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Observational features of charge distribution in Earth’s inner magnetosphere

  • Lai Gao
  • , Chao Shen*
  • , Yufei Zhou
  • , Yong Ji
  • , Zuyin Pu
  • , George Parks
  • , Christopher T. Russell
  • , Gang Zeng
  • , Lan Ma
  • , Roy B. Torbert
  • , Yanyan Yang
  • , James L. Burch
  • *Corresponding author for this work
  • Harbin Institute of Technology
  • Ningxia University
  • Peking University
  • University of California at Berkeley
  • University of California at Los Angeles
  • Jingchu University of Technology
  • University of New Hampshire
  • China Earthquake Administration
  • Southwest Research Institute

Research output: Contribution to journalArticlepeer-review

Abstract

Understanding the motion of charged particles in the electromagnetic field in the inner magnetosphere is essential for space science and space weather. Charge accumulation can occur due to the dipole magnetic and convective electric fields in this region. However, until the recent Magnetospheric Multiscale (MMS) mission, there were few means to detect charge distribution in situ. We report unambiguous in situ observation of the spatial distribution of the excess charge density in the inner magnetosphere by the MMS mission. We find that a positive (negative) charge accumulates in the dusk (dawn) side inner magnetospheres, which is contrary to the long assumed overall quasi-neutrality of space plasma. These observations and results offer insight into magnetosphere–ionosphere coupling.

Original languageEnglish
Article number63
JournalCommunications Physics
Volume7
Issue number1
DOIs
StatePublished - Dec 2024
Externally publishedYes

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