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Calculation of plasma characteristics of the sun
Authors:Muhammad Abbas Bari  Zhong Jia-Yong  Chen Min  Zhao Jing and Zhang Jie
Affiliation:Laboratory of Optical Physics, Institute of Physics, Chinese academy of Sciences, Beijing 100080, China; National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
Abstract: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.
Keywords:Saha equation  ionization balance  plasma characteristics
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