Magnetic activity in the extreme ultraviolet.

Details Magnetic activity in the extreme ultraviolet. Magnetic activity in the extreme ultraviolet.

Feb 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999tjph...23..399m&link_type=abstract

Turk. J. Phys., Vol. 23, No. 2, p. 399 - 413

Astronomy and Astrophysics

Astronomy

Cool Stars: Stellar Coronae, Cool Stars: Magnetic Fields

Scientific paper

The wealth of astronomical observations obtained in the extreme ultraviolet in recent years, have allowed comprehensive studies of the stellar transition regions and coronae to be carried out. For the first time the author has been able to resolve individual coronal lines of various elements formed over a large temperature range (105 - 107.2K). The temperature, densities, abundances and magnetic field strengths of the stellar coronae can now be determined. The author reviews some of the observations in the field of cool stars and discusses the implications on atmospheric heating requirements.

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