 more
doaj +1 more source