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MHD simulation of a propagation of loop-like and bubble-like magnetic clouds (1995)

Vandas, M. ; Dryer, M. ; Fischer, S. ; [et al.]

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Publication Date: 2011-08-24

Description: Propagation and evolution of magnetic clouds in the ambient solar wind flow is studied self-consistently using ideal MHD equations in three dimensions. Magnetic clouds as ideal force-free objects (cylinders or spheres) are ejected near the Sun and followed beyond the Earth's orbit. We investigate the influence of various initial parameters like the injection velocity, magnetic field strength, magnetic helicity, orientation of the clouds' axis, etc., on their propagation and evolution. We demonstrate that the injection velocity and magnetic field strength have a major influence on propagation. Simulation results are compared with analytical solutions of magnetic cloud evolution.

Keywords: Solar Physics

Type: International Solar Wind 8 Conference; 101; NASA-CR-199940

Format: text

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