Skewness and kurtosis of solar wind proton distribution functions: The normal inverse-Gaussian model and its implications

Open Access

Fig. 4.

Average distribution at 12:30 (same as in Fig. 3). The Gaussian fit of the core (M_c) and the NIG fit of the beam (NigB) are shown in blue. M_c + NigB, almost undiscernible from the measured distribution, is shown in green. The NIG fit of the whole distribution (NigT) is shown in red.

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