Andrew Wright, Thomas Elsden, Alexander Degeling, Ian R. Mann, Louis Ozeke, Timothy Yeoman, Jasmine Sandhu, Kazue Takahashi
{"title":"由快速波驱动的极向场线共振","authors":"Andrew Wright, Thomas Elsden, Alexander Degeling, Ian R. Mann, Louis Ozeke, Timothy Yeoman, Jasmine Sandhu, Kazue Takahashi","doi":"10.1029/2024GL111670","DOIUrl":null,"url":null,"abstract":"<p>We present numerical simulations of the excitation of resonant poloidal Alfvén waves. The resulting Alfvén waves could be loosely described as “high-<span></span><math>\n <semantics>\n <mrow>\n <mi>m</mi>\n </mrow>\n <annotation> $m$</annotation>\n </semantics></math>” (<span></span><math>\n <semantics>\n <mrow>\n <mi>m</mi>\n </mrow>\n <annotation> $m$</annotation>\n </semantics></math> is the azimuthal wave number) in as much as the azimuthal scale of the wave is much less than the scale in the direction normal to <span></span><math>\n <semantics>\n <mrow>\n <mi>L</mi>\n </mrow>\n <annotation> $L$</annotation>\n </semantics></math>-shells. Such waves are generally excited by wave-particle interactions. In this article we show how resonant poloidal Alfvén waves can be excited by a fast mode (of large azimuthal scale) in a cold plasma. The key property that enables this is a three-dimensional equilibrium, which facilitates the process of phasemixing in the azimuthal direction. We show that the classification of resonant Alfvén waves as high-<span></span><math>\n <semantics>\n <mrow>\n <mi>m</mi>\n </mrow>\n <annotation> $m$</annotation>\n </semantics></math> and low-<span></span><math>\n <semantics>\n <mrow>\n <mi>m</mi>\n </mrow>\n <annotation> $m$</annotation>\n </semantics></math> has limited applicability in 3D inhomogeneous media and suggest an alternative classification be based on the excitation mechanism.</p>","PeriodicalId":12523,"journal":{"name":"Geophysical Research Letters","volume":"52 3","pages":""},"PeriodicalIF":4.6000,"publicationDate":"2025-02-10","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://onlinelibrary.wiley.com/doi/epdf/10.1029/2024GL111670","citationCount":"0","resultStr":"{\"title\":\"Poloidal Field Line Resonances Driven by a Fast Wave\",\"authors\":\"Andrew Wright, Thomas Elsden, Alexander Degeling, Ian R. Mann, Louis Ozeke, Timothy Yeoman, Jasmine Sandhu, Kazue Takahashi\",\"doi\":\"10.1029/2024GL111670\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p>We present numerical simulations of the excitation of resonant poloidal Alfvén waves. The resulting Alfvén waves could be loosely described as “high-<span></span><math>\\n <semantics>\\n <mrow>\\n <mi>m</mi>\\n </mrow>\\n <annotation> $m$</annotation>\\n </semantics></math>” (<span></span><math>\\n <semantics>\\n <mrow>\\n <mi>m</mi>\\n </mrow>\\n <annotation> $m$</annotation>\\n </semantics></math> is the azimuthal wave number) in as much as the azimuthal scale of the wave is much less than the scale in the direction normal to <span></span><math>\\n <semantics>\\n <mrow>\\n <mi>L</mi>\\n </mrow>\\n <annotation> $L$</annotation>\\n </semantics></math>-shells. Such waves are generally excited by wave-particle interactions. In this article we show how resonant poloidal Alfvén waves can be excited by a fast mode (of large azimuthal scale) in a cold plasma. The key property that enables this is a three-dimensional equilibrium, which facilitates the process of phasemixing in the azimuthal direction. We show that the classification of resonant Alfvén waves as high-<span></span><math>\\n <semantics>\\n <mrow>\\n <mi>m</mi>\\n </mrow>\\n <annotation> $m$</annotation>\\n </semantics></math> and low-<span></span><math>\\n <semantics>\\n <mrow>\\n <mi>m</mi>\\n </mrow>\\n <annotation> $m$</annotation>\\n </semantics></math> has limited applicability in 3D inhomogeneous media and suggest an alternative classification be based on the excitation mechanism.</p>\",\"PeriodicalId\":12523,\"journal\":{\"name\":\"Geophysical Research Letters\",\"volume\":\"52 3\",\"pages\":\"\"},\"PeriodicalIF\":4.6000,\"publicationDate\":\"2025-02-10\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"https://onlinelibrary.wiley.com/doi/epdf/10.1029/2024GL111670\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Geophysical Research Letters\",\"FirstCategoryId\":\"89\",\"ListUrlMain\":\"https://onlinelibrary.wiley.com/doi/10.1029/2024GL111670\",\"RegionNum\":1,\"RegionCategory\":\"地球科学\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q1\",\"JCRName\":\"GEOSCIENCES, MULTIDISCIPLINARY\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Geophysical Research Letters","FirstCategoryId":"89","ListUrlMain":"https://onlinelibrary.wiley.com/doi/10.1029/2024GL111670","RegionNum":1,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"GEOSCIENCES, MULTIDISCIPLINARY","Score":null,"Total":0}
Poloidal Field Line Resonances Driven by a Fast Wave
We present numerical simulations of the excitation of resonant poloidal Alfvén waves. The resulting Alfvén waves could be loosely described as “high-” ( is the azimuthal wave number) in as much as the azimuthal scale of the wave is much less than the scale in the direction normal to -shells. Such waves are generally excited by wave-particle interactions. In this article we show how resonant poloidal Alfvén waves can be excited by a fast mode (of large azimuthal scale) in a cold plasma. The key property that enables this is a three-dimensional equilibrium, which facilitates the process of phasemixing in the azimuthal direction. We show that the classification of resonant Alfvén waves as high- and low- has limited applicability in 3D inhomogeneous media and suggest an alternative classification be based on the excitation mechanism.
期刊介绍:
Geophysical Research Letters (GRL) publishes high-impact, innovative, and timely research on major scientific advances in all the major geoscience disciplines. Papers are communications-length articles and should have broad and immediate implications in their discipline or across the geosciences. GRLmaintains the fastest turn-around of all high-impact publications in the geosciences and works closely with authors to ensure broad visibility of top papers.