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Comparison of Simulated and Observed Interplanetary Flux Ropes
2003
AIP Conference Proceedings
Preserved Fulltext
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.
doi:10.1063/1.1618688
fatcat:bkcxk7y77nfetnqfurd4ev3n4a