Japan Geoscience Union Meeting 2019

Presentation information

[E] Oral

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

[P-EM13] Inner magnetosphere: Recent understanding and new insights

Tue. May 28, 2019 3:30 PM - 5:00 PM A04 (TOKYO BAY MAKUHARI HALL)

convener:Yusuke Ebihara(Research Institute for Sustainable Humanosphere, Kyoto University), Danny Summers(Memorial University of Newfoundland), Yoshizumi Miyoshi(Institute for Space-Earth Environmental Research, Nagoya University), Shinji Saito(Graduate School of Science, Nagoya University), Chairperson:Yoshizumi Miyoshi(ISEE, Nagoya University), Danny Summers

3:30 PM - 3:50 PM

[PEM13-06] Deformation of electron pitch angle distributions caused by chorus waves observed by the Arase satellite

★Invited Papers

*Satoshi Kurita1, Yoshizumi Miyoshi1, Satoshi Kasahara2, Shoichiro Yokota3, Yoshiya Kasahara4, Shoya Matsuda5, Ayako Matsuoka5, Iku Shinohara5 (1.Institute for Space-Earth Environmental Research, Nagoya University, 2.The University of Tokyo, 3.Graduate School of Science, Osaka University, 4.Information Media Center, Kanazawa University, 5.ISAS/JAXA)

Keywords:ERG/Arase satellite, Chorus waves, Acceleration

We report on deformation of electron pitch angle distributions associated with chorus waves observed by the Arase satellite. The deformation is characterized by flux increase of 17-30 keV electrons in a narrow and oblique pitch angle range and by flux decrease in 7-17 keV electron flux in the smaller pitch angle range than the flux increase. Comparison of change in electron pitch angle distributions with resonant ellipses of the upper band chorus shows that the deformation appears where effective wave-particle interaction is expected in the velocity space, and the flux increase takes place along the resonant ellipse of the upper frequency of the wave. This strongly suggests that the deformation is a consequence of wave-particle interactions between electrons and upper band chorus. The Arase observation demonstrates that the deformation occurs within 30 s, which is faster than expected from the quasi-linear diffusion theory.