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Low-frequency waves in the Martian magnetosphere and their response to upstream solar wind driving conditions
Journal article   Open access   Peer reviewed

Low-frequency waves in the Martian magnetosphere and their response to upstream solar wind driving conditions

Suranga Ruhunusiri, J. S. Halekas, J. E. P. Connerney, J. R. Espley, J. P. McFadden, D. E. Larson, D. L. Mitchell, C. Mazelle and B. M. Jakosky
Geophysical research letters, Vol.42(21), pp.8917-8924
11/16/2015
DOI: 10.1002/2015GL064968
url
https://doi.org/10.1002/2015GL064968View
Published (Version of record) Open Access

Abstract

We characterize low-frequency plasma waves in the Martian magnetosphere and in the upstream region by using transport ratios. To compute the transport ratios, we use Mars Atmosphere and Volatile EvolutioN mission's (MAVEN) solar wind ion analyzer and suprathermal and thermal ion composition instrument measurements of the ion moments and the magnetometer measurements of the magnetic field. We find that the Alfvén waves are the most dominant wave mode in the upstream region and the magnetosheath. Fast waves are found frequently near the bow shock and the magnetic pileup boundary. Mirror and slow waves, on the other hand, occur much less frequently. We also find that the Alfvén and fast wave occurrences vary dominantly near the bow shock in response to the solar wind dynamic pressure.
magnetosphere Mars MAVEN MHD plasma waves

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