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.
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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.