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Katsova & Livshits poster paper on CS-11

Katsova M. M., Livshits M. A.

Role of Large-Scale Magnetic Fields in Stellar Activity Phenomena

keywords: late-type stars, activity, magnetic fields.


This paper was presented as a poster at "11th Cambridge Workshop on COOL STARS, STELLAR SYSTEMS AND THE SUN" was held at Puerto de la Cruz, Tenerife, Spain in October 4th - 8th, 1999. It will be available on CS-11 Proceedings CD-ROM.

You may see figures of this paper below... or download the whole paper in PostScript or LaTeX source, everything compressed by ZIP.

LaTeX notes: you would need some specific LaTeX styles. See CS-11 HomePage for more. Figures are in EPS (Encapsulated PostScript) format to be inserted using software like dvips.

You can download these files via ftp. If you use GIF format, choose "Save Image As..." on the images below, or click here: first and second.


Figure 1. The force lines of magnetic fields and the structure of the white-light corona during July 11, 1991 eclipse. Calculations were carried out with an assumption of the radial magnetic field on the source surface. (With permission of V.N.Obridko and J.Sykora ( See also Sykora J., Ambroz P., Minarovjech M., Obridko V.N., Pinter T., Rybansky M. 1998, in: Solar Jets and Coronal Plumes, ESA SP-421, 79.).)