Heliospheric langmuir wave observations from the ulysses spacecraft

R. J. MacDowall, Naiguo Lin, D. J. McComas

Research output: Contribution to journalArticle

5 Scopus citations

Abstract

Langmuir waves are electrostatic plasma oscillations produced by unstable electron beams in the solar wind and elsewhere. Typical electron sources are solar flares, shocks, and magnetic holes. In this paper, we present an overview of the Langmuir waves observed by Ulysses during both its solar minimum and solar maximum orbits. Langmuir waves in magnetic holes are a major component of the total Langmuir wave population; they occur preferentially in fast solar wind and are observed by Ulysses to be most intense within 2 AU of the Sun.

Original languageEnglish (US)
Pages (from-to)479-483
Number of pages5
JournalAdvances in Space Research
Volume32
Issue number4
DOIs
StatePublished - Jan 1 2003
Externally publishedYes

All Science Journal Classification (ASJC) codes

  • Aerospace Engineering
  • Astronomy and Astrophysics
  • Geophysics
  • Atmospheric Science
  • Space and Planetary Science
  • Earth and Planetary Sciences(all)

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