THE "FORCE-FREE SURFACE" OF THE MAGNETIZED CELESTIAL BODIES

被引:0
|
作者
Epp, V. [1 ,2 ]
Masterova, M. A. [1 ,3 ]
机构
[1] Tomsk State Pedag Univ, Tomsk 634061, Russia
[2] Tomsk State Univ, Tomsk 634050, Russia
[3] Tomsk Polytech Univ, Tomsk 634050, Russia
来源
ACTA PHYSICA POLONICA B | 2015年 / 46卷 / 08期
关键词
EFFECTIVE POTENTIAL-ENERGY; PULSAR; RADIATION; SPHERE;
D O I
10.5506/APhysPolB.46.1593
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The field of a uniformly magnetized rotating sphere is studied with special attention to the surface, where the electric and magnetic fields are orthogonal to each other. The equation of this surface, valid at arbitrary distances from the rotating magnetized sphere, is obtained. Inside the light cylinder, this surface can be considered as a force-free surface, i.e. as a place where the particles with strong radiation damping can be trapped due to their energy loss. Outside the light cylinder, this surface makes just a geometric locus which moves with a superlight velocity around the axis of rotation. The 2- and 3-dimensional plots of the force-free surface are constructed. Estimation of influence of the centrifugal force on the particle dynamics is made. It is shown that in the case of strong magnetic field, the centrifugal force is negligible small everywhere except a narrow neighbourhood of the light cylinder.
引用
收藏
页码:1593 / 1602
页数:10
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