A self-similar solution of expanding cylindrical flux ropes for any polytropic index value

Details A self-similar solution of expanding cylindrical flux ropes for any polytropic index value A self-similar solution of expanding cylindrical flux ropes for any polytropic index value

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aipc..679..737s&link_type=abstract

SOLAR WIND TEN: Proceedings of the Tenth International Solar Wind Conference. AIP Conference Proceedings, Volume 679, pp. 737-7

Physics

Particle Emission, Solar Wind, Interplanetary Magnetic Fields

Scientific paper

We found a new class of solutions for MHD equations that satisfies the condition that cylindrical flux ropes can expand self-similarly even when the polytropic index γ is larger than 1. We achieved this by including the effects of elongation along the symmetry axis as well as radial expansion and assuming that the radial expansion rate is the same as the elongation rate.

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