Quantifying the relative contributions of substorm injections and chorus waves to the rapid outward extension of electron radiation belt

TitleQuantifying the relative contributions of substorm injections and chorus waves to the rapid outward extension of electron radiation belt
Publication TypeJournal Article
Year of Publication2014
AuthorsSu, Z, Zhu, H, Xiao, F, Zheng, H, Wang, Y, Zong, Q-G, He, Z, Shen, C, Zhang, M, Wang, S, Kletzing, CA, Kurth, WS, Hospodarsky, GB, Spence, HE, Reeves, GD, Funsten, HO, Blake, JB, Baker, DN
JournalJournal of Geophysical Research: Space Physics
Date Published12/2014
KeywordsChorus wave; Electron acceleration; Radiation belt; substorm injection; Van Allen Probes; wave-particle interaction
AbstractWe study the rapid outward extension of the electron radiation belt on a timescale of several hours during three events observed by RBSP and THEMIS satellites, and particularly quantify the contributions of substorm injections and chorus waves to the electron flux enhancement near the outer boundary of radiation belt. A comprehensive analysis including both observations and simulations is performed for the first event on 26 May 2013. The outer boundary of electron radiation belt moved from L = 5.5 to L > 6.07 over about 6 hours, with up to four orders of magnitude enhancement in the 30 keV-5 MeV electron fluxes at L = 6. The observations show that the substorm injection can cause 100% and 20% of the total subrelativistic (~0.1 MeV) and relativistic (2-5 MeV) electron flux enhancements within a few minutes. The data-driven simulation supports that the strong chorus waves can yield 60%-80% of the total energetic (0.2-5.0 MeV) electron flux enhancement within about 6 hours. Some simple analyses are further given for the other two events on 2 and 29 June 2013, in which the contributions of substorm injections and chorus waves are shown to be qualitatively comparable to those for the first event. These results clearly illustrate the respective importance of substorm injections and chorus waves for the evolution of radiation belt electrons at different energies on a relatively short timescale.
URLhttp://doi.wiley.com/10.1002/2014JA020709
DOI10.1002/2014JA020709
Short TitleJ. Geophys. Res. Space Physics


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