Statistical Study of Selective Oxygen Increase in High‐Energy Ring Current Ions During Magnetic Storms

TitleStatistical Study of Selective Oxygen Increase in High‐Energy Ring Current Ions During Magnetic Storms
Publication TypeJournal Article
Year of Publication2019
AuthorsMitani, K, Seki, K, Keika, K, Gkioulidou, M, Lanzerotti, LJ, Mitchell, DG, Kletzing, CA, Yoshikawa, A, Obana, Y
JournalJournal of Geophysical Research: Space Physics
Date Published04/2019
ISSN2169-9380
KeywordsMagnetic Storms; Oxygen ions; ring current; Van Allen Probes
AbstractIon transport from the plasma sheet to the ring current is the main cause of the development of the ring current. Energetic (>150 keV) ring current ions are known to be transported diffusively in several days. A recent study suggested that energetic oxygen ions are transported closer to the Earth than protons due to the diffusive transport caused by a combination of the drift and drift‐bounce resonances with Pc 3–5 ultralow frequency waves during the 24 April 2013 magnetic storm. To understand the occurrence conditions of such selective oxygen increase (SOI), we investigate the phase space densities (PSDs) between protons and oxygen ions with the first adiabatic invariants (μ) of 0.1–2.0 keV/nT measured by the Radiation Belt Storm Probes Ion Composition Experiment instrument on the Van Allen Probes at L ~ 3–6 during 90 magnetic storms in 2013–2017. We identified the SOI events in which oxygen PSDs increase while proton PSDs do not increase during a period of ~9 hr (one orbital period). Among the 90 magnetic storms, 33% were accompanied by the SOI events. Global enhancements of Pc 4 and Pc 5 waves observed by ground magnetometers during the SOI events suggest that radial transport due to combination of the drift‐bounce resonance with Pc 4 oscillations and the drift resonance with Pc 5 oscillations can be the cause of SOIs. The contribution of the SOI events to the magnetic storm intensity is roughly estimated to be ~9% on average.
URLhttps://agupubs.onlinelibrary.wiley.com/doi/10.1029/2018JA026168
DOI10.1029/2018JA026168
Short TitleJ. Geophys. Res. Space Physics


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