Field configuration around large flux ropes in the solar corona and inner heliosphere

Details Field configuration around large flux ropes in the solar corona and inner heliosphere Field configuration around large flux ropes in the solar corona and inner heliosphere

Jan 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006adspr..38..447r&link_type=abstract

Advances in Space Research, Volume 38, Issue 3, p. 447-450.

Physics

Scientific paper

Our recently developed method, how to determine analytically a magnetic
field distribution in the vicinity of a large flux rope, is used to
describe field disturbances for few typical examples. The disturbed
field is treated as a combination of a pre-existing one and an
additional current-free part.

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