Separation rate of the magnetic field lines observed by ulysses at high latitude

G. Erdős, A. Balogh, J. Kóta

Research output: Contribution to journalArticle

4 Citations (Scopus)

Abstract

Ulysses has observed enhanced magnetic field fluctuations embedded in the fast solar wind originating from the high latitude coronal hole. These fluctuations proved to affect charged particle transport significantly. In this paper we apply a new method to determine the magnetic field line mixing from the actually measured magnetic field.

Original languageEnglish
Pages (from-to)843-846
Number of pages4
JournalAdvances in Space Research
Volume19
Issue number6
Publication statusPublished - 1997

Fingerprint

polar regions
Magnetic fields
magnetic field
magnetic fields
Solar wind
coronal holes
Charged particles
solar wind
charged particles
rate
particle
method

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Separation rate of the magnetic field lines observed by ulysses at high latitude. / Erdős, G.; Balogh, A.; Kóta, J.

In: Advances in Space Research, Vol. 19, No. 6, 1997, p. 843-846.

Research output: Contribution to journalArticle

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