tokens: Acknowledgments The authors would like to thank the anonymous referee for valuable comments that improved the manuscript. We thank the teams of Fermi and GOES for their open data-use policy. This study is supported by the National Natural Science Foundation of China (NSFC) under grants 11603077, 11573072, 11333009, 973 programme (2014CB744200) and Laboratory No. 2010DP173032. DL is supported by the Youth Fund of Jiangsu No. BK20161095. QMZ is supported by the Surface Project of Jiangsu No. BK20161618 and the Youth Innovation Promotion Association CAS. The authors wish to thank the International Space Science Institute in Beijing (ISSI-BJ) for supporting and hosting the meetings of the International Team on ‘Magnetohydrodynamic Seismology of the Solar Corona in the Era of SDO/AIA', during which discussions leading to this publication were held.
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