IMECH-IR  > 力学所知识产出(1956-2008)
Non-axisymmetric magnetostatic equilibrium with strong twisted component of magnetic field
Hu WR(胡文瑞); Long H(隆辉)
Source PublicationScientia Sinica Series A-Mathematical Physical Astronomical & Technical Sciences
1988
Volume31Issue:2Pages:192-205
ISSN0253-5831 
AbstractThe perturbation theory is applied further to the discussion of the equilibrium properties of a sunspot-like magnetic field with a strong twisted component. The basic state reduces to the usual one discussed extensively for the axisymmetric magnetostatic equilibrium with twisted component of magnetic field, and the perturbed state is described by two coupled equations. As the magnetic force-line is twisted, there is a magnetic tension in the azimuthal direction. In this case, the perturbed total pressure is no longer independent of the azimuthal variable θ, and the magnetic field in the dark penumbal fibril may be either stronger or weaker relatively.
Indexed BySCI
Language英语
WOS IDWOS:A1988M458800007
WOS Research AreaScience & Technology - Other Topics
WOS SubjectMultidisciplinary Sciences
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Document Type期刊论文
Identifierhttp://dspace.imech.ac.cn/handle/311007/39696
Collection力学所知识产出(1956-2008)
Recommended Citation
GB/T 7714
Hu WR,Long H. Non-axisymmetric magnetostatic equilibrium with strong twisted component of magnetic field[J]. Scientia Sinica Series A-Mathematical Physical Astronomical & Technical Sciences,1988,31,2,:192-205.
APA 胡文瑞,&隆辉.(1988).Non-axisymmetric magnetostatic equilibrium with strong twisted component of magnetic field.Scientia Sinica Series A-Mathematical Physical Astronomical & Technical Sciences,31(2),192-205.
MLA 胡文瑞,et al."Non-axisymmetric magnetostatic equilibrium with strong twisted component of magnetic field".Scientia Sinica Series A-Mathematical Physical Astronomical & Technical Sciences 31.2(1988):192-205.
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