Stellar flares - Pulsed processes in the atmospheres of late dwarfs

Details Stellar flares - Pulsed processes in the atmospheres of late dwarfs Stellar flares - Pulsed processes in the atmospheres of late dwarfs

Feb 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991azh....68..131k&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 68, Jan.-Feb. 1991, p. 131-157. In Russian.

Astronomy and Astrophysics

Astronomy

5

Late Stars, Red Dwarf Stars, Solar Flares, Stellar Atmospheres, Stellar Flares, Stellar Spectra, Gas Dynamics, Light Curve, Radio Spectra, Shock Fronts, Stellar Models, Visible Spectrum, X Ray Spectra

Scientific paper

Observations of the flares of red dwarfs in various spectral ranges are examined. The flares are shown to represent a highly dramatic stage of magnetic-field evolution in the atmospheres of late-type stars. The observed phenomena appear to occur in a sequence commencing with sudden short-duration releases of very small amounts of energy, and encompassing the multihour reconnection of the magnetic fields of immense coronal loops possibly located on different components of binary systems of RS CVn type. The total energies of the processes considered range from 10 to the 28th to 10 to the 37th erg, while the powers at maximum range from 10 to the 28th to 10 to the 30th erg/s.

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