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This article has been cited by the following article(s):
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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) https://doi.org/10.1093/mnras/stac2017
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) https://doi.org/10.1093/mnras/stac478
Over-expansion of a coronal mass ejection generates sub-Alfvénic plasma conditions in the solar wind at Earth