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Thermal Conductivity of Multilayer Insulation in the Martian Atmosphere
AbstractThe experimental results of measurements of the thermal conductivity of standard multilayer insulation (MLI) in vacuum and under conditions...
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On the Kinetic Features of Sedimentation of Dust Particles in the Martian Atmosphere
Abstract —The mode of subsidence of layered structures in the ionosphere of Mars has been studied taking into account the compositional features of...
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Photochemical depletion of heavy CO isotopes in the Martian atmosphere
The atmosphere of Mars is enriched in heavy isotopes with respect to Earth as a result of the escape of the atmosphere to space over billions of...
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LIDAR for Investigation of the Martian Atmosphere from the Surface
AbstractThe lidar device as part of the meteorological complex of the ExoMars-2022 landing platform is designed to study Martian aerosol, the...
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The Radiative Gas Dynamics of Spherical Spacecraft in the Martian Atmosphere
AbstractThe problem of radiative-convective heat transfer of spacecraft of the simplest shape in Martian atmosphere is solved. Selection of spherical...
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The Radiative Gas Dynamics of Spacecraft in the Martian Atmosphere
AbstractThe problems of the radiative gas dynamics of the Martian space vehicles MSRO , Pathfinder , and Exomars-2016 are solved using the author’s...
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Dynamical Phenomena in the Martian Atmosphere Through Mars Express Imaging
This review describes the dynamic phenomena in the atmosphere of Mars that are visible in images taken in the visual range through cloud formation...
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Thermal Sounding of the Martian Atmosphere Using the ACS TIRVIM FT-IR Spectrometer on Board ExoMars TGO: Method for Solving the Inverse Problem
AbstractThis paper presents a method for solving the inverse problem of thermal sounding using calibrated data from the ACS TIRVIM experiment on...
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Airglow and Aurora in the Martian Atmosphere: Contributions by the Mars Express and ExoMars TGO Missions
The study of atmospheric emissions from orbit to probe the middle and upper atmosphere of Mars, which started with the Mariner missions, is living a...
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Erratum to: LIDAR for Investigation of the Martian Atmosphere from the Surface
An Erratum to this paper has been published: https://doi.org/10.1134/S0038094623330018
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Attenuation of electromagnetic wave propagation in Martian dust storms
Mars dust storms can significantly affect the radio communication link. In this paper, we proposed a predictive model based on Rayleigh theory. The...
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7 Ground Ice in the Martian Regolith
The long-term existence of extremely cold climate on Mars has led to strong global freezing through upper layers of the planet’s crust that has...
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Upper Atmosphere of Mars
Mars’ atmosphere above 100 km is designated as the upper atmosphere where molecular diffusion dominates (McElroy et al., Science 194:1295–1298,...
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Observations and Modeling of Martian Auroras
Observations of planetary auroras form a new area of planetary exploration from space, especially for nonmagnetic planets since various kinds of...
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Structure of the Martian Dayside Magnetosphere: Two Types
AbstractA set of scientific instruments capable of high temporal resolution measurements onboard the Mars Atmosphere and Volatile Evolution (MAVEN)...
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The Generation of O2 and CO by CO2 Glow Discharge for In-Situ Martian Atmospheric Utilization
AbstractMars has nearly ideal conditions for CO 2 dissociation by glow discharge plasmas. The directly generation of O 2 and CO on Mars was considered...
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Accelerometers of the Meteorological Complex for the Study of the Upper Atmosphere of Mars
AbstractThe accelerometers and the angular velocity sensor, which are part of the meteorological complex of the ExoMars-2022 landing platform (LP),...
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Trace Gases of Mars Atmosphere
The atmosphere of Mars is primarily composed of CO2 (~ 95%) with small amounts of N2 (~ 2.6%), Ar (~ 1.9%, O2 (0.16%) and CO (~ 0.06%). The O3, H2O,...
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Models of the Martian Ionosphere
In this Chapter we have described important models which have been used to study the Martian ionosphere and give several examples of their usage...
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Radiative–Convective Heating of the Surface of the Martian Descent Vehicle MSL with Taking into Account the Turbulent Nature of Flow
AbstractThe three-dimensional computer model based on the Reynolds-averaged Navier–Stokes equations together with the Baldwin–Lomax and Prandtl...
