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      The atmosphere of Mars as observed by InSight

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      Nature Geoscience
      Springer Science and Business Media LLC
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          Gravity wave dynamics and effects in the middle atmosphere

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            Mars Reconnaissance Orbiter's High Resolution Imaging Science Experiment (HiRISE)

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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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                Author and article information

                Journal
                Nature Geoscience
                Nat. Geosci.
                Springer Science and Business Media LLC
                1752-0894
                1752-0908
                February 24 2020
                Article
                10.1038/s41561-020-0534-0
                8767a41c-6bb9-4037-8595-222144e15f0b
                © 2020

                http://www.springer.com/tdm

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