Mass motions in optically thin solar transition zone lines
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/195/2/107/
Cited by 25 articles. 订阅此论文施引文献 订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献
1. HIGH SPATIAL RESOLUTION Fe xii OBSERVATIONS OF SOLAR ACTIVE REGIONS;The Astrophysical Journal;2016-08-11
2. The Relationship of the Chromosphere to the Lower Solar Transition Region;The Astrophysical Journal;2004-07-10
3. Properties of the Lower Transition Region: The Widths of Optically Allowed and Intersystem Spectral Lines;The Astrophysical Journal;2004-01-10
4. Solar EUV spectroscopic observations with SOHO/CDS;Astronomy & Astrophysics;2001-11
5. Extreme‐Ultraviolet Spectral Line Widths in Quiet‐Sun Coronal Plasmas at Distances of \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $1.03\leq R_{\odot }\leq 1.45$ \end{document} along the Solar Equatorial Plane;The Astrophysical Journal;2000-01-20
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