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      Evaluating the Wind-Induced Mechanical Noise on the InSight Seismometers

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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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            Seismology on Mars

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              Planetary seismology

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                Author and article information

                Journal
                Space Science Reviews
                Space Sci Rev
                Springer Nature America, Inc
                0038-6308
                1572-9672
                October 2017
                November 29 2016
                October 2017
                : 211
                : 1-4
                : 429-455
                Article
                10.1007/s11214-016-0311-y
                ca8c2dac-1e6f-4b31-aff2-7709366c5db2
                © 2017

                http://www.springer.com/tdm

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