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Precipitation induced by explosive volcanism on Mars and its implications for unexpected equatorial ice. [PDF]

Nat Commun
Hamid SS, Kerber L, Clarke AB.
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Upper Atmosphere and Ionosphere of Mars

Science, 1966
It is argued that the single-layer ionosphere at 125 kilometers discovered in the Mariner IV occultation experiment is an F1 region coinciding with the ultraviolet photoionization peak. The CO 2 density there must be of the order of 10 11 molecules per cubic centimeter.
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The Atmosphere of Mars

1973
The main emphasis of this review will be on Martian aeronomy, here defined to be the interaction of solar UV radiation with the atmosphere of Mars. A general outline of contemporary knowledge of the chemical composition and of the thermal structure of the Martian atmosphere, necessary for aeronomical calculations, is given in Sections 2 and 3 ...
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Ionization in the Atmosphere of Mars

Proceedings of the IRE, 1929
Assuming that the atmosphere at the surface of Mars consists of ⅕ oxygen and ⅘ other gases, as nitrogen, etc., the composition of the atmosphere to great heights is calculated, just as was done for the earth, from the actions of gas diffusion and gravity. The electron density in the atmosphere of Mars due to the ultraviolet light of the sun is found to
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The atmosphere and haze of Mars

Journal of Geophysical Research, 1960
The 'blue haze' is an absorbing smoke, dark as soot in reflection, red in transmission. Its currently accepted explanation by pure scattering (omnidirectional or forward) is untenable, as it would either increase the surface brightness of fall to obscure the surface details.
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The Atmosphere and Climate of Mars

2017
Humanity has long been fascinated by the planet Mars. Was its climate ever conducive to life? What is the atmosphere like today and why did it change so dramatically over time? Eleven spacecraft have successfully flown to Mars since the Viking mission of the 1970s and early 1980s.
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Emirates Mars Mission Characterization of Mars Atmosphere Dynamics and Processes

Space Science Reviews, 2021
Andrew R Jones, David Brain, Bruce Jakosky   +2 more
exaly  

The Atmospheres of Mars and Venus

1965
The nine planets of our solar system can be grouped into two distinct classes: (1) the terrestrial planets, which include Mercury, Venus, Earth and Mars; and (2) the major planets — Jupiter, Saturn, Uranus, Neptune and Pluto.
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A multiannual record of gravity wave activity in Mars’s lower atmosphere from on-planet observations by the Mars Climate Sounder

Icarus, 2020
Nicholas Heavens, David Kass, Armin Kleinböhl   +2 more
exaly  

The Atmosphere of Mars

Scientific American, 1977
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