Different types of whistler mode chorus in the equatorial source region

Ulrich Taubenschuss, Ondrej Santolík, Daniel B. Graham, Huishan Fu, Yuri V. Khotyaintsev, Olivier Le Contel

Research output: Contribution to journalArticlepeer-review

Abstract

The Time History of Events and Macroscale Interactions during Substorms-D spacecraft crossed an active equatorial source region of whistler mode chorus rising tones on 23 October 2008. Rising tones are analyzed in terms of spectral and polarization characteristics, with special emphasis on wave normal angles. The latter exhibit large variations from quasi-parallel to oblique, even within single bursts, but seem to follow a definite pattern, which enables an unambiguous classification into five different groups. Furthermore, we discuss the frequently observed splitting of chorus bursts into a lower and an upper band around one half of the local electron cyclotron frequency. At chorus frequencies close to the gap, we find significantly lowered wave planarities and a tendency of wave normal angles to approach the Gendrin angle.

Original languageEnglish
Pages (from-to)8271-8279
Number of pages9
JournalGeophysical Research Letters
Volume42
Issue number20
DOIs
Publication statusPublished - 28 Oct 2015

Keywords

  • Gendrin angle
  • chorus
  • equatorial source
  • spectral gap
  • wave normals
  • whistler mode

Fingerprint

Dive into the research topics of 'Different types of whistler mode chorus in the equatorial source region'. Together they form a unique fingerprint.

Cite this