tokens: We thank the referee for their helpful comments. This work was supported by the BK21 plus program through the National Research Foundation (NRF) funded by the Ministry of Education of Korea, the Basic Science Research Program through the NRF funded by the Ministry of Education (NRF-2016R1A2B4013131, NRF-2016R1A6A3A11932534, NRF-2019R1A2C1002634), the NRF of Korea Grant funded by the Korean Government (NRF-2013M1A3A3A02042232), the Korea Astronomy and Space Science Institute under the RD program supervised by the Ministry of Science, ICT and Future Planning, the Korea Astronomy and Space Science Institute under the RD program Development of a Solar Coronagraph on International Space Station (Project No. 2019-1-850-02) supervised by the Ministry of Science, ICT and Future Planning, and the Institute for Information communications Technology Promotion (IITP) grant funded by the Korea government (MSIP) (2018-0-01422, Study on analysis and prediction technique of solar flares). The data used here are provided courtesy of NASA/ SDO and the HMI science team, as well as the GOES team.
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