The equilibrium configuration of the corona loop and the corona archide

Details The equilibrium configuration of the corona loop and the corona archide The equilibrium configuration of the corona loop and the corona archide

Jan 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982chjss...2...12h&link_type=abstract

Chinese Journal of Space Sciences, vol. 2, Jan. 1982, p. 12-20. In Chinese, with abstract in English.

Physics

3

Coronal Loops, Magnetic Effects, Solar Corona, Solar Magnetic Field, Equilibrium Equations, Fourier Transformation, Plasma Heating, Solar Flares, Solar Physics

Scientific paper

Assuming a linear field, the two-dimensional coronal loop configuration is presently given by an equation that may be solved by means of the Fourier transformation method. These theoretical results indicate that the pressure should be uniform along the loop, and that the loop configuration is more stable than that of the force field. Attention is also given to the influence of the shear magnetic field and pressure on the configuration. If more magnetic energy or magnetic shear is stored in the loop, the coronal loop will be driven to produce the corona transient process. Alternatively, the plasma will be heated or accelerated to produce solar flares if part of the stored energy is released.

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