Rapid motion of filaments - Eruptive prominences

Details Rapid motion of filaments - Eruptive prominences Rapid motion of filaments - Eruptive prominences

Feb 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992azh....69..181m&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 69, no. 1, Jan.-Feb. 1992, p. 181-191. In Russian.

Astronomy and Astrophysics

Astronomy

10

Photosphere, Plasma Dynamics, Solar Prominences, Spaceborne Astronomy, Dipole Moments, Plasma Currents, Velocity Distribution

Scientific paper

The rapid motion of filaments is interpreted as the result of the interaction between the filament current, the active region field, and the 'mirror' current field. A summary of velocity observations of eruptive prominences during their removal from the limb is presented. The filament energy integral is considered. The most rapid filament motion arises when loss of equilibrium occurs near the 'saddle' point of the potential surface. A comparison of parameters of eruptive prominences with finite and infinite motions is carried out on the basis of observations in June-July 1989.

Affiliated with

Also associated with

No associations

Rating

Rapid motion of filaments - Eruptive prominences 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 Rapid motion of filaments - Eruptive prominences, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Rapid motion of filaments - Eruptive prominences will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1047133