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Physical parameters of the martian atmosphere

Earth, Moon, and Planets, 1989
The following physical parameters have been computed from 0 to 200 km altitude; (1) pressure, (2) density (3), speed of sound, (4) density, (5) number density, (6) mean free path, (7) viscosity, (8) pressure scale, (9) mean particle velocity, (10) collisional frequency and (11) columnar mass.
Basil Petropoulos, Constantin Macris
openaire   +1 more source

Making oxygen from the Martian atmosphere 

Aether, 2022
The possibility of a manned mission to Mars is gaining traction. But how do you create the oxygen necessary for the astronauts to remain on the planet and, more importantly, how do you develop the rocket fuel necessary to bring them back? MOXIE is the answer.
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Change in the Martian Atmosphere

1999
There are several lines of evidence that the atmosphere of Mars has significantly evolved over the history of the planet. Because Mars does not have a strong intrinsic magnetic field, the atmosphere is eroded by interactions with the solar wind. Conditions in the early solar-system significantly enhanced this loss, notably the component due to solar ...
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Martian Atmosphere Boundary Layer Code

26th Thermophysics Conference, 1991
HARTMUT LEGNER   +3 more
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Evolution of the Martian atmosphere

Advances in Space Research, 1997
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FTS of the Martian Atmosphere

2009
Formisano V   +4 more
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