Solar-like activity in late-type stars

Details Solar-like activity in late-type stars Solar-like activity in late-type stars

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988iraj...18..257f&link_type=abstract

(Astronomocal Science Group of Ireland, Meeting, University College, Cork, Republic of Ireland, Mar. 31, 1988) Irish Astronomica

Astronomy and Astrophysics

Astronomy

Chromosphere, Late Stars, Stellar Activity, Ultraviolet Spectra, Astronomical Spectroscopy, Magnetic Flux, Solar Corona, Stellar Magnetic Fields, Stellar Models, Stellar Temperature

Scientific paper

Solar active structures such as magnetic flux tubes or large-scale active regions in the chromosphere and transition region have been studied from images and spectra in UV continua or chromospheric lines formed at different heights and temperatures. These active structures, reflecting subphotospheric magnetic field and the underlying dynamo and participating in the heating of the upper atmosphere, are also of particular importance for the study of stellar magnetic fields, internal dynamics, chromospheres and coronae.

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