Van Allen Probes observation and modeling of chorus excitation and propagation during weak geomagnetic activities

TitleVan Allen Probes observation and modeling of chorus excitation and propagation during weak geomagnetic activities
Publication TypeJournal Article
Year of Publication2015
AuthorsHe, Y, Xiao, F, Zhou, Q, Yang, C, Liu, S, Baker, DN, Kletzing, CA, Kurth, WS, Hospodarsky, GB, Spence, HE, Reeves, GD, Funsten, HO, Blake, JB
JournalJournal of Geophysical Research: Space Physics
Date Published07/2015
Keywordschorus wave excitation; energetic electrons; Geomagnetic storm; Van Allen Probes; Van Allen probes results; wave-particle interaction
AbstractWe report correlated data on nightside chorus waves and energetic electrons during two small storm periods: 1 November 2012 (Dst≈-45) and 14 January 2013 (Dst≈-18). The Van Allen Probes simultaneously observed strong chorus waves at locations L = 5.8 − 6.3, with a lower frequency band 0.1 − 0.5fce and a peak spectral density ∼[10−4 nT2/Hz. In the same period, the fluxes and anisotropy of energetic (∼ 10-300 keV) electrons were greatly enhanced in the interval of large negative interplanetary magnetic field Bz. Using a bi-Maxwellian distribution to model the observed electron distribution, we perform ray tracing simulations to show that nightside chorus waves are indeed produced by the observed electron distribution with a peak growth for a field-aligned propagation around between 0.3fce and 0.4fce, at latitude <7∘. Moreover, chorus waves launched with initial normal angles either θ < 90∘ or >90∘ propagate along the field either northward or southward, and then bounce back either away from Earth for a lower frequency or towards Earth for higher frequencies. The current results indicate that nightside chorus waves can be excited even during weak geomagnetic activities in cases of continuous injection associated with negative Bz. Moreover, we examine a dayside event during a small storm C on 8 May 2014 (Dst≈-45) and find that the observed anisotropic energetic electron distributions potentially contribute to the generation of dayside chorus waves, but this requires more thorough studies in the future.
URLhttp://doi.wiley.com/10.1002/2015JA021376
DOI10.1002/2015JA021376
Short TitleJ. Geophys. Res. Space Physics


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