Alternate oscillations of Martian hydrogen and oxygen upper atmospheres during a major dust storm
Dust storms on Mars drive water escape to space. Here, the authors show the impact Martian dust storms have on the abundance of atmospheric hydrogen and oxygen, and how this helps to overall oxidize the Martian atmosphere.
Kei Masunaga+13 more
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A distinct ripple-formation regime on Mars revealed by the morphometrics of barchan dunes
Dust storms on Mars drive water escape to space. Here, the authors show the impact Martian dust storms have on the abundance of atmospheric hydrogen and oxygen, and how this helps to overall oxidize the Martian atmosphere.
Lior Rubanenko+4 more
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Simulation of Transient Topside Layer in the Martian Ionosphere
Many Mars missions, e.g., Mariner, Viking, Mars Global Surveyor (MGS), Mars Express (MEX), and Mars Atmosphere and Volatile Evolution (MAVEN), have been launched to study the Martian atmosphere.
Chunhua Jiang, Rong Tian, Lehui Wei
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Global distribution and climate sensitivity of the tropical montane forest nitrogen cycle
Dust storms on Mars drive water escape to space. Here, the authors show the impact Martian dust storms have on the abundance of atmospheric hydrogen and oxygen, and how this helps to overall oxidize the Martian atmosphere.
Justin D. Gay+2 more
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Diurnal Variations of Water Ice in the Martian Atmosphere Observed by Mars Climate Sounder
Simulation studies have proposed a significant thermal effect of water ice clouds on the Martian atmosphere and climate. However, previous studies focused more on seasonal variations but less on short-term changes.
Zhaopeng Wu+4 more
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Effects of Charged Martian Dust on Martian Atmosphere Remote Sensing
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+3 more
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MAVEN Observations of the Interloop Magnetic Reconnections at Mars
Magnetic reconnection between neighboring magnetic field loops, the so-called interloop reconnection, is a common process to drive flares in the solar atmosphere.
Guo Chen+9 more
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Mie scattering and the Martian atmosphere [PDF]
It has been suggested that the discrepancy between radio occultation determinations of the Martian atmospheric surface pressure (3.8 to 7 mb) and those deduced from optical polarization measurements and a simple Rayleigh atmosphere model (about 10 mb) are the results of sub-micron sized aerosols in the Martian atmosphere.
Walter G. Egan, K. M. Foreman
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Outgassing History and Escape of the Martian Atmosphere and Water Inventory [PDF]
The evolution and escape of the martian atmosphere and the planet’s water inventory can be separated into an early and late evolutionary epoch. The first epoch started from the planet’s origin and lasted ∼500 Myr.
H. Lammer+13 more
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Long-Endurance Mars Exploration Flying Vehicle: A Project Brief
The paper presents specifications for the Long-Endurance Mars Exploration Flying Vehicle (LEMFEV), which will be used as future design input data. The specifications are based on the analysis of previous Mars missions and scientific data collected by the
Elena Karpovich+4 more
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