Equilibrium and Stability of Prominence Flux Ropes

Details Equilibrium and Stability of Prominence Flux Ropes Equilibrium and Stability of Prominence Flux Ropes

May 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000spd....31.0146f&link_type=abstract

American Astronomical Society, SPD Meeting #31, #01.46; Bulletin of the American Astronomical Society, Vol. 32, p.809

Statistics

Computation

Scientific paper

We present two-dimensional equilibrium solutions to the MHD equations relevant to solar prominences. Computationally determined configurations are found that have realistic pressure, density, and temperature profiles, supported by nearly force-free, flux rope-type magnetic fields. The stability of such equilibria to gravity and pressure driven modes is determined. The evolution of marginally unstable equilibria is discussed within the framework of a nonlinear dynamical theory for pressure and gravity driven modes. The National Center for Atmospheric Research is sponsored by the National Science Foundation

Affiliated with

Also associated with

No associations

Rating

Equilibrium and Stability of Prominence Flux Ropes 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 Stability of Prominence Flux Ropes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Equilibrium and Stability of Prominence Flux Ropes will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1348107