Correlated ULF Waves, Whistler-mode Chorus and Pulsating Aurora Observed by the Van Allen Probes and Ground-based Systems
Correlated ULF Waves, Whistler-mode Chorus and Pulsating Aurora Observed by the Van Allen Probes and Ground-based Systems
Previously Published Material: Preliminary findings reported at LWS meeting (Oct 2014) and more analysis reported at AGU (Dec 2014). Final work is expected to be published before Joint Assembly in the Pulsating Aurora special issue of JGR.
Abstract ID#: 35354
English Abstract:
Theory and observations have linked equatorial VLF waves with pulsating aurora for decades, invoking the process of pitch-angle scattering of 10's keV electrons in the equatorial magnetosphere. Recent satellite studies have strengthened this argument, by showing strong correlation between pulsating auroral patches and (1) lower-band chorus observed by THEMIS and (2) 30-100 keV electron modulation in the vicinity of geosynchronous orbit observed by GOES. Additionally, a link has been made between Pc4-5 compressional pulsations and modulation of whistler-mode chorus using THEMIS. Here we present simultaneous in-situ observations of structured chorus waves and an apparent field line resonance as a result of a substorm injection, observed by Van Allen Probes, along with ground-based observations of pulsating aurora. We demonstrate the possible scenario being one of substorm-driven ULF pulsations modulating chorus waves, and thus providing the driver for pulsating particle precipitation into the Earth's atmosphere. We also show, for the first time, a particular 3-Hz modulation of individual chorus elements. Such modulation has been noticed as a high-frequency component in camera data of pulsating aurora for decades, and is possibly a result of nonlinear chorus wave interactions.
Back to: The Physics of the Aurora I
