Journal article
Low-frequency waves in the Martian magnetosphere and their response to upstream solar wind driving conditions
Geophysical research letters, Vol.42(21), pp.8917-8924
11/16/2015
DOI: 10.1002/2015GL064968
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.
Details
- Title: Subtitle
- Low-frequency waves in the Martian magnetosphere and their response to upstream solar wind driving conditions
- Creators
- Suranga Ruhunusiri - University of IowaJ. S. Halekas - University of IowaJ. E. P. Connerney - Goddard Space Flight CenterJ. R. Espley - Goddard Space Flight CenterJ. P. McFadden - University of California, BerkeleyD. E. Larson - University of California, BerkeleyD. L. Mitchell - Space Sciences Laboratory, University of California, California, Berkeley, USAC. Mazelle - Institut de Recherche en Astrophysique et PlanétologieB. M. Jakosky - University of Colorado Boulder
- Resource Type
- Journal article
- Publication Details
- Geophysical research letters, Vol.42(21), pp.8917-8924
- DOI
- 10.1002/2015GL064968
- ISSN
- 0094-8276
- eISSN
- 1944-8007
- Publisher
- Blackwell Publishing Ltd
- Number of pages
- 8
- Language
- English
- Date published
- 11/16/2015
- Academic Unit
- Physics and Astronomy
- Record Identifier
- 9984429037002771
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