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

Wed. May 29, 2019 9:00 AM - 10:30 AM 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:Shinji Saito(ISEE, Nagoya University), Yusuke Ebihara(RISH, Kyoto University)

9:45 AM - 10:00 AM

[PEM13-14] Plasmaspheric EMIC waves excited through mode conversion from equatorial noise under existence of M/Q=2 ions

*Yoshizumi Miyoshi1, Shoya Matsuda2, Satoshi Kurita1, koji nomura1, Kunihiro Keika3, Masafumi Shoji1, Naritoshi Kitamura3, Yoshiya Kasahara4, Ayako Matsuoka2, Iku Shinohara2, Kazuo Shiokawa1, Shinobu Machida1, Ondrej Santolik5, Scott Boardsen6, Richard Horne7, Wygant John8 (1.Institute for Space-Earth Environmental Research, Nagoya University, 2.JAXA, 3.University of Tokyo, 4.Kanazawa University, 5.CAS, 6.NASA, 7.British Antarctic Survey, 8.University of Minnesota)

Keywords:Arase, Plasmaspheric EMIC waves, M/Q=2 ions

Equatorial noise (EN, and referred to as magnetosonic mode waves) emissions are observed inside and outside the plasmapause and propagate across the magnetic field. In this study, we found the mode conversion from EN to EMIC waves in the plasmasphere using the plasma wave data from Van Allen Probes and Arase. When EN propagates into the earthward across the field line toward the Earth, EN splits into different waves modes; EN, and EMIC waves with the existence of M/Q=2 ions (deuteron or alpha particles) in the deep plasmasphere and the topside ionosphere. The oblique EMIC waves are excited through this mode conversion process, which are different characteristics of the propagation directions from EMIC waves generated from other processes. This mode conversion contributes to an origin of the plasmaspheric EMIC waves, especially at L<2.