Do the Line Widths of Coronal Emission Lines Increase with Height above the Limb?
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference30 articles.
1. Nonthermal Velocities in Different Temperature Regions of the Solar Lower Transition Region
2. Further Measurements of Emission Line Profiles in the Solar Ultraviolet Spectrum
3. The SOHO mission: An overview
4. 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
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