Excitation of nightside magnetosonic waves observed by Van Allen Probes

TitleExcitation of nightside magnetosonic waves observed by Van Allen Probes
Publication TypeJournal Article
Year of Publication2014
AuthorsZhou, Q, Xiao, F, Yang, C, Liu, S, Kletzing, CA, Kurth, WS, Hospodarsky, GB, Spence, HE, Reeves, GD, Funsten, HO, Blake, JB, Baker, DN, Wygant, JR
JournalJournal of Geophysical Research: Space Physics
Paginationn/a - n/a
Date Published11/2014
Keywordsmagnetosonic wave; RBSP results; Van Allen Probes; wave-particle interaction
AbstractDuring the recovery phase of the geomagnetic storm on 30-31 March 2013, Van Allen Probe A detected enhanced magnetosonic (MS) waves in a broad range of L =1.8-4.7 and MLT =17-22 h, with a frequency range ~10-100 Hz. In the meanwhile, distinct proton ring distributions with peaks at energies of ~10 keV, were also observed in L =3.2-4.6 and L =5.0-5.6. Using a subtracted bi-Maxwellian distribution to model the observed proton ring distribution, we perform three dimensional ray tracing to investigate the instability, propagation and spatial distribution of MS waves. Numerical results show that nightside MS waves are produced by proton ring distribution and grow rapidly from the source location L =5.6 to the location L =5.0, but remain nearly stable at locations L <5.0 Moreover, waves launched toward lower L-shells with different initial azimuthal angles propagate across different MLT regions with divergent paths at first, then gradually turn back toward higher L-shells and propagate across different MLT regions with convergent paths. The current results further reveal that MS waves are generated by a ring distribution of ~10 keV proton and proton ring in one region can contribute to the MS wave power in another region.
Short TitleJ. Geophys. Res. Space Physics

Page Last Modified: November 3, 2014