The structure of the meridian solar wind and its effect on the propagation of coronal mass ejections

Details The structure of the meridian solar wind and its effect on the propagation of coronal mass ejections The structure of the meridian solar wind and its effect on the propagation of coronal mass ejections

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991chjss..11..168g&link_type=abstract

Chinese Journal of Space Science (ISSN 0254-6124), vol. 11, no. 3, p. 168-175.

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2

Flow Distribution, Hydrodynamic Equations, Magnetohydrodynamics, Solar Wind, Stellar Mass Ejection, Computational Grids, Radial Distribution

Scientific paper

A combined scheme is developed to solve the ideal MHD equations. Keeping certain precision, this model has ensured stability and small computing capacity. A two-dimensional helmet streamer solution of the meridian solar wind near the sun is obtained. Using this solution as initial state, the effect of the helmet-streamer configuration on the propagation of coronal mass ejections is investigated. It is found that the configuration deflects the ejected mass toward equator. This effect can satisfactorily explain some observational results.

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