Dynamical Evolution of Magnetic Flux Tube in the Solar Convective Zone

Details Dynamical Evolution of Magnetic Flux Tube in the Solar Convective Zone Dynamical Evolution of Magnetic Flux Tube in the Solar Convective Zone

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aca....48..789s&link_type=abstract

Acta Astronomica, v.48, pp.789-802, (1998).

Statistics

Computation

1

Sun: Magnetic Fields, Sun: Activity, Magnetohydrodynamics (Mhd)

Scientific paper

We present computations of nonlinear development of the kink instability in a horizontal magnetic flux tube lying initially in the deep convective zone. Obtained results are compared with an independent solution of the problem obtained formerly by Moreno-Insertis (1986). Consistency of solutions allows to evaluate the numerical code, in particular the treatment of the energy balance which is different than that of Moreno-Insertis.

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