Propagation of a Toroidal Magnetic Cloud through the Inner Heliosphere

Details Propagation of a Toroidal Magnetic Cloud through the Inner Heliosphere Propagation of a Toroidal Magnetic Cloud through the Inner Heliosphere

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aipc..679..180r&link_type=abstract

SOLAR WIND TEN: Proceedings of the Tenth International Solar Wind Conference. AIP Conference Proceedings, Volume 679, pp. 180-1

Physics

1

Particle Emission, Solar Wind, Interplanetary Magnetic Fields, Solar Wind Plasma, Sources Of Solar Wind

Scientific paper

An analytical solution for a potential magnetic field with arbitrary
intensity around a toroidal magnetic cloud has been found. The
background external field may have a gradient. The solution is used for
calculation of magnetic cloud propagation. Obtained velocity profiles
show a good agreement with in situ observations near the Earth's orbit.

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