W. Z. Zhang, H. S. Fu, J. B. Cao, W. D. Fu, Z. Z. Guo, Z. Wang, C. Q. Wang, C. X. Du
{"title":"反双极化前沿后的电子水龙波动","authors":"W. Z. Zhang, H. S. Fu, J. B. Cao, W. D. Fu, Z. Z. Guo, Z. Wang, C. Q. Wang, C. X. Du","doi":"10.1029/2024GL114386","DOIUrl":null,"url":null,"abstract":"<p>Magnetic reconnection hosts regions of enhanced temperature anisotropy that could excite various kinetic instabilities and waves. However, the relation between electron firehose instability and the leading edge of tailward reconnection jets, as referred to anti-dipolarization fronts (ADFs), is still unclear. Here, for the first time, we provide direct observations of electron firehose fluctuations behind ADF by the Magnetospheric Multiscale (MMS) mission. These compressible fluctuations converted by the bulk flow have zero frequency in the plasma frame and large wave normal angles with respect to the background magnetic fields, and appears simultaneously with parallel electron temperature anisotropy. Our results found that the wave properties of the observed fluctuations largely agree with kinetic theoretical predictions of the non-propagating electron firehose mode. Specifically, the threshold of electron oblique firehose instability is exceeded under local plasma parameters and such instability has a growth rate of <span></span><math>\n <semantics>\n <mrow>\n <mi>γ</mi>\n <mo>∼</mo>\n <mn>0.01</mn>\n <mspace></mspace>\n <msub>\n <mi>ω</mi>\n <mrow>\n <mi>c</mi>\n <mi>e</mi>\n </mrow>\n </msub>\n </mrow>\n <annotation> $\\gamma \\mathit{\\sim }0.01\\,{\\omega }_{ce}$</annotation>\n </semantics></math>. These findings improve our understanding of wave dynamics near the ADFs.</p>","PeriodicalId":12523,"journal":{"name":"Geophysical Research Letters","volume":"52 10","pages":""},"PeriodicalIF":4.6000,"publicationDate":"2025-05-16","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://onlinelibrary.wiley.com/doi/epdf/10.1029/2024GL114386","citationCount":"0","resultStr":"{\"title\":\"Electron Firehose Fluctuations Behind Anti-Dipolarization Front\",\"authors\":\"W. Z. Zhang, H. S. Fu, J. B. Cao, W. D. Fu, Z. Z. Guo, Z. Wang, C. Q. Wang, C. X. Du\",\"doi\":\"10.1029/2024GL114386\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p>Magnetic reconnection hosts regions of enhanced temperature anisotropy that could excite various kinetic instabilities and waves. However, the relation between electron firehose instability and the leading edge of tailward reconnection jets, as referred to anti-dipolarization fronts (ADFs), is still unclear. Here, for the first time, we provide direct observations of electron firehose fluctuations behind ADF by the Magnetospheric Multiscale (MMS) mission. These compressible fluctuations converted by the bulk flow have zero frequency in the plasma frame and large wave normal angles with respect to the background magnetic fields, and appears simultaneously with parallel electron temperature anisotropy. Our results found that the wave properties of the observed fluctuations largely agree with kinetic theoretical predictions of the non-propagating electron firehose mode. Specifically, the threshold of electron oblique firehose instability is exceeded under local plasma parameters and such instability has a growth rate of <span></span><math>\\n <semantics>\\n <mrow>\\n <mi>γ</mi>\\n <mo>∼</mo>\\n <mn>0.01</mn>\\n <mspace></mspace>\\n <msub>\\n <mi>ω</mi>\\n <mrow>\\n <mi>c</mi>\\n <mi>e</mi>\\n </mrow>\\n </msub>\\n </mrow>\\n <annotation> $\\\\gamma \\\\mathit{\\\\sim }0.01\\\\,{\\\\omega }_{ce}$</annotation>\\n </semantics></math>. These findings improve our understanding of wave dynamics near the ADFs.</p>\",\"PeriodicalId\":12523,\"journal\":{\"name\":\"Geophysical Research Letters\",\"volume\":\"52 10\",\"pages\":\"\"},\"PeriodicalIF\":4.6000,\"publicationDate\":\"2025-05-16\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"https://onlinelibrary.wiley.com/doi/epdf/10.1029/2024GL114386\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Geophysical Research Letters\",\"FirstCategoryId\":\"89\",\"ListUrlMain\":\"https://onlinelibrary.wiley.com/doi/10.1029/2024GL114386\",\"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/10.1029/2024GL114386","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}
Electron Firehose Fluctuations Behind Anti-Dipolarization Front
Magnetic reconnection hosts regions of enhanced temperature anisotropy that could excite various kinetic instabilities and waves. However, the relation between electron firehose instability and the leading edge of tailward reconnection jets, as referred to anti-dipolarization fronts (ADFs), is still unclear. Here, for the first time, we provide direct observations of electron firehose fluctuations behind ADF by the Magnetospheric Multiscale (MMS) mission. These compressible fluctuations converted by the bulk flow have zero frequency in the plasma frame and large wave normal angles with respect to the background magnetic fields, and appears simultaneously with parallel electron temperature anisotropy. Our results found that the wave properties of the observed fluctuations largely agree with kinetic theoretical predictions of the non-propagating electron firehose mode. Specifically, the threshold of electron oblique firehose instability is exceeded under local plasma parameters and such instability has a growth rate of . These findings improve our understanding of wave dynamics near the ADFs.
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.