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ON THE ENHANCED CORONAL MASS EJECTION DETECTION RATE SINCE THE SOLAR CYCLE 23 POLAR FIELD REVERSAL

  • Authors: G. J. D. Petrie

2015 The Astrophysical Journal 812 74.

  • Provider: AAS Journals

Caption: Figure 5.

Stacked annual histograms of CME angular widths (left) and angular widths for all detections (middle) and for detections with angular width >30° (right), from the SEEDS (top), CACTus (middle), and CDAW (bottom) databases. The dotted lines in the left plots indicate the angular width cutoff at 30°, below which the detections are excluded from the right plots.

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