Knowledge Management System of Institue of Mechanics, CAS
On the magnetospheric structure of pulsars | |
Hu WR(胡文瑞)![]() | |
Source Publication | Chinese Physics
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1982 | |
Volume | 2Issue:3Pages:677-687 |
ISSN | 0273-429X |
Abstract | The magnetospheric structure of a pulsar is discussed for a non-force-free magnetic field. The local solution to the axisymmetric equations of the pulsar is obtained by the method of expanding in the polar angle. Particular attention is given to the solutions near the polar axis and the equator. Near the pulsar surface, the magnetic field energy density is found to be larger than the other energy components; the gravitational potential and the kinetic energy are relatively larger far away from the pulsar surface. It is shown that these relations influence the mass distribution in the pulsar magnetosphere. The results also show that the plasma rotation may be nonrigid and, hence, that a corotational region with a closed magnetic field may not exist. |
Indexed By | SCI |
Language | 英语 |
WOS ID | WOS:A1982NZ29100013 |
WOS Research Area | Physics |
WOS Subject | Physics, Multidisciplinary |
Citation statistics | |
Document Type | 期刊论文 |
Identifier | http://dspace.imech.ac.cn/handle/311007/39950 |
Collection | 力学所知识产出(1956-2008) |
Corresponding Author | HU, WR (reprint author), ACAD SINICA,INST MECH,BEIJING,PEOPLES R CHINA. |
Recommended Citation GB/T 7714 | Hu WR,HU, WR . On the magnetospheric structure of pulsars[J]. Chinese Physics,1982,2,3,:677-687. |
APA | 胡文瑞,&HU, WR .(1982).On the magnetospheric structure of pulsars.Chinese Physics,2(3),677-687. |
MLA | 胡文瑞,et al."On the magnetospheric structure of pulsars".Chinese Physics 2.3(1982):677-687. |
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