A possible interpretation of the inhomogeneity and material motion within the post-flare loop of June 26, 1992.

Details A possible interpretation of the inhomogeneity and material motion within the post-flare loop of June 26, 1992. A possible interpretation of the inhomogeneity and material motion within the post-flare loop of June 26, 1992.

May 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998acasn..39..165y&link_type=abstract

Acta Astron. Sin., Vol. 39, No. 2, p. 165 - 171

Astronomy and Astrophysics

Astronomy

Solar Flares: Loops

Scientific paper

Using the theory of linear current instability, the authors discussed the possibility of inhomogeneous "knot" structures within the post-flare loop of June 25 - 26, 1992. Besides, by simultaneously considering the gravity of the Sun, magnetic stress within the loop and primary velocity at the top, the authors theoretically calculated the motion of matter within the post-flare loop. The theoretical results are in accord with observations.

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