Skip to main navigation Skip to search Skip to main content

Electron Scattering by Highly Oblique Quasi-Electrostatic Chorus Waves Under Realistic Magnetospheric Conditions

  • Lixian Yang
  • , Si Liu
  • , Zhonglei Gao
  • , Wenya Li
  • , Fuliang Xiao
  • , Zhaoguo He
  • , Xingran Chen
  • , Yuyue Jin
  • , Qian He
  • , Zhoukun Deng
  • , Jiawen Tang
  • Changsha University of Science and Technology
  • CAS - National Space Science Center
  • Macau University of Science and Technology

Research output: Contribution to journalArticlepeer-review

Abstract

Using Van Allen Probes data (2013–2015), we report that highly oblique chorus waves frequently occur in low-density regions where (Formula presented.). These waves exhibit an electric-to-magnetic energy ratio (Formula presented.), much higher than the typical (Formula presented.) for quasi-parallel chorus, indicating a quasi-electrostatic nature, termed highly oblique quasi-electrostatic (HOQE) chorus. Incorporating realistic wave properties and plasma environments, numerical modeling shows that HOQE lower-band chorus with the central wave normal angle (Formula presented.) can efficiently scatter relativistic electrons up to 2 MeV near (Formula presented.) equatorial pitch angles primarily via higher-order resonance. Additionally, HOQE upper-band chorus (Formula presented.) drives strong diffusion of tens of keV electrons at moderate pitch angles. These findings reveal a previously overlooked pathway for MeV electron loss, advancing our understanding of chorus wave-particle interactions.

Original languageEnglish
Article numbere2026GL122429
JournalGeophysical Research Letters
Volume53
Issue number12
DOIs
StatePublished - 28 Jun 2026
Externally publishedYes

Fingerprint

Dive into the research topics of 'Electron Scattering by Highly Oblique Quasi-Electrostatic Chorus Waves Under Realistic Magnetospheric Conditions'. Together they form a unique fingerprint.

Cite this