Comparison of Simulated and Observed Interplanetary Flux Ropes

Details Comparison of Simulated and Observed Interplanetary Flux Ropes Comparison of Simulated and Observed Interplanetary Flux Ropes

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aipc..679..691v&link_type=abstract

SOLAR WIND TEN: Proceedings of the Tenth International Solar Wind Conference. AIP Conference Proceedings, Volume 679, pp. 691-6

Computer Science

1

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

Scientific paper

Three dimensional magnetohydrodynamic numerical simulations of propagating interplanetary flux ropes are presented and compared with ``in-situ'' spacecraft measurements. Flux ropes are injected near the Sun with various inclinations. Specific features followed from simulations, as double-peak magnetic field profiles or a possibility to observe one flux rope two times by the same spacecraft, are searched in observational data.

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