activity
20042009
most citedDo mean-field dynamos in nonrotating turbulent shear-flows exist?

47 citations · 138 across the 7 of their papers we have counts for

collaborators
Showing astro-phShow all

9 papers · 1 filter

astro-ph200816 cited

Diamagnetic pumping near the base of a stellar convection zone

L. L. Kitchatinov, G. Rüdiger

The property of inhomogeneous turbulence in conducting fluids to expel large-scale magnetic fields in the direction of decreasing turbulence intensity is shown as important for the…

astro-ph20074 cited

Stability of toroidal magnetic fields in the solar tachocline and beneath

L. L. Kitchatinov, G. Rüdiger

Stability of toroidal magnetic field in a stellar radiation zone is considered for the cases of uniform and differential rotation. In the rigidly rotating radiative core shortly be…

astro-ph2007

Sunspot models with bright rings

L. L. Kitchatinov, G. Ruediger

A theoretical sunspot model is provided including magnetic suppression of the diffusivities and also a strong stratification of density and temperature. Heat diffusion alone with g…

astro-ph200746 cited

Stability of Toroidal Magnetic Fields in Rotating Stellar Radiation Zones

L. L. Kitchatinov, G. Ruediger

The questions of how strong magnetic fields can be stored in rotating stellar radiative zones without being subjected to pinch-type instabilities and how much radial mixing is prod…

astro-ph200725 cited

Structure and stability of the magnetic solar tachocline

G. Ruediger, L. L. Kitchatinov

Rather weak fossil magnetic fields in the radiative core can produce the solar tachocline if the field is poloidal and almost horizontal in the tachocline region, i.e. if the field…

astro-ph200647 cited

Do mean-field dynamos in nonrotating turbulent shear-flows exist?

G. Ruediger, L. L. Kitchatinov

A plane-shear flow in a fluid with forced turbulence is considered. If the fluid is electrically-conducting then a mean electromotive force (EMF) results even without basic rotatio…