Ten years magnetic modelling of stars by field sources - a review

Details Ten years magnetic modelling of stars by field sources - a review Ten years magnetic modelling of stars by field sources - a review

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008coska..38..173g&link_type=abstract

Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 38, no. 2, p. 173-178.

Astronomy and Astrophysics

Astronomy

Stars: Magnetic Fields, Methods: Analytical

Scientific paper

Ten years ago Glagolevskij and Gerth proposed a modelling method to construct the magnetic field out of its sources and vortices. The sources can be positioned inside and/or outside the star, filling by their superposed fields the entire space - the magneto-sensitive atmosphere included. On the basis of matrix and vector algebra there have been developed computer programs to calculate the stellar magnetic field by a straightforward strategy, thereby fitting to the observational facts. The review points only to some main aspects of the Magnetic Charge Method of magnetic modelling and refers to the literature.

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