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
Meteoric Metal Chemistry in the Martian Atmosphere. [PDF]
Recent measurements by the Imaging Ultraviolet Spectrograph (IUVS) instrument on NASA's Mars Atmosphere and Volatile EvolutioN mission show that a persistent layer of Mg+ ions occurs around 90 km in the Martian atmosphere but that neutral Mg atoms are ...
Plane JMC +5 more
europepmc +2 more sources
Clouds in the Martian Atmosphere
Although resembling an extremely dry desert, planet Mars hosts clouds in its atmosphere. Every day somewhere on the planet a part of the tiny amount of water vapor held by the atmosphere can condense as ice crystals to form mainly cirrus-type clouds. The
Anni Määttänen, Franck Montmessin
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Laser Ablation Sampling With Low-Power Plasma: A LA-MIP-MS Instrument for Spaceflight. [PDF]
ABSTRACT Rationale Inductively coupled plasma (ICP) is a commonly used ion source for mass spectrometry‐based chemical analysis of a wide range of materials. Traditional ICP ion sources use high power (> 1000 W) and significant gas flow (> 10 L/min), rendering them unsuitable for spaceflight, as they are too resource‐intensive for planetary spacecraft.
Farcy BJ +11 more
europepmc +2 more sources
Detection of a persistent meteoric metal layer in the Martian atmosphere [PDF]
Matteo Crismani +15 more
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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 CO2 is known to induce strong isotopic fractionation of the carbon between CO2 and ...
Tatsuya Yoshida +9 more
semanticscholar +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
Nonmigrating tides in the Martian atmosphere as observed by MAVEN IUVS [PDF]
Daniel Lo +16 more
openalex +2 more sources
Interannual similarity in the Martian atmosphere during the dust storm season [PDF]
D. M. Kass +4 more
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Martian Dust Storms and Gravity Waves: Disentangling Water Transport to the Upper Atmosphere [PDF]
Simulations with the Max Planck Institute Martian general circulation model for Martian years 28 and 34 reveal details of the water “pump” mechanism and the role of gravity wave (GW) forcing.
D. Shaposhnikov +4 more
semanticscholar +1 more source

