Astronomy and Astrophysics – Astrophysics
Scientific paper
Mar 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996a%26a...307..293k&link_type=abstract
Astronomy and Astrophysics, v.307, p.293
Astronomy and Astrophysics
Astrophysics
50
Turbulence, Magnetohydrodynamics (Mhd), Instabilities, Sun: Oscillations, Sunspots
Scientific paper
As was previously shown (Kleeorin et al. 1990; Kleeorin & Rogachevskii 1994a), small-scale magnetohydrodynamic (MHD) turbulence results in modification of the Ampere law, by significantly reducing the elasticity of the magnetic field lines. As a result, the `effective' magnetic pressure is reduced and may even reverse its sign. We show here that this modification can be related to a variety of phenomena observed in the Sun and in particular the following four are investigated: the 11-year variations of the solar radius, the torsional oscillations and the meridional flows, the solar short time oscillations and the large-scale magnetic flux ropes formation in convective zones of the Sun (as well as in stars and spiral galaxies).
Kleeorin Nathan
Mond Michael
Rogachevskii Igor
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