3D MHD Simulation of Flux Tube Dynamics: Comparison with Thin Flux Tube Models

Details 3D MHD Simulation of Flux Tube Dynamics: Comparison with Thin Flux Tube Models 3D MHD Simulation of Flux Tube Dynamics: Comparison with Thin Flux Tube Models

May 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000spd....31.0135f&link_type=abstract

American Astronomical Society, SPD Meeting #31, #01.35; Bulletin of the American Astronomical Society, Vol. 32, p.807

Astronomy and Astrophysics

Astronomy

Scientific paper

We have used the anelastic 3D MHD code ``ANMHD'' to perform simulations of emerging magnetic flux tubes moving in a gravitationally stratified background model representing the solar convection zone. The MHD model is computed within a local Cartesian geometry, with Coriolis forces included, using the f-plane approximation. The evolution of flux tubes computed with the code will be compared and contrasted with results computed with the thin flux tube approximation. This work was supported by NASA and NSF.

Affiliated with

Also associated with

No associations

Rating

3D MHD Simulation of Flux Tube Dynamics: Comparison with Thin Flux Tube Models 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 3D MHD Simulation of Flux Tube Dynamics: Comparison with Thin Flux Tube Models, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and 3D MHD Simulation of Flux Tube Dynamics: Comparison with Thin Flux Tube Models will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1348076