Calculation of plasma characteristics of the sun

Muhammad Abbas Bari; Jia Yong Zhong; Min Chen; Jing Zhao; Jie Zhang

doi:10.1088/1009-1963/15/11/020

Calculation of plasma characteristics of the sun

Muhammad Abbas Bari, Jia Yong Zhong, Min Chen, Jing Zhao, Jie Zhang^*

^*此作品的通讯作者

科研成果: 期刊稿件 › 文章 › 同行评审

1 引用（Scopus）

摘要

The ionization level and free electron density of most abundant elements (C, N, O, Mg, Al, Si, S, and Fe) in the sun are calculated from the centre of the sun to the surface of the photosphere. The model and computations are made under the assumption of local thermodynamic equilibrium (LTE). The Saha equation has been used to calculate the ionization level of elements and the electron density. Temperature values for calculations along the solar radius are taken from references.

源语言	英语
文章编号	020
页（从-至）	2578-2582
页数	5
期刊	Chinese Physics
卷	15
期	11
DOI	https://doi.org/10.1088/1009-1963/15/11/020
出版状态	已出版 - 1 11月 2006
已对外发布	是

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Bari, M. A., Zhong, J. Y., Chen, M., Zhao, J., & Zhang, J. (2006). Calculation of plasma characteristics of the sun. Chinese Physics, 15(11), 2578-2582. 文章 020. https://doi.org/10.1088/1009-1963/15/11/020

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keywords = "Ionization balance, Plasma characteristics, Saha equation",

author = "Bari, {Muhammad Abbas} and Zhong, {Jia Yong} and Min Chen and Jing Zhao and Jie Zhang",

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AU - Bari, Muhammad Abbas

AU - Zhong, Jia Yong

AU - Chen, Min

AU - Zhao, Jing

AU - Zhang, Jie

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N2 - The ionization level and free electron density of most abundant elements (C, N, O, Mg, Al, Si, S, and Fe) in the sun are calculated from the centre of the sun to the surface of the photosphere. The model and computations are made under the assumption of local thermodynamic equilibrium (LTE). The Saha equation has been used to calculate the ionization level of elements and the electron density. Temperature values for calculations along the solar radius are taken from references.

AB - The ionization level and free electron density of most abundant elements (C, N, O, Mg, Al, Si, S, and Fe) in the sun are calculated from the centre of the sun to the surface of the photosphere. The model and computations are made under the assumption of local thermodynamic equilibrium (LTE). The Saha equation has been used to calculate the ionization level of elements and the electron density. Temperature values for calculations along the solar radius are taken from references.

KW - Ionization balance

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Calculation of plasma characteristics of the sun

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