Counter-Streaming Velocities in a Quiescent Filament
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DOI: 10.1007/s11207-025-02509-w
Abstract: Filaments/prominences are cold plasma (≈104\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$\approx 10^{4}$\end{document} K) embedded in the solar corona, two orders of magnitude hotter. Filament plasma is structured by the magnetic field in… read more here.
Keywords: document; filament; streaming velocities; usepackage ... See more keywords