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Cited article:

Artificial Intelligence for the Characterization of the 2024 May Superstorm: Active Region Classification, Flare Forecasting, and Geomagnetic Storm Prediction

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The Astrophysical Journal 985 (1) 53 (2025)
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Forbush decreases associated with coronal mass ejections from active and non-active regions: statistical comparison

A A Melkumyan, A V Belov, M A Abunina, A A Abunin, N S Shlyk, V A Oleneva and V G Yanke
Monthly Notices of the Royal Astronomical Society 515 (3) 4430 (2022)
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Forbush decreases caused by paired interacting solar wind disturbances

N S Shlyk, A V Belov, M A Abunina, A A Abunin, V A Oleneva and V G Yanke
Monthly Notices of the Royal Astronomical Society 511 (4) 5897 (2022)
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Over-expansion of a coronal mass ejection generates sub-Alfvénic plasma conditions in the solar wind at Earth

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Astronomy & Astrophysics 647 A149 (2021)
https://doi.org/10.1051/0004-6361/202039867