𝔖 Bobbio Scriptorium
✦   LIBER   ✦

Fluctuating dynamo models

✍ Scribed by R. Friedrich

Publisher
Elsevier Science
Year
1989
Tongue
English
Weight
411 KB
Volume
137
Category
Article
ISSN
0375-9601

No coin nor oath required. For personal study only.

πŸ“œ SIMILAR VOLUMES

Dynamically consistent spherical mean-fi
Dynamically consistent spherical mean-field dynamo models
✍ H. Fuchs; K.-H. RΓ€dler; M. Rheinhardt; M. SchΓΌler πŸ“‚ Article πŸ“… 1995 πŸ› Elsevier Science 🌐 English βš– 602 KB

Ah&met-Spherical mean-field dynamo models are considered which involve in part the interaction between the magnetic field and the motion of the electrically conducting fluid. Whereas the influence of the magnetic field on the small-scale motions responsible for the o-effect is ignored, the effect of

Polar branches of stellar activity waves
Polar branches of stellar activity waves: Dynamo models
✍ D.D. Sokoloff; A.F. Lanza; D.L. Moss; S.M. Tarbeeva πŸ“‚ Article πŸ“… 2011 πŸ› John Wiley and Sons 🌐 English βš– 518 KB

## Abstract Stellar activity data provide evidence that some activity wave branches propagate polewards rather than equatorwards (the latter being the solar case). This evidence is especially pronounced for the well‐observed subgiant HR 1099. For this star, the polar branch seems to coexist with an