The periods of stellar models with linked poloidal-toroidal magnetic fields

Details The periods of stellar models with linked poloidal-toroidal magnetic fields The periods of stellar models with linked poloidal-toroidal magnetic fields

Jul 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978ap%26ss..56..473m&link_type=abstract

Astrophysics and Space Science, vol. 56, no. 2, July 1978, p. 473-478.

Astronomy and Astrophysics

Astrophysics

5

Magnetic Field Configurations, Magnetic Stars, Periodic Variations, Perturbation Theory, Stellar Magnetic Fields, Stellar Models, Modes (Standing Waves), Oscillations, Pulse Rate, Toroids

Scientific paper

First-order perturbation theory results for the changes in pulsation frequencies of a Cowling model star containing a magnetic field with both poloidal and toroidal components are presented. A toroidal field large enough to stabilize the poloidal field may reverse the sign of the frequency change caused by a purely poloidal field for some modes, including the fundamental radial mode

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