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

Open Access

Fig. 7.

Examples of distributions and fits in an alfvénic wind (14/07/2020): The Gaussian fit of the core (M_c) is shown in light blue, the NIG fits of the core (NigC) and beam (NigB) are in blue and their sum in green.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.