Japan Geoscience Union Meeting 2021

Presentation information

[E] Poster

P (Space and Planetary Sciences ) » P-EM Solar-Terrestrial Sciences, Space Electromagnetism & Space Environment

[P-EM12] Dynamics of the Inner Magnetospheric System

Sat. Jun 5, 2021 5:15 PM - 6:30 PM Ch.04

convener:Kunihiro Keika(Department of Earth and Planetary Science, Graduate School of Science, The University of Tokyo), Yoshizumi Miyoshi(Institute for Space-Earth Environmental Research, Nagoya University), W Lauren Blum(University of Colorado Boulder), Yuri Shprits(Helmholtz Centre Potsdam GFZ German Research Centre for Geosciences)

5:15 PM - 6:30 PM

[PEM12-P26] An observational study on possible excitation of storm-time Pc5 waves

*Kento Otani1, Iku Shinohara2, Mariko Teramoto3, Tomotsugu Yamakawa1, Kanako Seki4, Satoshi Kasahara4, Shoichiro Yokota5, Kunihiro Keika1, Naoko Takahashi4, Takefumi Mitani2, Nana Higashio2, Ayako Matsuoka6, Kazuhiro Yamamoto4 (1.Tokyo University/Graduate School of Science, 2.JAXA, 3.Kyushu Institute of Technology, 4.Tokyo University, 5.Graduate school of Science, Osaka University, 6.Graduate school of Science, Kyoto University)

The adiabatic acceleration associated with the radial diffusion by the ULF wave is an important mechanism that generates relativistic electrons in the radiation belts. Among various ULF waves observed in the geospace, the storm-time Pc5 wave is a possible candidate to drive the radial diffusion during magnetic storms, although its excitation process and the relation between the observed waves and the radial diffusion have not been confirmed. Storm-time Pc5 wave is thought to be excited by injected ions from magnetotail to the ring current. Recently, Yamakawa et al. (2019) demonstrate that Pc5 waves can be excited by the injected ions via the drift resonance by a numerical simulation study.

This paper would like to address the Pc5 excitation process based on recent multi-satellite observation datasets obtained in the inner magnetosphere. According to the results of Yamakawa et al. (2019), Pc5 waves excited by the drift resonance have a characteristic of the frequency evolution. Using the magnetic field observation of Arase (ERG), we have collected Pc5 wave events that show the same frequency evolution as that observed in the numerical simulation. As a result, the occurrence probability of the Pc5 wave events depends on the geomagnetic activity, and the spatial distribution of the selected events is consistent with the simulation results.

Further, we pick up the examples of Pc5 events where the ion injections are observed just before and investigate if the observed injected ions can excite Pc5 waves through drift resonance. This presentation will discuss the relationship between ion injection events and Pc5 observations in the drift resonance context.