Stellar magnetic-cycle phasing

Details Stellar magnetic-cycle phasing Stellar magnetic-cycle phasing

Feb 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994pasp..106..145g&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 106, no. 696, p. 145-148

Astronomy and Astrophysics

Astronomy

9

Solar Convection (Astronomy), Solar Magnetic Field, Stellar Convection, Stellar Magnetic Fields, Stellar Temperature, Dynamo Theory, Photosphere, Solar Temperature, Sunspots

Scientific paper

During magnetic-cycle-type variations in dwarf stars, changes in the H
and K magnetic activity index precede changes in temperature by times
ranging from several years at GO down near zero at K2. These results are
preliminary, however, because they are based on observations of only
three stars.

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