The magnetic ejecta of two interplanetary CMEs remain near-isothermal (Gamma_eff = 0.88 and 0.76) at 1 AU, with Kolmogorov-like turbulence in the fast event and shallower, less developed turbulence in the slow event.
@doi [Space Weather] 10.1029/2009SW000465, https://ui.adsabs.harvard.edu/abs/2009SpWea...7.2003B 7
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Thermal and Turbulence Characteristics of Fast and Slow Coronal Mass Ejections at 1 AU
The magnetic ejecta of two interplanetary CMEs remain near-isothermal (Gamma_eff = 0.88 and 0.76) at 1 AU, with Kolmogorov-like turbulence in the fast event and shallower, less developed turbulence in the slow event.