Low-harmonic magnetosonic waves observed by the Van Allen Probes

TitleLow-harmonic magnetosonic waves observed by the Van Allen Probes
Publication TypeJournal Article
Year of Publication2015
AuthorsPosch, JL, Engebretson, MJ, Olson, CN, Thaller, SA, Breneman, AW, Wygant, JR, Boardsen, SA, Kletzing, CA, Smith, CW, Reeves, GD
JournalJournal of Geophysical Research: Space Physics
Date Published07/2015
Keywordsequatorial noise; inner magnetosphere; magnetosonic waves; Van Allen Probes; waves in plasmas
AbstractPurely compressional electromagnetic waves (fast magnetosonic waves), generated at multiple harmonics of the local proton gyrofrequency, have been observed by various types of satellite instruments (fluxgate and search coil magnetometers and electric field sensors), but most recent studies have used data from search coil sensors, and many have been restricted to high harmonics. We report here on a survey of low-harmonic waves, based on electric and magnetic field data from the EFW double probe and EMFISIS fluxgate magnetometer instruments, respectively, on the Van Allen Probes spacecraft during its first full precession through all local times, from October 1, 2012 through July 13, 2014. These waves were observed both inside and outside the plasmapause (PP), at L shells from 2.4 to ~6 (the spacecraft apogee), and in regions with plasma number densities ranging from 10 to >1000 cm-3. Consistent with earlier studies, wave occurrence was sharply peaked near the magnetic equator. Waves appeared at all local times but were more common from noon to dusk, and often occurred within three hours after substorm injections. Outside the PP occurrence maximized broadly across noon, and inside the PP occurrence maximized in the dusk sector, in an extended plasmasphere. We confirm recent ray-tracing studies showing wave refraction and/or reflection at PP-like boundaries. Comparison with waveform receiver data indicates that in some cases these low-harmonic magnetosonic wave events occurred independently of higher-harmonic waves; this indicates the importance of including this population in future studies of radiation belt dynamics.
URLhttp://doi.wiley.com/10.1002/2015JA021179
DOI10.1002/2015JA021179
Short TitleJ. Geophys. Res. Space Physics


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