Interplanetary Coronal Mass Ejections Observed in the Heliosphere: 1. Review of Theory

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THE DEFLECTION OF THE TWO INTERACTING CORONAL MASS EJECTIONS OF 2010 MAY 23–24 AS REVEALED BY COMBINED IN SITU MEASUREMENTS AND HELIOSPHERIC IMAGING (2012, methodology): “This has been pointed out before, especially for fitting methods; both the HM and FΦ fitting tend to produce different directions and speeds, but similar arrival times (for example, see Howard & Tappin (2009), Möstl et al. (2011), Lugaz et al. (2012)).”
Coronal Mass Ejections: Observations (2012, background): “(1978) was the statistically significant temporal clustering of Culgoora type III radio bursts an average of 6 hours before Skylab CME onsets. Culgoora radioheliograph positional data revealed that these same type IIIs clustered spatially at the limb within 20° of the centroid of the CME. Recently, ”