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このアイテムのファイル:
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s41598-021-92541-0.pdf | 2.64 MB | Adobe PDF | 見る/開く |
完全メタデータレコード
DCフィールド | 値 | 言語 |
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dc.contributor.author | Shoji, Masafumi | en |
dc.contributor.author | Miyoshi, Yoshizumi | en |
dc.contributor.author | Kistler, Lynn M. | en |
dc.contributor.author | Asamura, Kazushi | en |
dc.contributor.author | Matsuoka, Ayako | en |
dc.contributor.author | Kasaba, Yasumasa | en |
dc.contributor.author | Matsuda, Shoya | en |
dc.contributor.author | Kasahara, Yoshiya | en |
dc.contributor.author | Shinohara, Iku | en |
dc.contributor.alternative | 小路, 真史 | ja |
dc.contributor.alternative | 三好, 由純 | ja |
dc.contributor.alternative | キスラー, リーン | ja |
dc.contributor.alternative | 浅村, 和史 | ja |
dc.contributor.alternative | 松岡, 彩子 | ja |
dc.contributor.alternative | 笠羽, 康正 | ja |
dc.contributor.alternative | 松田, 昇也 | ja |
dc.contributor.alternative | 笠原, 禎也 | ja |
dc.contributor.alternative | 篠原, 育 | ja |
dc.date.accessioned | 2021-07-14T00:35:32Z | - |
dc.date.available | 2021-07-14T00:35:32Z | - |
dc.date.issued | 2021 | - |
dc.identifier.uri | http://hdl.handle.net/2433/264433 | - |
dc.description | 宇宙空間で電波を生み出す陽子の集団を発見 --JAXAの人工衛星「あらせ」の観測と解析から--. 京都大学プレスリリース. 2021-07-12. | ja |
dc.description.abstract | A study using Arase data gives the first observational evidence that the frequency drift of electromagnetic ion cyclotron (EMIC) waves is caused by cyclotron trapping. EMIC emissions play an important role in planetary magnetospheres, causing scattering loss of radiation belt relativistic electrons and energetic protons. EMIC waves frequently show nonlinear signatures that include frequency drift and amplitude enhancements. While nonlinear growth theory has suggested that the frequency change is caused by nonlinear resonant currents owing to cyclotron trapping of the particles, observational evidence for this has been elusive. We survey the wave data observed by Arase from March, 2017 to September 2019, and find the best falling tone emission event, one detected on 11th November, 2017, for the wave particle interaction analysis. Here, we show for the first time direct evidence of the formation of a proton hill in phase space indicating cyclotron trapping. The associated resonance currents and the wave growth of a falling tone EMIC wave are observed coincident with the hill, as theoretically predicted. | en |
dc.language.iso | eng | - |
dc.publisher | Springer Nature | en |
dc.rights | © The Author(s) 2021 | en |
dc.rights | This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article's Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article's Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. | en |
dc.rights.uri | http://creativecommons.org/licenses/by/4.0/ | - |
dc.subject | Magnetospheric physics | en |
dc.title | Discovery of proton hill in the phase space during interactions between ions and electromagnetic ion cyclotron waves | en |
dc.type | journal article | - |
dc.type.niitype | Journal Article | - |
dc.identifier.jtitle | Scientific Reports | en |
dc.identifier.volume | 11 | - |
dc.relation.doi | 10.1038/s41598-021-92541-0 | - |
dc.textversion | publisher | - |
dc.identifier.artnum | 13480 | - |
dc.address | Institute for Space Earth Environmental Research, Nagoya University | en |
dc.address | Institute for Space Earth Environmental Research, Nagoya University | en |
dc.address | Institute for Space Earth Environmental Research, Nagoya University; Space Science Center, University of New Hampshire | en |
dc.address | Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency | en |
dc.address | Data Analysis Center for Geomagnetism and Space Magnetism, Graduate School of Science, Kyoto University | en |
dc.address | Planetary Plasma and Atmospheric Research Center, Tohoku University | en |
dc.address | Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency | en |
dc.address | Graduate School of Natural Science and Technology, Kanazawa University | en |
dc.address | Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency | en |
dc.identifier.pmid | 34188084 | - |
dc.relation.url | https://www.kyoto-u.ac.jp/ja/research-news/2021-07-12 | - |
dcterms.accessRights | open access | - |
datacite.awardNumber | 15H05747 | - |
datacite.awardNumber | 15H05815 | - |
datacite.awardNumber | 17H06140 | - |
datacite.awardNumber | 17K14402 | - |
datacite.awardNumber | 20H01959 | - |
datacite.awardNumber | 20K14546 | - |
datacite.awardNumber.uri | https://kaken.nii.ac.jp/ja/grant/KAKENHI-PROJECT-15H05747/ | - |
datacite.awardNumber.uri | https://kaken.nii.ac.jp/ja/grant/KAKENHI-PLANNED-15H05815/ | - |
datacite.awardNumber.uri | https://kaken.nii.ac.jp/ja/grant/KAKENHI-PROJECT-17H06140/ | - |
datacite.awardNumber.uri | https://kaken.nii.ac.jp/ja/grant/KAKENHI-PROJECT-17K14402/ | - |
datacite.awardNumber.uri | https://kaken.nii.ac.jp/ja/grant/KAKENHI-PROJECT-20H01959/ | - |
datacite.awardNumber.uri | https://kaken.nii.ac.jp/ja/grant/KAKENHI-PROJECT-20K14546/ | - |
dc.identifier.eissn | 2045-2322 | - |
jpcoar.funderName | 日本学術振興会 | ja |
jpcoar.funderName | 日本学術振興会 | ja |
jpcoar.funderName | 日本学術振興会 | ja |
jpcoar.funderName | 日本学術振興会 | ja |
jpcoar.funderName | 日本学術振興会 | ja |
jpcoar.funderName | 日本学術振興会 | ja |
jpcoar.awardTitle | 極限時間分解能観測によるオーロラ最高速変動現象の解明 | ja |
jpcoar.awardTitle | 地球電磁気圏擾乱現象の発生機構の解明と予測 | ja |
jpcoar.awardTitle | 宇宙プラズマ中の電磁サイクロトロン波による電子加速散乱機構の実証的研究 | ja |
jpcoar.awardTitle | 多次元空間におけるイオンサイクロトロン波動粒子相互作用の解明 | ja |
jpcoar.awardTitle | あらせ衛星観測とシミュレーションによる放射線帯電子の非線形加速・散乱過程の理解 | ja |
jpcoar.awardTitle | 宇宙自然プラズマ波動の同時多点観測による励起・伝搬特性の三次元的理解と利活用 | ja |
jpcoar.funderName.alternative | Japan Society for the Promotion of Science (JSPS) | en |
jpcoar.funderName.alternative | Japan Society for the Promotion of Science (JSPS) | en |
jpcoar.funderName.alternative | Japan Society for the Promotion of Science (JSPS) | en |
jpcoar.funderName.alternative | Japan Society for the Promotion of Science (JSPS) | en |
jpcoar.funderName.alternative | Japan Society for the Promotion of Science (JSPS) | en |
jpcoar.funderName.alternative | Japan Society for the Promotion of Science (JSPS) | en |
出現コレクション: | 学術雑誌掲載論文等 |

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