Magnetohydrodynamic behaviour of disturbance of finite amplitude magnetic field in the solar atmosphere

Details Magnetohydrodynamic behaviour of disturbance of finite amplitude magnetic field in the solar atmosphere Magnetohydrodynamic behaviour of disturbance of finite amplitude magnetic field in the solar atmosphere

Apr 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983chjss...3..113l&link_type=abstract

Chinese Journal of Space Science, vol. 3, April 1983, p. 113-121. In Chinese, with abstract in English.

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Computation

Magnetic Field Configurations, Magnetohydrodynamic Stability, Plasma Dynamics, Solar Activity, Solar Atmosphere, Solar Magnetic Field, Force-Free Magnetic Fields, Magnetohydrodynamic Waves, Nonlinear Evolution Equations, Potential Fields, Solar Flux

Scientific paper

Dynamic processes in the solar atmosphere are studied numerically from a complete set of MHD equations. Computational results are presented which quantitatively give the nonlinear evolution of strong magnetic fields. These results may help explain coronal transients, surge, spray, and eruptive prominence events in the solar atmosphere, as well as help model plasma behavior in high beta structure experiments in the laboratory.

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