3-D MHD Simulations of Flux Tube Emergence

Details 3-D MHD Simulations of Flux Tube Emergence 3-D MHD Simulations of Flux Tube Emergence

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agusm..sh41a10a&link_type=abstract

American Geophysical Union, Spring Meeting 2001, abstract #SH41A-10

Astronomy and Astrophysics

Astrophysics

7500 Solar Physics, Astrophysics, And Astronomy, 7524 Magnetic Fields

Scientific paper

We present initial results from coupled 3-D MHD simulations of twisted magnetic flux tubes that have risen through a model solar convection zone and emerged into the lower corona. We use the anelastic code ``ANMHD'' to simulate the rise of buoyant flux tubes through the solar convection zone, and use this data to generate a photospheric boundary that drives a simple simulation of the solar transition region and corona using a modified version of the publicly available code ``ZEUS3D''

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