Abstract
GEOPHYSICAL RESEARCH LETTERS,
VOL. 35,
L09202,
5 PP., 2008
doi:10.1029/2008GL033388
Observation of atmospheric tides in the Martian exosphere using Mars Reconnaissance Orbiter radio tracking data
Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, Massachusetts, USA
Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, Massachusetts, USA
Solar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, Maryland, USA
Solar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, Maryland, USA
Solar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, Maryland, USA
Based on the perturbations of the trajectory of the Mars Reconnaissance Orbiter due to atmospheric drag, we estimate, using Precision Orbit Determination, the density of the Martian exosphere near 250 km altitude with much better temporal (and therefore spatial) resolution than previously possible with this method. Small longitudinal density variations are observed to be consistent over long time periods. Although they appear fixed with respect to the planet, we interpret them as non-migrating tides because of the Sun-synchronous spacecraft orbit. Similar tides were observed previously by MGS at much lower altitude (∼125 km), and our results agree to first order with the MGS findings.
Received 28 January 2008; accepted 24 March 2008; published 7 May 2008.
Citation: (2008), Observation of atmospheric tides in the Martian exosphere using Mars Reconnaissance Orbiter radio tracking data, Geophys. Res. Lett., 35, L09202, doi:10.1029/2008GL033388.
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