Results 1 to 10 of about 711,511 (171)

Dust tides and rapid meridional motions in the Martian atmosphere during major dust storms. [PDF]

open access: yesNat Commun, 2020
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]

open access: yesJ Geophys Res Planets, 2018
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

open access: greenOxford Research Encyclopedia of Planetary Science, 2018
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
openalex   +3 more sources

Laser Ablation Sampling With Low-Power Plasma: A LA-MIP-MS Instrument for Spaceflight. [PDF]

open access: yesRapid Commun Mass Spectrom
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]

open access: bronze, 2017
Matteo Crismani   +15 more
openalex   +2 more sources

Strong Depletion of 13C in CO Induced by Photolysis of CO2 in the Martian Atmosphere, Calculated by a Photochemical Model [PDF]

open access: yesThe Planetary Science Journal, 2023
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]

open access: yesProc Natl Acad Sci U S A, 2015
Shaheen R   +4 more
europepmc   +2 more sources

Nonmigrating tides in the Martian atmosphere as observed by MAVEN IUVS [PDF]

open access: bronze, 2015
Daniel Lo   +16 more
openalex   +2 more sources

Interannual similarity in the Martian atmosphere during the dust storm season [PDF]

open access: bronze, 2016
D. M. Kass   +4 more
openalex   +2 more sources

Martian Dust Storms and Gravity Waves: Disentangling Water Transport to the Upper Atmosphere [PDF]

open access: yesJournal of Geophysical Research: Planets, 2022
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

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