Seven-year climatology of dust opacity on Mars [PDF]
This paper describes the procedure we have used to produce multi-annual dust scenarios for Martian years 24 to 30 from a multi-instrument dataset of total dust opacity observations.
Forget, F. +3 more
core
Monitoring excited hydroxyl (OH*) airglow is broadly used for characterizing the state and dynamics of the terrestrial atmosphere. Recently, the existence of excited hydroxyl was confirmed using satellite observations in the Martian atmosphere.
Dmitry S. Shaposhnikov +4 more
doaj +1 more source
Advective fluxes influence methane and CO2 soil emissions into the atmosphere on Earth and may drive trace gas emissions in the Mars atmosphere. However, their relevance in the Martian regolith has not been evaluated to date.
D. Viúdez‐Moreiras +6 more
doaj +1 more source
Very high elevation water ice clouds on Mars: Their morphology and temporal behavior [PDF]
Quantitative analysis of Viking images of the martian planetary limb has uncovered the existence and temporal behavior of water ice clouds that form between 50 and 90 km elevation.
Jaquin, Fred
core +1 more source
Erratum to: LIDAR for Investigation of the Martian Atmosphere from the Surface [PDF]
A. N. Lipatov +10 more
openalex +1 more source
A First Look at Carbon and Oxygen Stable Isotope Measurements of Martian Atmospheric C02 by the Phoenix Lander [PDF]
Precise stable isotope measurements of the CO2 in the martian atmosphere have the potential to provide important constraints for our understanding of the history of volatiles, the carbon cycle, current atmospheric processes, and the degree of water/rock ...
Boynton, W.V. +4 more
core +1 more source
Kinetic model of carbonate dissolution in Martian meteorite ALH84001 [PDF]
The magnetites and sulfides located in the rims of carbonate globules in the Martian meteorite ALH84001 have been claimed as evidence of past life on Mars.
Humayun, Munir, Kopp, Robert E.
core +1 more source
An estimation of the mass dragged by the solar wind from Mars’s atmosphere in its geologic history [PDF]
In the past Mars had a denser atmosphere, but it lacks a magnetic field to protect the ionosphere and exosphere from the solar wind. A model for describing the loss of atmosphere in geologic time is presented.
Héctor Javier Durand-Manterola
doaj
Development of a modular central electronic unit (CEU) for data handling and management in Martian atmosphere investigations [PDF]
Luca Marrocchi
openalex +1 more source
Replication Data for: Impact of Novel H2O Cross Sections on the Present-Day Martian Atmosphere
Kayla Smith
openalex +1 more source

