Rope structure of a buoyant solar magnetic field

Details Rope structure of a buoyant solar magnetic field Rope structure of a buoyant solar magnetic field

Dec 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977pazh....3..554u&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal, vol. 3, Dec. 1977, p. 554-558. In Russian.

Physics

2

Magnetic Flux, Magnetohydrodynamic Stability, Solar Magnetic Field, Solar Physics, Chromosphere, Filaments, Solar Flares, Topology

Scientific paper

Plasma-stability theory is applied to a buoyant solar magnetic flux tube. Piddington's (1976) model is confirmed whereby a buoyant magnetic field splits up into flux ropes at the solar surface. It is shown that strong twisting of individual flux ropes as a result of the screw instability may disrupt the matter circulation within the ropes and produce a prominence by the Pikel'ner (1971) siphon mechanism. The equilibrium of an individual flux rope of large radius is evaluated.

Affiliated with

Also associated with

No associations

Rating

Rope structure of a buoyant solar magnetic field does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Rope structure of a buoyant solar magnetic field, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Rope structure of a buoyant solar magnetic field will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1419776