研究者業績

大矢 浩代

オオヤ ヒロヨ  (Hiroyo Ohya)

基本情報

所属
千葉大学 大学院工学研究院基幹工学専攻電気電子工学コース 助教
学位
博士(理学)(名古屋大学)

研究者番号
00241943
ORCID ID
 https://orcid.org/0000-0001-7637-8008
J-GLOBAL ID
200901034091674769
researchmap会員ID
1000249464

論文

 25
  • Asuka Hirai, Fuminori Tsuchiya, Takahiro Obara, Yoshizumi Miyoshi, Yuto Katoh, Yasumasa Kasaba, Kazuo Shiokawa, Atsushi Kumamoto, Yoshiya Kasahara, Shoya Matsuda, Hiroaki Misawa, Satoshi Kurita, Chae-Woo Jun, Hiroyo Ohya, Martin G. Connors
    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS 130(3) 2025年3月  
    Electromagnetic ion cyclotron (EMIC) waves are believed to cause the loss of relativistic electrons from the outer radiation belt into the atmosphere due to pitch angle scattering. However, it is still unclear whether all EMIC waves can scatter relativistic electrons or which conditions are favorable for pitch angle scattering by EMIC waves. In this study, we performed a 2-year data analysis of EMIC waves and EMIC wave-driven electron precipitation (EP), from 1 November 2016-31 October 2018. Electromagnetic ion cyclotron waves were observed using a ground-based magnetometer installed at Athabasca (ATH, L= $L=$4.3), Canada. Electron precipitation events were identified from very low-frequency radio waves propagated from the transmitters at North Dakota (NDK, L= $L=$3.0) and Seattle (NLK, L= $L=$2.9) stations in USA to the receiver installed at ATH. The magnetic local time dependence of EMIC waves showed higher occurrence rates in the dawn sector. In contrast, EMIC waves accompanied by EP were localized in the dusk sector and were likely to occur during geomagnetic substorms. We found that EMIC waves accompanied by EP were associated with the main phase of geomagnetic storms and occurred inside the plasmapause. These results suggest that the EMIC waves that cause EP occur in the overlap region between the ring current and dense cold plasma during the main phase of geomagnetic storms. This is consistent with previous studies describing that the electron resonant energy with EMIC waves is lower in regions with high plasma density.
  • Hiroyo Ohya, Fuminori Tsuchiya, Masaharu Nakayama, Sora Maruyama, Akane Kubota, Yukihiro Takahashi, Emanuel Sungging Mumpuni, La Ode Muhammad Musafar Kilowasid, Timbul Manik
    Springer Proceedings in Physics 153-160 2025年2月15日  
  • Ryota Furuya, Hiroyo Ohya, Fuminori Tsuchiya, Masa-yuki Yamamoto, Hiroyuki Nakata
    Springer Proceedings in Physics 205-212 2025年2月15日  
  • Asuka Hirai, Fuminori Tsuchiya, Takahiro Obara, Yoshizumi Miyoshi, Yuto Katoh, Yasumasa Kasaba, Kazuo Shiokawa, Atsushi Kumamoto, Yoshiya Kasahara, Shoya Matsuda, Hiroaki Misawa, Satoshi Kurita, Chae-Woo Jun, Hiroyo Ohya, Martin Connors
    2024年9月30日  
  • Hiroyo Ohya, Fuminori Tsuchiya, Tamio Takamura, Hiroyuki Shinagawa, Yukihiro Takahashi, Alfred B. Chen
    Scientific Reports 14(1) 2024年7月16日  査読有り筆頭著者責任著者
    Abstract The submarine volcano Hunga Tonga–Hunga Ha’apai erupted explosively on January 15, 2022, offering a unique opportunity to investigate interactions between the atmosphere and ionosphere caused by Lamb and Pekeris waves. However, the resonance of Pekeris waves has not been previously detected. In this study, we applied a multi-point monitoring approach focusing on the lower ionosphere and atmospheric electric field. Here we show observed oscillations of 100–200 s in manmade transmitter signals and the magnetic and atmospheric electric fields, which were caused by Pekeris waves. However, no corresponding changes with the period of 100–200 s in atmospheric pressure due to Pekeris waves were observed on the ground. A simulation of neutral wind revealed Pekeris waves oscillating near the mesopause, suggesting resonance. Therefore, the oscillation in atmospheric electric field is interpreted that the resonance in the lower ionosphere was projected onto the Earth's surface via a global electric circuit.

MISC

 122

講演・口頭発表等

 20

担当経験のある科目(授業)

 6

共同研究・競争的資金等の研究課題

 7

社会貢献活動

 7