Thermodynamical properties of unresolved magnetic flux tubes
β Scribed by Egidio Landi Degl'Innocenti; Marco Landolfi
- Publisher
- Springer
- Year
- 1982
- Tongue
- English
- Weight
- 599 KB
- Volume
- 77
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
It has been suggested that the activity of cosmical magnetic fields is a consequence of a general topological nonequilibrium in the neighbourhood of magnetostatic equilibria. Evidence for this suggestion can be obtained from the Kolmogorov-Arnold-Moser theorem of classical mechanics, applied to the
Photometric and Doppler imaging observations of active binaries indicate the existence of starspots at preferred longitudes (position angles with respect to the companion star). We investigate the stability of magnetic flux tubes in the convection zone of close, fast-rotating binary stars and explor
A basic procedure is presented for dealing with the resonance problems that appear in MHD of which resonant absorption of waves at the Alfv~n resonance point is the best known example in solar physics. The procedure avoids solving the full fourth-order differential equation of dissipative MHD by usi