On the generation of magnetic fields in late-type stars - A local time-dependent dynamo model

Details On the generation of magnetic fields in late-type stars - A local time-dependent dynamo model On the generation of magnetic fields in late-type stars - A local time-dependent dynamo model

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...108..322r&link_type=abstract

Astronomy and Astrophysics, vol. 108, no. 2, Apr. 1982, p. 322-325.

Astronomy and Astrophysics

Astrophysics

45

Dynamo Theory, Late Stars, Magnetic Stars, Stellar Magnetic Fields, Stellar Models, Emission Spectra, Magnetic Flux, Solar Cycles, Stellar Evolution, Stellar Rotation, Time Dependence

Scientific paper

We assume that the magnetic field of late-type stars is generated in the lower part of the star's convection zone and study this generation mechanism with the help of local (in latitude) dynamo equations. For the spectral types GO, GS, KO, KS, MO, M2, and M5 we evaluate the magnetic field and period of the cycles as a function of rotation and compare them with the available observational data.

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