NAOC Open IR
Corrections to Solar Thermal Structure when a Turbulent Magnetic Field is Included
Yi Liao; Bi Shaolan
2004
Source PublicationChinese Journal of Astronomy and Astrophysics
ISSN1009-9271
Volume4Issue:5Pages:490
AbstractCorrection of non-ideal effect due to a magnetic fluctuating tensor is derived from the ideal MHD equations. The inclusion of a magnetic turbulent field leads to modifications of the hydrostatic equilibrium equation and thermodynamical variables such as the temperature T, the adiabatic exponent γ, the adiabatic temcations in the adiabatic and radiative temperature gradients will result in a change in the Schwarzchild criterion, hence in the location of the base of the convective zone. Incorporating the modifications, we construct a modified thermodynamical equilibrium structure of the Sun.
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/47921
Collection中国科学院国家天文台
Affiliation中国科学院国家天文台
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Yi Liao,Bi Shaolan. Corrections to Solar Thermal Structure when a Turbulent Magnetic Field is Included[J]. Chinese Journal of Astronomy and Astrophysics,2004,4(5):490.
APA Yi Liao,&Bi Shaolan.(2004).Corrections to Solar Thermal Structure when a Turbulent Magnetic Field is Included.Chinese Journal of Astronomy and Astrophysics,4(5),490.
MLA Yi Liao,et al."Corrections to Solar Thermal Structure when a Turbulent Magnetic Field is Included".Chinese Journal of Astronomy and Astrophysics 4.5(2004):490.
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