CMEs during active solar phases are faster with stronger magnetic fields than in quiet phases (even after speed matching), while toroidal and poloidal field components decay similarly with distance and front-to-rear asymmetry increases.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
physics.space-ph 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Authors advocate precise terminology for interplanetary phenomena like CIRs over the broader SIR label and introduce Super CIR as a new category for exceptionally strong events from coronal hole jets.
citing papers explorer
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Evolution of Coronal Mass Ejection Properties through Superposed Epoch Analysis from 0.2 to 2.2 au
CMEs during active solar phases are faster with stronger magnetic fields than in quiet phases (even after speed matching), while toroidal and poloidal field components decay similarly with distance and front-to-rear asymmetry increases.
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"Corotating Interaction Regions (CIRs)", "Interaction Regions (IRs)" and "Stream Interaction Regions (SIRs)", which term should be used?
Authors advocate precise terminology for interplanetary phenomena like CIRs over the broader SIR label and introduce Super CIR as a new category for exceptionally strong events from coronal hole jets.