Fig. 39
From: Earth-affecting solar transients: a review of progresses in solar cycle 24
Predicted (non-black curves and shaded areas) and observed (black curves) CME magnetic field profiles at 1 AU from two different models. Panel (a): from Kay and Gopalswamy 2018; panel (b): from Scolini et al. 2019b. The predicted profiles consider uncertainties in input parameters. In both panels from top to bottom the magnetic field magnitude, and its Bx, By, and Bz components in the GSE system are plotted