Separation rate of the magnetic field lines observed by ULYSSES at high latitude
DOI: 10.1016/S0273-1177(97)00289-5
Bibcode: 1997AdSpR..19..843E
Balogh, A.; Erdös, G.; Kóta, J.
Hungary, United Kingdom
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.
1997
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Advances in Space Research
Ulysses
4