Damped transverse oscillations of interacting coronal loops
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361/201526919/pdf
Reference47 articles.
1. Abramowitz, M., & Stegun, I. A. 1972, Handbook of Mathematical Functions (National Bureau of Standards – U.S. Government Printing Office)
2. Modified Kelvin‐Helmholtz Instabilities and Resonant Flow Instabilities in a One‐dimensional Coronal Plume Model: Results for Plasma \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 $\beta =0$ \end{document}
3. The influence of the internal structuring of coronal loops on the properties of their damped transverse oscillations
4. The Resonant Damping of Fast Magnetohydrodynamic Oscillations in a System of Two Coronal Slabs
5. Coronal Loop Oscillations Observed with theTransition Region and Coronal Explorer
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3. Magnetohydrodynamic Waves in the Solar Corona;Annual Review of Astronomy and Astrophysics;2020-08-18
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