Nevertheless, the visually estimated trend of the minimum peak flux shows an increasing trend with frequency, which can be described as \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${\log }_{10}({I}_{0D})=-0.76+2.13\times 1{0}^{-2}f$$\end{document} log 10 ( I 0 D ) = − 0.76 + 2.13 × 1 0 − 2 f .
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Imaging spectroscopy reveals spike-like repeating radio burst pairs in the solar corona.
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