Method for solving the problem of a magnetohydrodynamic dynamo

Details Method for solving the problem of a magnetohydrodynamic dynamo Method for solving the problem of a magnetohydrodynamic dynamo

Aug 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976zvmmf..16..956i&link_type=abstract

Zhurnal Vychislitel'noi Matematiki i Matematicheskoi Fiziki, vol. 16, June-Aug. 1976, p. 956-968. In Russian.

Astronomy and Astrophysics

Astronomy

Astronomical Models, Dynamo Theory, Magnetohydrodynamics, Solar Magnetic Field, Elliptic Differential Equations, Finite Difference Theory, Numerical Integration, Parabolic Differential Equations, Poisson Equation

Scientific paper

A method for solving a system of differential equations describing the hydrodynamic generation of the periodic magnetic field of the sun is developed. The initial problem consists of solving the nonstationary internal problem for a system of two parabolic equations and the external problem for a system of elliptic equations. The external problem is expressed through the Poisson integral along the boundary of the function to be sought. A finite difference scheme is used to solve the system of equations which is obtained.

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