Electron density diagnostics by use of a collisional excitation model of the oxygen VI doublet in the solar transition region
Author:
Funder
National Natural Science Foundation of China
Publisher
Informa UK Limited
Subject
Spectroscopy,Atomic and Molecular Physics, and Optics,Analytical Chemistry
Link
http://www.tandfonline.com/doi/pdf/10.1080/00387010.2016.1231694
Reference20 articles.
1. An approximate calculation of the effect of opacity in the solar spectral lines of C III
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3. The Optically Thick FexviiSpectrum: X‐Ray, Extreme‐Ultraviolet, and Forbidden Line Ratios
4. Past and recent observations of the solar upper atmosphere at vacuum-ultraviolet wavelengths
5. Quantitative Magnetohydrodynamic Modeling of the Solar Transition Region
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1. Spectroscopic diagnostic of electron density for four-level system by collisional excitation model;Spectroscopy Letters;2021-06-01
2. Study on Electron Density Diagnostics of Si VIII Ion for Non-Maxwellian Distribution in Solar Transition Region;Astronomy Letters;2020-01
3. Spectroscopic diagnostics of electron density in a flare ribbon by oxygen IV lines using Non-Maxwellian distribution;Spectroscopy Letters;2019-10-24
4. Study of non-Maxwellian distributions of electron energies in the solar transition region;Journal of the Korean Physical Society;2017-01
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