Dynamic modeling of coronal transients and interplanetary disturbances

Details Dynamic modeling of coronal transients and interplanetary disturbances Dynamic modeling of coronal transients and interplanetary disturbances

Jul 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982uci..rept.....s&link_type=abstract

Final Technical Report California Univ., Irvine.

Computer Science

Numerical Analysis

Computerized Simulation, Solar Activity, Solar Corona, Solar Wind, Systems Simulation, Dynamic Models, Equations Of Motion, Magnetohydrodynamic Flow, Numerical Analysis, Solar Wind Velocity, Time Dependence

Scientific paper

The numerical simulation of the propagation of solar generated disturbances through the lower corona and the solar wind was investigated. The application of a numerical code to the study of a particular solar related phenomena is described. Two dimensional studies, and a one dimensional code are presented. The numerical solution of the time dependent dissipationless, magnetohydrodynamic equations of motion are studied.

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