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général - iate.europa.eu
The variability of active galactic nuclei and the radial transport of vertical magnetic flux... In gas pressure dominated disks the poloidal magnetic field will move outward at a rate comparable to its inward advection....
général - core.ac.uk - PDF: core.ac.uk
Submitted to apj the effect of poloidal magnetic field on type i planetary migration: significance of magnetic resonanceWe study the effect of poloidal magnetic field on type I planetary migration by linear perturbation analysis in the shearing-sheet approximation and the analytic results are compared with numerical ...
Viscous dissipative effects in white dwarfs and neutron stars...i.e., its magnetic symmetry axis is inclining at a gradually increasing angle with respect to its invariant angular momentum axis up to the perpendicular position (situation known as “perpendicular rotator”), the poloidal magnetic field causes interchange of angular momentum via hydromagnetic Alfven waves propagating along the poloidal magnetic field lines and, accordingly, the resulting...
Self-similar solutions of viscous-resistive adafs with poloidal magnetic fields... We consider an axisymmetric, rotating,isotheral steady accretion flow which contains a poloidal magnetic field of thecentral star....
 PDF: arxiv.org
On the energy of the poloidal magnetic field near the ionosphere... The generation of the Hall current (together with the associated poloidal magnetic field) will be shown to occur during the growth stage, when the electromagnetic energy is pumped through the divergent Hall current, regardless of how slow the...

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