Numerical MHD Simulation of Flux-Rope Formed Ejecta Interaction With Bimodal Solar Wind

Details Numerical MHD Simulation of Flux-Rope Formed Ejecta Interaction With Bimodal Solar Wind Numerical MHD Simulation of Flux-Rope Formed Ejecta Interaction With Bimodal Solar Wind

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aipc..679..457w&link_type=abstract

SOLAR WIND TEN: Proceedings of the Tenth International Solar Wind Conference. AIP Conference Proceedings, Volume 679, pp. 457-4

Computer Science

6

Particle Emission, Solar Wind, Solar Wind Plasma, Sources Of Solar Wind

Scientific paper

A theoretic numerical simulation of interaction between CME ejecta and bimodal solar wind from solar surface to 30 solar radii has been presented. A comparison with an interaction between CME ejecta with homogeneous and bimodal solar wind is given. The results show that the bimodal solar wind changes the topology of CME ejecta with faster propagation speed away from the equator, and fast wind will energize the CME. Also the results of steady-state bimodal solar wind characteristics that extend to 1AU are presented.

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