Magnitude of the dynamo-generated magnetic field in solar-type convective zones

Details Magnitude of the dynamo-generated magnetic field in solar-type convective zones Magnitude of the dynamo-generated magnetic field in solar-type convective zones

May 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995a%26a...297..159k&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 297, no. 1, p. 159-167

Astronomy and Astrophysics

Astronomy

51

Solar Convection (Astronomy), Stellar Magnetic Fields, Stellar Magnitude, Stellar Models, Dynamic Models, Nonlinearity, Stellar Luminosity, Stellar Rotation, X Rays

Scientific paper

Using a nonlinear dynamo model (in a single-mode approximation), and analytical expression is derived which gives the magnitude of the mean magnetic field as a function of rotation and other parameters for a solar-type convection zone. By means of this expression we find a power-law relation between the X-ray luminosity and stellar rotation. The exponent in this relation is in agreement with observations.

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