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. https://www.marketingjeunesse.com/product-category/whip/
Prediction of Large Solar Flares Based on SHARP and High-energy-density Magnetic Field Parameters
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