AbstractOur 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.
Field configuration around large flux ropes in the solar corona and inner heliosphere
Advances in Space Research ; 38 , 3 ; 447-450
2005-06-27
4 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
Field configuration around large flux ropes in the solar corona and inner heliosphere
Online Contents | 2006
|Field configuration around large flux ropes in the solar corona and inner heliosphere
British Library Conference Proceedings | 2006
|On the Motion of Toroidal Magnetic Clouds in the Solar Corona and Inner Heliosphere
British Library Conference Proceedings | 2006
|THE EMERGENCE AND EVOLUTION OF TWISTED MAGNETIC FLUX ROPES IN THE SOLAR CORONA
British Library Conference Proceedings | 2005
|Preface: Magnetic flux ropes in solar environments
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