Spatio‐Temporal Characteristics of IPDP‐Type EMIC Waves on April 19, 2017: Implications for Loss of Relativistic Electrons in the Outer Belt
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- Asuka Hirai
- Graduate School of Science Tohoku University Sendai Japan
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- Fuminori Tsuchiya
- Graduate School of Science Tohoku University Sendai Japan
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- Takahiro Obara
- Graduate School of Science Tohoku University Sendai Japan
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- Yuto Katoh
- Graduate School of Science Tohoku University Sendai Japan
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- Yoshizumi Miyoshi
- Institute for Space‐Earth Environmental Research Nagoya University Nagoya Japan
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- Kazuo Shiokawa
- Institute for Space‐Earth Environmental Research Nagoya University Nagoya Japan
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- Yasumasa Kasaba
- Graduate School of Science Tohoku University Sendai Japan
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- Hiroaki Misawa
- Graduate School of Science Tohoku University Sendai Japan
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- Chae‐Woo Jun
- Institute for Space‐Earth Environmental Research Nagoya University Nagoya Japan
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- Satoshi Kurita
- Research Institute for Sustainable Humanosphere Kyoto University Uji Japan
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- Martin G. Connors
- Athabasca University AB Athabasca Canada
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- Aaron T. Hendry
- University of Otago Dunedin New Zealand
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- Atsuki Shinbori
- Institute for Space‐Earth Environmental Research Nagoya University Nagoya Japan
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- Yuichi Otsuka
- Institute for Space‐Earth Environmental Research Nagoya University Nagoya Japan
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- Takuya Tsugawa
- National Institute of Information and Communications Technology Koganei Japan
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- Michi Nishioka
- National Institute of Information and Communications Technology Koganei Japan
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- Septi Perwitasari
- National Institute of Information and Communications Technology Koganei Japan
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- Jerry W. Manweiler
- Fundamental Technologies LLC KS Lawrence USA
書誌事項
- 公開日
- 2023-08
- 資源種別
- journal article
- 権利情報
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- http://creativecommons.org/licenses/by/4.0/
- DOI
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- 10.1029/2023ja031479
- 公開者
- American Geophysical Union (AGU)
この論文をさがす
説明
<jats:title>Abstract</jats:title><jats:p>To understand the mechanism of the increased frequency of intervals of pulsations of diminishing periods (IPDPs), we analyzed IPDP‐type electromagnetic ion cyclotron (EMIC) waves that occurred on 19 April 2017, using ground and satellite observations. Observations by low‐altitude satellites and ground‐based magnetometers indicate that the increased IPDP frequency is caused by an inward (i.e., Earthward) shift of the EMIC wave source region. The EMIC wave source region moves inward along the mid‐latitude trough, which we used as a proxy for the plasmapause location. A statistical analysis shows that increases in the IPDP frequency showed a positive correlation with polar cap potentials. These results suggest an enhanced convection electric field causes an inward shift of the source region. The inward shift of the source region allows EMIC waves to scatter relativistic electrons over a wide range of radial distances during the IPDP event. This mechanism suggests that IPDP‐type EMIC waves are more likely to scatter relativistic electrons than other EMIC waves. We also show that the decreased phase‐space density of relativistic electrons in the outer radiation belt is consistent with the extent of the source region and the resonant energy of EMIC waves, implying a possible contribution of EMIC waves to outer radiation belt loss during the main phase of geomagnetic storms.</jats:p>
収録刊行物
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- Journal of Geophysical Research: Space Physics
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Journal of Geophysical Research: Space Physics 128 (8), 2023-08
American Geophysical Union (AGU)
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詳細情報 詳細情報について
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- CRID
- 1360021390558279808
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- ISSN
- 21699402
- 21699380
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- 資料種別
- journal article
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- データソース種別
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- Crossref
- KAKEN
- OpenAIRE
