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Comparison between statistical properties of Forbush decreases caused by solar wind disturbances from coronal mass ejections and coronal holes
Authors:AA Melkumyan  AV Belov  MA Abunina  AA Abunin  EA Eroshenko  VG Yanke  VA Oleneva
Institution:1. Gubkin Russian State University of Oil and Gas (National Research University), 65 Leninsky Prospect, Moscow 119991, Russia;2. Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation Russian Academy of Sciences, IZMIRAN, Kaluzhskoe Hwy 4, Troitsk, Moscow 108840, Russia
Abstract:
Keywords:Forbush decrease  Coronal mass ejection  Coronal hole  Solar wind  Statistical analysis
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