Simulation of magnetic cloud propagation in three dimensions

Details Simulation of magnetic cloud propagation in three dimensions Simulation of magnetic cloud propagation in three dimensions

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.477..293v&link_type=abstract

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

Physics

3

Magnetic Clouds, Numerical Simulations, Space Weather

Scientific paper

Magnetohydrodynamic simulation is used to study evolution and propagation of loop-like magnetic clouds through interplanetary space in three dimensions. Results show that a flux rope becomes highly deformed; for instance, a spacecraft located at 1 AU would cross two times the same flux rope when the flux rope has a low inclination to the ecliptic plane. Initially circular cross section of the flux rope becomes very prolate at 1 AU.

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