Equilibrium and non-equilibrium of two-arch structures in the solar atmosphere

Details Equilibrium and non-equilibrium of two-arch structures in the solar atmosphere Equilibrium and non-equilibrium of two-arch structures in the solar atmosphere

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989cha%26a..13..432s&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 13, Issue 4, p. 432-441.

Astronomy and Astrophysics

Astrophysics

Sun--Solar Activity--Equilibrium--Non-Equilibrium --Nonlinear Differential Equations

Scientific paper

We have derived a similarity solution in the form of a power series of the nonlinear magnetostatic equilibrium equation and identified the region of convergence in the parameter space. Within this region we have equilibrium configurations, outside it, non-equilibrium configurations. An example of nonlinear equilibrium configuration is shown graphically.
Our results can be used to explain the generation of multi-ribbon flares, the two-arch structures and the structures of the magnetic fields above elongated sunspot groups.

Affiliated with

Also associated with

No associations

Rating

Equilibrium and non-equilibrium of two-arch structures in the solar atmosphere 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 Equilibrium and non-equilibrium of two-arch structures in the solar atmosphere, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Equilibrium and non-equilibrium of two-arch structures in the solar atmosphere will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1569025