Results 121 to 130 of about 25,419 (252)
Martian Ionosphere: A Component Due to Solar Protons [PDF]
Carl Sagan, Joseph Veverka
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Mercury's Tidal Love Number h2 ${h}_{2}$ From Co‐Registration of MLA Profiles
Abstract Due to its eccentric orbit, Mercury experiences a varying gravitational pull from the Sun along its orbit, leading to periodic surface tidal deformation. The previous measurement of Mercury's tidal h2 ${h}_{2}$ by Bertone et al. (2021, https://doi.org/10.1029/2020je006683) is based on minimizing height differences at cross‐overs of the Mercury
Haifeng Xiao+5 more
wiley +1 more source
Observational Characteristics of Electron Distributions in the Martian Induced Magnetotail
Abstract Mars's magnetotail represents a unique case within the solar system, embodying both intrinsic and induced magnetic fields. Yet, the electron dynamics within this region have remained largely unexplored. Utilizing nine years of electron and magnetic field data from the Mars Atmosphere and Volatile EvolutioN mission (MAVEN), we conducted a ...
Chi Zhang+10 more
wiley +1 more source
Properties of Solar Wind Current Sheets in the Martian Space Environment
Transient current sheets (CSs) are common magnetic structures in the solar wind that can significantly disturb the planetary space environment and cause space weather phenomena.
Yangjun Chen+8 more
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A Revised Upper Limit of NO_{2} in the Martian Atmosphere [PDF]
Brian O'Leary
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Direct Formation of Structural Components Using a Martian Soil Simulant
Martian habitats are ideally constructed using only locally available soils; extant attempts to process structural materials on Mars, however, generally require additives or calcination.
Brian J. Chow+3 more
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Spectroscopic study of the gas-cap radiation intensity for simulated martian atmospheric probes [PDF]
W. Winovich
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Survival of Microorganisms in a Simulated Martian Environment [PDF]
C. A. Hagen+2 more
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Atmospheric re-entry into the Martian atmosphere with variable lift control [PDF]
H. Ohtakay
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