Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/71
Title: Fundamental Flux Tubes in the Solar Magnetic Fields: Generation of the FFT's and the periodic field reversal
Authors: Gokhale, M. H
Keywords: Solar Activity
Solat Magnetic Fields
Solar Convection
Magnetohydrodynamics
Issue Date: 1977
Publisher: Indian Institute of Astrophysics, Bangalore
Citation: Kodaikanal Observatory Bulletins Series A, Vol. 2, pp. 19-27
Abstract: It is conceviable that the periodic reversal of the Sun'd large-scale magnetic field and the concentration of the field in strong, thin flux tubes on small scales could bith result from the following likely processes near the base of the convection zone. It is likely that in a "base layer" of thickness ~10(power 5) km near the base of the convection zone a small part (~0.4%) of the energy flux below goes into an azimuthal magnetoaccoustic oscillation and once in ~ 11 y or so such an oscillation reaches a critical amplitude ~ 10 (power 4) cm s(power (-1)) when it undergoes a 'shock transition' to a cellular (azimuthal) convective mode. The shock transition will involve creation of electric current sheaths and magnetic flux sheaths of field intensity ~ 10 (power 4) G and thickness ~ 10 (power 2) km each near the 'nodal' meridian palnes. The electric current sheaths would provide the 'reserved' magnetic field on one side and the magnetic flux sheaths would eventually degenerated into 'cluster' of thousands of flux tubes of fluxes ~ 10 (power 18) Mx each. This model does need further detailed investigation; but if it is valid, it would be free from the difficulties of the earlier models of the solar magnetic cycle.
URI: http://hdl.handle.net/2248/71
ISSN: 0374-3632
Appears in Collections:IIAP Publications
Kodaikanal Observatory Bulletins (1905 - 1997 )

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