@erikapal @theauroraguy @AndresCalabia @eelcodoornbos @halocme @chrisoutofspace @TamithaSkov The figure is in here: https://t.co/ytfaaDEMFP But the ICME start and end times are straight from Ian Richardson's list. I'd definitely debate a few of them, but
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RT @mathewjowens: Fast magnetic clouds are distinct from other interplanetary coronal mass ejections in terms of their coronal source prope…
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Solar Physics: Solar Wind and Heavy Ion Properties of Interplanetary Coronal Mass Ejections: Abstract Magnetic field and plasma properties of the solar wind measured in near-Earth space are a convolution of coronal source conditions and in-transit… https:/
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Fast magnetic clouds are distinct from other interplanetary coronal mass ejections in terms of their coronal source properties. Different initiation processes? https://t.co/pr7Kfmf4Hm