Japan Geoscience Union Meeting 2024

Presentation information

[E] Poster

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

[P-EM13] Dynamics of the Inner Magnetospheric System

Sun. May 26, 2024 5:15 PM - 6:45 PM Poster Hall (Exhibition Hall 6, Makuhari Messe)

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), Theodore E Sarris(Democritus University of Thrace), Evan G Thomas(Dartmouth College)


5:15 PM - 6:45 PM

[PEM13-P08] Local time dependence of energetic electron precipitation induced by the VLF signal from the ground-based transmitter

*Satoshi Kurita1, Shuei Noda1, Yoshiya Kasahara2, Shoya Matsuda2, Fuminori Tsuchiya3, Atsushi Kumamoto3, Tomoaki Hori4, Atsuki Shinbori4, Yoshizumi Miyoshi4, Iku Shinohara5 (1.Research Institute for Sustainable Humanosphere, 2.Kanazawa University, 3.Tohoku University, 4.ISEE/Nagoya University, 5.ISAS/JAXA)

Keywords:VLF transmitter, wave-particle interaction, energetic electron precipitation, Arase satellite

Intense signal from ground-based VLF wave transmitters can go through the ionosphere and penetrate into the magnetosphere, where they propagate further as whistler mode waves. The waves can resonantly interact with energetic electrons in the inner magnetosphere, resulting in the precipitation loss of electrons in the radiation belts. Previous studies show that a day-night asymmetry in the signal intensity of the VLF transmitters in the magnetosphere. Such an asymmetry of the signal intensity is attributed to the day-night variation in the ionospheric density, which is caused by presence and absence of the enhanced ionization of high-altitude atmosphere controlled by the solar illumination. Since the ionospheric density strongly depends on the local time, it is expected that the intensity of the VLF transmitter signals observed in the magnetosphere also depends on the local time and hence the resultant energetic electron precipitation may also have similar dependence. In this study, we analyzed the data obtained by the Arase satellite and the POES satellites to investigate local time dependence of the VLF transmitter signals in the magnetosphere and energetic electron precipitation. We find that the electron precipitation shows expected dependence on local time, and discuss the cause of the dependence from the point of view of resonance energy. It is revealed that local time dependence of the resonance energy can be a candidate to cause the local time dependent precipitation of energetic electrons due to the VLF transmitter signals.