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

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

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997adspr..19..843e&link_type=abstract

Advances in Space Research, Volume 19, Issue 6, p. 843-846.

Physics

2

Scientific paper

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.

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