Modeling of IMF draping around a supersonic magnetic cloud

Details Modeling of IMF draping around a supersonic magnetic cloud Modeling of IMF draping around a supersonic magnetic cloud

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.477..297r&link_type=abstract

In: Proceedings of the Second Solar Cycle and Space Weather Euroconference, 24 - 29 September 2001, Vico Equense, Italy. Editor:

Computer Science

Magnetic Clouds

Scientific paper

We have found an approximate analytical solution of magnetic field distribution around a flux rope. The obtained solution shows a behavior of magnetic field lines around a cylindrical magnetically closed body with a bow shock ahead. The bow shock shape was assumed to be a parabolic cylinder. The resulting field is described by a sum of a few functions with coefficients, which are obtained from the following conditions: (i) no normal field component at the flux rope surface; (ii) normal components are continuous at the bow shock; and (iii) the field approaches undisturbed values at large distances from the center of the body.

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