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      Pressure observations by the Curiosity rover: Initial results : MSL PRESSURE OBSERVATIONS: INITIAL RESULTS

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          Improved general circulation models of the Martian atmosphere from the surface to above 80 km

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            The Mars Pathfinder Atmospheric Structure Investigation/Meteorology (ASI/MET) Experiment

            The Mars Pathfinder atmospheric structure investigation/meteorology (ASI/MET) experiment measured the vertical density, pressure, and temperature structure of the martian atmosphere from the surface to 160 km, and monitored surface meteorology and climate for 83 sols (1 sol = 1 martian day = 24.7 hours). The atmospheric structure and the weather record are similar to those observed by the Viking 1 lander (VL-1) at the same latitude, altitude, and season 21 years ago, but there are differences related to diurnal effects and the surface properties of the landing site. These include a cold nighttime upper atmosphere; atmospheric temperatures that are 10 to 12 degrees kelvin warmer near the surface; light slope-controlled winds; and dust devils, identified by their pressure, wind, and temperature signatures. The results are consistent with the warm, moderately dusty atmosphere seen by VL-1.
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              Meteorological results from the surface of Mars: Viking 1 and 2

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                Author and article information

                Journal
                Journal of Geophysical Research: Planets
                J. Geophys. Res. Planets
                Wiley-Blackwell
                21699097
                January 2014
                January 2014
                : 119
                : 1
                : 82-92
                Article
                10.1002/2013JE004423
                26213667
                fe163dc7-0c1c-4c5c-9e2a-a21ac76d9af9
                © 2014

                http://doi.wiley.com/10.1002/tdm_license_1.1

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