A study of the physical mechanisms for filament eruption and coronal mass ejection via numerical simulation
Abstract
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.
- Publication:
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Alabama Univ., Huntsville Report
- Pub Date:
- December 1992
- Bibcode:
- 1992alab.reptQ....W
- Keywords:
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- Force-Free Magnetic Fields;
- Magnetohydrodynamics;
- Mathematical Models;
- Solar Flux;
- Stellar Mass Ejection;
- Two Dimensional Models;
- Nonlinear Systems;
- Numerical Analysis;
- Steady State;
- Solar Physics