Xinlin Li, Zheng Xiang, Yang Mei, Declan O'Brien, David Brennan, Hong Zhao, Daniel N. Baker, Michael A. Temerin
{"title":"A New Electron and Proton Radiation Belt Identified by CIRBE/REPTile-2 Measurements After the Magnetic Super Storm of 10 May 2024","authors":"Xinlin Li, Zheng Xiang, Yang Mei, Declan O'Brien, David Brennan, Hong Zhao, Daniel N. Baker, Michael A. Temerin","doi":"10.1029/2024JA033504","DOIUrl":null,"url":null,"abstract":"<p>Following the largest magnetic storm in 20 years (10 May 2024), REPTile-2 on NASA's CIRBE satellite identified two new radiation belts containing 1.3–5 MeV electrons around <i>L</i> = 2.5–3.5 and 6.8–20 MeV protons around <i>L</i> = 2. The region around <i>L</i> = 2.5–3.5 is usually devoid of relativistic electrons due to wave-particle interactions that scatter them into the atmosphere. However, these 1.3–5 MeV electrons in this new belt seemed unaffected until a magnetic storm on 28 June 2024, perturbed the region. The long-lasting nature of this new electron belt has physical implications for the dependence of electron wave-particle interactions on energy, plasma density, and magnetic field strength. The enhancement of protons around <i>L</i> = 2 exceeded an order of magnitude between 6.8 and 15 MeV forming a distinct new proton belt that appears even more stable. CIRBE, after a year of successful operation, malfunctioned 25 days before the super storm but returned to functionality 1 month after the storm, enabling these discoveries.</p>","PeriodicalId":15894,"journal":{"name":"Journal of Geophysical Research: Space Physics","volume":"130 2","pages":""},"PeriodicalIF":2.6000,"publicationDate":"2025-02-06","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://onlinelibrary.wiley.com/doi/epdf/10.1029/2024JA033504","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Geophysical Research: Space Physics","FirstCategoryId":"89","ListUrlMain":"https://onlinelibrary.wiley.com/doi/10.1029/2024JA033504","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
Following the largest magnetic storm in 20 years (10 May 2024), REPTile-2 on NASA's CIRBE satellite identified two new radiation belts containing 1.3–5 MeV electrons around L = 2.5–3.5 and 6.8–20 MeV protons around L = 2. The region around L = 2.5–3.5 is usually devoid of relativistic electrons due to wave-particle interactions that scatter them into the atmosphere. However, these 1.3–5 MeV electrons in this new belt seemed unaffected until a magnetic storm on 28 June 2024, perturbed the region. The long-lasting nature of this new electron belt has physical implications for the dependence of electron wave-particle interactions on energy, plasma density, and magnetic field strength. The enhancement of protons around L = 2 exceeded an order of magnitude between 6.8 and 15 MeV forming a distinct new proton belt that appears even more stable. CIRBE, after a year of successful operation, malfunctioned 25 days before the super storm but returned to functionality 1 month after the storm, enabling these discoveries.