Japan Geoscience Union Meeting 2025

Presentation information

[J] Oral

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

[P-EM17] Space Plasma Science

Tue. May 27, 2025 10:45 AM - 12:15 PM 303 (International Conference Hall, Makuhari Messe)

convener:Takanobu Amano(Department of Earth and Planetary Science, University of Tokyo), Yohei Miyake(Graduate School of System Informatics, Kobe University), Shogo Isayama(Interdisciplinary Graduate School of Engineering Sciences, Kyushu University), Takayuki Umeda(Information Initiative Center, Hokkaido University), Chairperson:Shogo Isayama(Interdisciplinary Graduate School of Engineering Sciences, Kyushu University), Yohei Miyake(Graduate School of System Informatics, Kobe University)

12:00 PM - 12:15 PM

[PEM17-12] Threshold analysis of lower hybrid and ion Bernstein wave instability driven by energetic ions

*Tsubasa Kotani1, Mieko Toida2, Toseo Moritaka2, Satoshi Taguchi1 (1.Graduate School of Science, Kyoto University, 2.National Institute for Fusion Science)

Keywords:lower hybrid wave, ion Bernstein wave, energetic ions, instability analysis

Taking into account the thermal effects, the lower hybrid wave can be considered as a type of ion Bernstein wave. Assuming that energetic ions, as the driving source of these waves, have a ring-like velocity distribution characterized by the delta function, the instability can be determined by the only four parameters: the ion-to-electron mass mi/me, the ratio of the electron plasma frequency to the electron gyro frequency ωpee, the ratio of the energetic ion velocity to the bulk ion thermal velocity u/vti, and the density ratio of energetic ions to electrons nh/ne. There are many previous studies to investigate a lower hybrid and ion Bernstein wave instability, but most of them used limited parameters to analyze the instability.

In this study, we perform parametric instability analyses for lower hybrid and ion Bernstein waves driven by energetic ions. We consider these waves propagating exactly perpendicular to the magnetic field. We analyze the instability threshold (nh/ne) for the two parameters (ωpee and u/vti ) in a hydrogen-electron (mi/me=1836) plasma.