Prediction of Large Solar Flares Based on SHARP and High-energy-density Magnetic Field Parameters

Prediction of Large Solar Flares Based on SHARP and High-energy-density Magnetic Field Parameters

The existing flare prediction primarily relies on photospheric magnetic field parameters from the entire active region (AR), such as Space-Weather HMI Activity Region Patches (SHARP) parameters. However, these parameters may not capture the details of the AR evolution preceding flares. The magnetic...

Full description

Saved in:
Bibliographic Details
Main Authors: Xuebao Li, Xuefeng Li, Yanfang Zheng, Ting Li, Pengchao Yan, Hongwei Ye, Shunhuang Zhang, Xiaotian Wang, Yongshang Lv, Xusheng Huang
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal Supplement Series
Subjects:
Solar activity
Solar flares
Solar active region magnetic fields
Astronomy data analysis
Online Access:https://doi.org/10.3847/1538-4365/ad8b2a
Tags: Add Tag
No Tags, Be the first to tag this record!

Internet

https://doi.org/10.3847/1538-4365/ad8b2a

Similar Items