A study of the physical mechanisms for filament eruption and coronal mass ejection via numerical simulation

Details A study of the physical mechanisms for filament eruption and coronal mass ejection via numerical simulation A study of the physical mechanisms for filament eruption and coronal mass ejection via numerical simulation

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992alab.reptq....w&link_type=abstract

Progress Report, 1 Jan. - 31 Dec. 1992 Alabama Univ., Huntsville. Dept. of Mechanical Engineering.

Computer Science

Numerical Analysis

Force-Free Magnetic Fields, Magnetohydrodynamics, Mathematical Models, Solar Flux, Stellar Mass Ejection, Two Dimensional Models, Nonlinear Systems, Numerical Analysis, Steady State

Scientific paper

During this period of performance (1 Jan. 1992 - 31 Dec. 1992), the investigation of the following tasks was accomplished: (1) application of the Non-linear Force-free Field (NLFF) Model to study the active region evolution; (2) coronal dynamical responses due to emerging flux including the transition region; (3) loss of MHD equilibrium due to footpoint motions; and (4) two-dimensional MHD global coronal model: steady-state streamers. The detailed description of these studies are included.

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