Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975azh....52..351v&link_type=abstract
Astronomicheskii Zhurnal, vol. 52, Mar.-Apr. 1975, p. 351-358. In Russian.
Astronomy and Astrophysics
Astronomy
Astronomical Models, Convection Currents, Magnetic Field Configurations, Solar Cycles, Stellar Envelopes, Stellar Magnetic Fields, Lines Of Force, Magnetic Flux, Toroids, Viscosity
Scientific paper
A hypothesis is discussed, according to which the magnetic field in convective shells of stars compensates for the mean azimuthal force (which is equivalent to negative viscosity) generated by convective motions. Some examples are cited which support the existence of a negative viscosity effect. The hypothesis postulates that the azimuthal force is expanded both for sustaining the differential rotation of the medium and the stretching of the lines of forces in the formation of a toroidal field from a poloidal one. It also assumes that the change in direction of the poloidal field component occurs at the end of the amplification phase in a certain layer located below the main amplification zone of the field, and that the mechanism of this change is associated with instability.
No associations
LandOfFree
A possible mechanism of the solar cycle does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with A possible mechanism of the solar cycle, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A possible mechanism of the solar cycle will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-947759