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Discovery of proton hill in the phase space during interactions between ions and electromagnetic ion cyclotron waves
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...
Autores principales: | , , , , , , , , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
Nature Publishing Group UK
2021
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8241848/ https://www.ncbi.nlm.nih.gov/pubmed/34188084 http://dx.doi.org/10.1038/s41598-021-92541-0 |
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author | Shoji, Masafumi Miyoshi, Yoshizumi Kistler, Lynn M. Asamura, Kazushi Matsuoka, Ayako Kasaba, Yasumasa Matsuda, Shoya Kasahara, Yoshiya Shinohara, Iku |
author_facet | Shoji, Masafumi Miyoshi, Yoshizumi Kistler, Lynn M. Asamura, Kazushi Matsuoka, Ayako Kasaba, Yasumasa Matsuda, Shoya Kasahara, Yoshiya Shinohara, Iku |
author_sort | Shoji, Masafumi |
collection | PubMed |
description | 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. |
format | Online Article Text |
id | pubmed-8241848 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2021 |
publisher | Nature Publishing Group UK |
record_format | MEDLINE/PubMed |
spelling | pubmed-82418482021-07-06 Discovery of proton hill in the phase space during interactions between ions and electromagnetic ion cyclotron waves Shoji, Masafumi Miyoshi, Yoshizumi Kistler, Lynn M. Asamura, Kazushi Matsuoka, Ayako Kasaba, Yasumasa Matsuda, Shoya Kasahara, Yoshiya Shinohara, Iku Sci Rep Article 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. Nature Publishing Group UK 2021-06-29 /pmc/articles/PMC8241848/ /pubmed/34188084 http://dx.doi.org/10.1038/s41598-021-92541-0 Text en © The Author(s) 2021 https://creativecommons.org/licenses/by/4.0/Open Access 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. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/ (https://creativecommons.org/licenses/by/4.0/) . |
spellingShingle | Article Shoji, Masafumi Miyoshi, Yoshizumi Kistler, Lynn M. Asamura, Kazushi Matsuoka, Ayako Kasaba, Yasumasa Matsuda, Shoya Kasahara, Yoshiya Shinohara, Iku Discovery of proton hill in the phase space during interactions between ions and electromagnetic ion cyclotron waves |
title | Discovery of proton hill in the phase space during interactions between ions and electromagnetic ion cyclotron waves |
title_full | Discovery of proton hill in the phase space during interactions between ions and electromagnetic ion cyclotron waves |
title_fullStr | Discovery of proton hill in the phase space during interactions between ions and electromagnetic ion cyclotron waves |
title_full_unstemmed | Discovery of proton hill in the phase space during interactions between ions and electromagnetic ion cyclotron waves |
title_short | Discovery of proton hill in the phase space during interactions between ions and electromagnetic ion cyclotron waves |
title_sort | discovery of proton hill in the phase space during interactions between ions and electromagnetic ion cyclotron waves |
topic | Article |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8241848/ https://www.ncbi.nlm.nih.gov/pubmed/34188084 http://dx.doi.org/10.1038/s41598-021-92541-0 |
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