Results 151 to 160 of about 76,454 (246)
Abstract The western delta fan in Jezero crater hosts one of Mars's best‐preserved examples of fluvial accretion surfaces, recently investigated by NASA's Perseverance Rover. Erosional windows reveal this geologic unit, which records evidence of fluvial point bar deposition.
Kartikeya S. Sangwan +2 more
wiley +1 more source
Atmospheric re-entry into the Martian atmosphere with variable lift control [PDF]
H. Ohtakay
openalex +1 more source
Phase Boundaries Among Three Hydrous Ferric Sulfates and Their Implications for Mars
Abstract Ferric sulfate minerals have been identified by orbital and landed missions at multiple locations on Mars and are the most common minerals in the Acid Mine Drainage (AMD) system on Earth. The occurrences and the speciation of ferric sulfates are very sensitive to variations in environmental conditions, such as temperature (T), relative ...
Erbin Shi +3 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
doaj +1 more source
The Abundance and Temperature of CO_{2} in the Martian Atmosphere
M. J. S. Belton, D. M. Hunten
openalex +1 more source
Using Venus, Earth, and Mars to Understand Exoplanet Volatile and Climate Evolution
Abstract Venus, Earth, and Mars exhibit a wide range of interactions between their deep interiors, surfaces, lower and upper atmospheres, and the Sun, with commensurate variations in the nature of their atmospheres and evolution of their volatiles. By examining these worlds' characteristics and behavior, we can gain some understanding of the breadth of
Bruce M. Jakosky, Paul K. Byrne
wiley +1 more source
The detection of Martian polar ice cap change patterns is important for understanding their effects on driving Mars’s global water cycle and for regulating atmospheric circulation.
Weiye Xu +7 more
doaj +1 more source
Martian and terrestrial dust devils [PDF]
When dust devils or convective vortices form they can be identified by specific meteorological parameters, a ‘signature’.
Ringrose, Tim, Zarnecki, John
core
Measurement of the Abundance of CO_{2} in the Martian Atmosphere
N. P. Carleton +4 more
openalex +1 more source

