Prominence support in helical coronal fields formed by photospheric motions

Details Prominence support in helical coronal fields formed by photospheric motions Prominence support in helical coronal fields formed by photospheric motions

Aug 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993soph..146..277r&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 146, no. 2, p. 277-296.

Physics

18

Cold Plasmas, Dense Plasmas, Photosphere, Solar Corona, Solar Limb, Solar Prominences, Gravitational Effects, Helical Flow, Solar Gravitation, Solar Magnetic Field

Scientific paper

We consider the effect of converging photospheric motions acting upon a
sheared cylindrically-symmetric line-tied arcade. The motions drive a
reconnection process whereby a helical structure is formed, in which
cool, dense plasma may accumulate at the lowest points of the helical
windings thus creating a prominence.

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