CAOSP abstracts, Volume: 38, No.: 2, year: 2008

Abstract: 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.

Full text version of this article in PostScript (600dpi) format compressed by gzip; or in PDF.

Back to:
CAOSP Vol. 38 No. 2 index
CAOSP archive main index
CAOSP main page
Astronomical Institute home page
Valid XHTML 1.0! Valid CSS!

Last update: April 17, 2008