Li, Xuebao https://orcid.org/0000-0003-0397-4372
Li, Xuefeng https://orcid.org/0009-0000-6353-5473
Zheng, Yanfang https://orcid.org/0000-0003-0229-3989
Li, Ting https://orcid.org/0000-0001-6655-1743
Yan, Pengchao https://orcid.org/0000-0002-3667-3587
Ye, Hongwei https://orcid.org/0009-0009-9722-5794
Zhang, Shunhuang https://orcid.org/0009-0003-0325-1366
Wang, Xiaotian https://orcid.org/0009-0004-1408-8055
Lv, Yongshang https://orcid.org/0009-0004-9110-0425
Huang, Xusheng https://orcid.org/0009-0008-1279-1870
Funding for this research was provided by:
MOST ∣ National Natural Science Foundation of China (12222306)
MOST ∣ National Natural Science Foundation of China (12473056)
MOST ∣ National Natural Science Foundation of China (11703009)
MOST ∣ National Natural Science Foundation of China (11803010)
JST ∣ Natural Science Foundation of Jiangsu Province (BK20241830)
JST ∣ Natural Science Foundation of Jiangsu Province (BK20170566)
JST ∣ Natural Science Foundation of Jiangsu Province (BK20201199)
Article Title: Prediction of Large Solar Flares Based on SHARP and High-energy-density Magnetic Field Parameters
Journal Title: The Astrophysical Journal Supplement Series
Article Type: paper
Copyright Information: © 2024. The Author(s). Published by the American Astronomical Society.
Publication dates
Date Received: 2024-06-04
Date Accepted: 2024-10-22
Online publication date: 2024-12-12