Computer Science – Sound
Scientific paper
May 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004agusmsa31a..03e&link_type=abstract
American Geophysical Union, Spring Meeting 2004, abstract #SA31A-03
Computer Science
Sound
2459 Planetary Ionospheres (5435, 5729, 6026, 6027, 6028), 2483 Wave/Particle Interactions, 2752 Mhd Waves And Instabilities, 5464 Remote Sensing, 6225 Mars
Scientific paper
Recently, general characterizations have been made of the magnetic oscillations observed in the Martian magnetosheath and below the magnetic pileup boundary. We expand upon that work to examine in detail the magnetic oscillations at the lowest observed altitudes. We find that low frequency magnetic oscillations at or below the proton gyrofrequency are consistently observed at altitudes as low as 200 km. We discuss the physical origin of these waves and what this implies about the plasma from which the waves originate. We also note the relevance of these waves in the exploration of the deep subsurface using inductive sounding techniques such as those found in magnetotelluric and magnetic gradiometry methods.
Cloutier Paul A.
Delory Gregory T.
Espley Jared R.
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