Yingying Zhao, Hui Zhu, Huicong Chen, Zhijie Qin, Zhenghao She
{"title":"ULF Wave-Driven Energization of Plasmaspheric Plume Ions During Multi-Step Geomagnetic Storms","authors":"Yingying Zhao, Hui Zhu, Huicong Chen, Zhijie Qin, Zhenghao She","doi":"10.1029/2025JA034430","DOIUrl":null,"url":null,"abstract":"<p>We report direct observations of the energization of plasmaspheric plume ions by ultralow frequency (ULF) waves during a multi-step geomagnetic storm from 25–29 August 2015. Based on Van Allen Probes observations, we identify multiple plasmaspheric plume regions in the afternoon-dusk sector during the storm, characterized by highly irregular density structures. Concurrently, the cold (<span></span><math>\n <semantics>\n <mrow>\n <mo><</mo>\n <mn>100</mn>\n </mrow>\n <annotation> ${< } 100$</annotation>\n </semantics></math> V) ion fluxes exhibit intermittent enhancements within these regions. A detailed analysis reveals that the ion flux variations result from the modulation of the ULF wave-driven <span></span><math>\n <semantics>\n <mrow>\n <mi>E</mi>\n <mo>×</mo>\n <mi>B</mi>\n </mrow>\n <annotation> $E\\times B$</annotation>\n </semantics></math> drift. Interestingly, the modulated ion fluxes appear at near <span></span><math>\n <semantics>\n <mrow>\n <mn>90</mn>\n <mo>°</mo>\n </mrow>\n <annotation> $90{}^{\\circ}$</annotation>\n </semantics></math> pitch angles and occur only in high-density plumes; no modulation signatures appear in low-density plasma troughs. These observations strongly support that ULF waves can perpendicularly modulate plasmaspheric plume ions within high-density regions via <span></span><math>\n <semantics>\n <mrow>\n <mi>E</mi>\n <mo>×</mo>\n <mi>B</mi>\n </mrow>\n <annotation> $E\\times B$</annotation>\n </semantics></math> effects. The present results provide a deeper understanding of the interactions between ULF waves and plasmaspheric plume ions in the inner magnetosphere.</p>","PeriodicalId":15894,"journal":{"name":"Journal of Geophysical Research: Space Physics","volume":"130 9","pages":""},"PeriodicalIF":2.9000,"publicationDate":"2025-09-15","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Geophysical Research: Space Physics","FirstCategoryId":"89","ListUrlMain":"https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2025JA034430","RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
We report direct observations of the energization of plasmaspheric plume ions by ultralow frequency (ULF) waves during a multi-step geomagnetic storm from 25–29 August 2015. Based on Van Allen Probes observations, we identify multiple plasmaspheric plume regions in the afternoon-dusk sector during the storm, characterized by highly irregular density structures. Concurrently, the cold ( V) ion fluxes exhibit intermittent enhancements within these regions. A detailed analysis reveals that the ion flux variations result from the modulation of the ULF wave-driven drift. Interestingly, the modulated ion fluxes appear at near pitch angles and occur only in high-density plumes; no modulation signatures appear in low-density plasma troughs. These observations strongly support that ULF waves can perpendicularly modulate plasmaspheric plume ions within high-density regions via effects. The present results provide a deeper understanding of the interactions between ULF waves and plasmaspheric plume ions in the inner magnetosphere.