MHD turbulence in the solar wind‐comet interaction region

R. Z. Sagdeev, V. D. Shapiro, V. I. Shevchenko, K. Szego

Research output: Contribution to journalArticle

68 Citations (Scopus)

Abstract

One of the most striking features discovered during the encounter of space probe ICE and comet Giacobini‐Zinner was the presence of intensive MHD turbulence even at large distances from the comet. In this paper it is shown that the mass loading of the solar wind with cometary ions can cause such a phenomenon.

Original languageEnglish
Pages (from-to)85-88
Number of pages4
JournalGeophysical Research Letters
Volume13
Issue number2
DOIs
Publication statusPublished - Feb 1986

ASJC Scopus subject areas

  • Geophysics
  • Earth and Planetary Sciences(all)

Fingerprint Dive into the research topics of 'MHD turbulence in the solar wind‐comet interaction region'. Together they form a unique fingerprint.

  • Cite this