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Modelling coronal magnetic fields
Solar Physics, 1981The ‘hairy ball’ model of coronal magnetic fields has a spherical source surface separating potential and radial magnetic fields. In the present model the source surface is chosen such that the wind speed equals the Alfvenic speed at selected points on the source surface. Results have been obtained for a dipole base field and an isothermal corona.
D. P. Rowse, I. W. Roxburgh
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Electromagnet Model Through Magnetic Field Analysis
International Journal of Modelling and Simulation, 1987In this paper, parallel processing computer system models are considered, in which, each CPU service time of programs subdivides into independent parts (tasks) that can be processed in parallel.Dif...
CHIAMPI M., TARTAGLIA, Michele
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String Cosmological Models with Magnetic Field
General Relativity and Gravitation, 1999A new class of string cosmological models with and without magnetic field in the context of a spacetime with \(G_3\) symmetry has been presented. In order to study the effects of magnetic field, the standard energy-momentum tensor is modified by incorporating an additional term due to a magnetic field.
Singh, G. P., Singh, Triloki
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2011
The magnetic field modeling of the PM-pole rotor is presented. According to the magnetic characteristics of the three regions of the rotor space, Laplace’s equations of magnetic scalar potential are derived. By using the boundary conditions in between neighboring regions as well as the spherical harmonic expansion of radial component of the residual ...
Liang Yan +4 more
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The magnetic field modeling of the PM-pole rotor is presented. According to the magnetic characteristics of the three regions of the rotor space, Laplace’s equations of magnetic scalar potential are derived. By using the boundary conditions in between neighboring regions as well as the spherical harmonic expansion of radial component of the residual ...
Liang Yan +4 more
openaire +1 more source

