𝔖 Bobbio Scriptorium
✦   LIBER   ✦

A nonlinear model of the solar dynamo

✍ Scribed by R. L. Jennings


Publisher
Springer
Year
1993
Tongue
English
Weight
822 KB
Volume
143
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.


πŸ“œ SIMILAR VOLUMES


Toward a dynamo model for the solar tach
✍ Rolando Lillo; Pablo D. Mininni; Daniel O. GΓ³mez πŸ“‚ Article πŸ“… 2005 πŸ› Elsevier Science 🌐 English βš– 271 KB

The generation of magnetic field on the Sun is caused by a dynamo mechanism, and is related with the differential rotation of the solar interior. Helioseismologic observations show that strong velocity gradients concentrate in a thin layer located at the base of the convective region, known as the t

The solar dynamo
✍ A. A. Ruzmaikin πŸ“‚ Article πŸ“… 1985 πŸ› Springer 🌐 English βš– 907 KB

The basic features of the solar activity mechanism are explained in terms of the dynamo theory of mean magnetic fields. The field generation sources are the differential rotation and the mean helicity of turbulent motions in the convective zone. A nonlinear effect of the magnetic field upon the mean

Nonlinear dynamo in a simplified statist
✍ Eun-jin Kim πŸ“‚ Article πŸ“… 1999 πŸ› Elsevier Science 🌐 English βš– 89 KB

A fully self-consistent nonlinear dynamo is studied in the limit of the low kinetic Reynolds number by adopting a simplified statistical model. Governing equations for the evolution of a mean magnetic field and correlation functions of fluctuating magnetic fields are derived for arbitrary values of

The nonlinear solar dynamo and different
✍ A. Brandenburg; D. Moss; G. RΓΌdiger; I. Tuominen πŸ“‚ Article πŸ“… 1990 πŸ› Springer 🌐 English βš– 533 KB

We consider dynamically consistent mean-field dynamos in a spherical shell of incompressible fluid. The generation of magnetic field and differential rotation is parameterized by the ~-and A-effects, respectively. Extending previous investigations, we include now the eases of moderate and rapid rota