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The turbulent magnetic prandtl number of mhd turbulence in disks... Phenomenological models of the evolution of large scale poloidal magnetic fields in disks suggest that the turbulent magnetic Prandtl number PrM,T controls the rate of escape of vertical field from the disk; for PrM,T ≤ R/H vertical...
général - core.ac.uk - PDF: citeseerx.ist.psu.edu
Gravitational collapse of polytropic, magnetized, filamentary clouds... If the axial motions and poloidal magnetic fields aresufficiently weak, we could reasonably expect our solutions to be a goodapproximation....
 PDF: arxiv.org
Old models for cygnus x-1 and agn... The goal of this electronic publication is to draw attention to our old papers where many ideas of recent discussions were anticipated (hot coronae, Comptonization, photon damping of waves, particle acceleration and matter ejection from accretion disks with large scale poloidal magnetic fields, etc.
 PDF: core.ac.uk
Gravitational waves and hydromagnetic instabilities in rotating magnetized neutron starsWe perform nonlinear general relativistic ideal magnetohydrodynamicsimulations of poloidal magnetic fields in rotating polytropic neutron stars.We...
 PDF: arxiv.org
A moment equation description of magnetic reversals in the earth... The link suggests that nonperiodic reversal is an intrinsic feature of the alpha dynamo equations provided the forcing is vigorous and the toroidal and poloidal magnetic fields are sufficiently out of phase....

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