IMECH-IR  > 力学所知识产出(1956-2008)
On the magnetospheric structure of pulsars
Hu WR(胡文瑞); HU, WR (reprint author), ACAD SINICA,INST MECH,BEIJING,PEOPLES R CHINA.
Source PublicationChinese Physics
1982
Volume2Issue:3Pages:677-687
ISSN0273-429X
AbstractThe 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 BySCI
Language英语
WOS IDWOS:A1982NZ29100013
WOS Research AreaPhysics
WOS SubjectPhysics, Multidisciplinary
Citation statistics
Document Type期刊论文
Identifierhttp://dspace.imech.ac.cn/handle/311007/39950
Collection力学所知识产出(1956-2008)
Corresponding AuthorHU, 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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