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dc.contributor.authorShoji, Masafumien
dc.contributor.authorMiyoshi, Yoshizumien
dc.contributor.authorKistler, Lynn M.en
dc.contributor.authorAsamura, Kazushien
dc.contributor.authorMatsuoka, Ayakoen
dc.contributor.authorKasaba, Yasumasaen
dc.contributor.authorMatsuda, Shoyaen
dc.contributor.authorKasahara, Yoshiyaen
dc.contributor.authorShinohara, Ikuen
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.accessioned2021-07-14T00:35:32Z-
dc.date.available2021-07-14T00:35:32Z-
dc.date.issued2021-
dc.identifier.urihttp://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.abstractA 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.isoeng-
dc.publisherSpringer Natureen
dc.rights© The Author(s) 2021en
dc.rightsThis 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.urihttp://creativecommons.org/licenses/by/4.0/-
dc.subjectMagnetospheric physicsen
dc.titleDiscovery of proton hill in the phase space during interactions between ions and electromagnetic ion cyclotron wavesen
dc.typejournal article-
dc.type.niitypeJournal Article-
dc.identifier.jtitleScientific Reportsen
dc.identifier.volume11-
dc.relation.doi10.1038/s41598-021-92541-0-
dc.textversionpublisher-
dc.identifier.artnum13480-
dc.addressInstitute for Space Earth Environmental Research, Nagoya Universityen
dc.addressInstitute for Space Earth Environmental Research, Nagoya Universityen
dc.addressInstitute for Space Earth Environmental Research, Nagoya University; Space Science Center, University of New Hampshireen
dc.addressInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agencyen
dc.addressData Analysis Center for Geomagnetism and Space Magnetism, Graduate School of Science, Kyoto Universityen
dc.addressPlanetary Plasma and Atmospheric Research Center, Tohoku Universityen
dc.addressInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agencyen
dc.addressGraduate School of Natural Science and Technology, Kanazawa Universityen
dc.addressInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agencyen
dc.identifier.pmid34188084-
dc.relation.urlhttps://www.kyoto-u.ac.jp/ja/research-news/2021-07-12-
dcterms.accessRightsopen access-
datacite.awardNumber15H05747-
datacite.awardNumber15H05815-
datacite.awardNumber17H06140-
datacite.awardNumber17K14402-
datacite.awardNumber20H01959-
datacite.awardNumber20K14546-
datacite.awardNumber.urihttps://kaken.nii.ac.jp/ja/grant/KAKENHI-PROJECT-15H05747/-
datacite.awardNumber.urihttps://kaken.nii.ac.jp/ja/grant/KAKENHI-PLANNED-15H05815/-
datacite.awardNumber.urihttps://kaken.nii.ac.jp/ja/grant/KAKENHI-PROJECT-17H06140/-
datacite.awardNumber.urihttps://kaken.nii.ac.jp/ja/grant/KAKENHI-PROJECT-17K14402/-
datacite.awardNumber.urihttps://kaken.nii.ac.jp/ja/grant/KAKENHI-PROJECT-20H01959/-
datacite.awardNumber.urihttps://kaken.nii.ac.jp/ja/grant/KAKENHI-PROJECT-20K14546/-
dc.identifier.eissn2045-2322-
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.alternativeJapan Society for the Promotion of Science (JSPS)en
jpcoar.funderName.alternativeJapan Society for the Promotion of Science (JSPS)en
jpcoar.funderName.alternativeJapan Society for the Promotion of Science (JSPS)en
jpcoar.funderName.alternativeJapan Society for the Promotion of Science (JSPS)en
jpcoar.funderName.alternativeJapan Society for the Promotion of Science (JSPS)en
jpcoar.funderName.alternativeJapan Society for the Promotion of Science (JSPS)en
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