On a peculiar type of prominence activation

Details On a peculiar type of prominence activation On a peculiar type of prominence activation

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984basi...12..252p&link_type=abstract

Astronomical Society of India, Bulletin, vol. 12, Sept. 1984, p. 252-257.

Mathematics

Logic

3

Chromosphere, Magnetohydrodynamic Stability, Solar Activity, Solar Prominences, Coronal Loops, Solar Magnetic Field

Scientific paper

Time-lapse H-alpha observations of a peculiar type of prominence activation on October 7, 1981, are presented, and its morphological behavior is described. The prominence material seems to have originated from the photosphere as a huge twisted ropelike structure. It reached a height of about 100,000 km and later on split into braided closed looplike features which remained stable for a few minutes before breaking up at the top of the loop and finally fading out. The splitting of the twisted ropelike structure is explained on the basis of a screw-type instability in the current-carrying plasma column.

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