The spontaneous magnetization of a one-dimensional model of a ferromagnetic toroid in a magnetic field

1955 ◽  
Vol 5 (3) ◽  
pp. 291-298 ◽  
Author(s):  
Luboš Valenta
1961 ◽  
Vol 10 (3) ◽  
pp. 473-479 ◽  
Author(s):  
J. W. Dungey

A one-dimensional model with no magnetic field is considered. It is supposed that the plasma starts in thermal equilibrium and then a current is forced to grow. Instability leads to the growth of waves, which are shown to stir the distribution in phase space, but only over a limited range of velocity. It is concluded that in order to restore stability the energy in the wave must become comparable to the energy of drift.


2014 ◽  
Vol 10 (S305) ◽  
pp. 238-244
Author(s):  
I. Milić ◽  
M. Faurobert

AbstractOne of the methods for diagnosing vector magnetic fields in solar prominences is the so called “inversion” of observed polarized spectral lines. This inversion usually assumes a fairly simple generative model and in this contribution we aim to study the possible systematic errors that are introduced by this assumption. On two-dimensional toy model of a prominence, we first demonstrate importance of multidimensional radiative transfer and horizontal inhomogeneities. These are able to induce a significant level of polarization in Stokes U, without the need for the magnetic field. We then compute emergent Stokes spectrum from a prominence which is pervaded by the vector magnetic field and use a simple, one-dimensional model to interpret these synthetic observations. We find that inferred values for the magnetic field vector generally differ from the original ones. Most importantly, the magnetic field might seem more inclined than it really is.


2004 ◽  
Vol 21 (7) ◽  
pp. 1344-1347
Author(s):  
Tian Ye ◽  
Kong Xiang-Yan ◽  
Wang Hui-Wu ◽  
Zhao Shi-Ping ◽  
Chen Geng-Hua ◽  
...  

2009 ◽  
Vol 87 (4) ◽  
pp. 329-336 ◽  
Author(s):  
Magdy A. Ezzat ◽  
Alaa Abd El Bary ◽  
Ahmed S. El Karamany

A one-dimensional model of the two-temperature generalized magneto-viscoelasticity with two relaxation times in a perfect conducting medium is established. The state space approach is adopted for the solution of one-dimensional problems for any set of boundary conditions. The resulting formulation together with the Laplace transform techniques are applied to a specific problem of a half-space subjected to thermal shock and traction-free surface. The inversion of the Laplace transforms is carried out using a numerical approach. Numerical results are given and illustrated graphically for the problem. Some comparisons have been shown in figures to estimate the effects of the temperature discrepancy and the applied magnetic field.


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