Fig. 5
Spectral index s of the modeled differential fluxes as a function of time after passage of the stream interface. Power-law indexes γs for the distribution correspond to γs = 2(s − 1). For example, a spectral index of s = −2 corresponds to a power-law index of γs = −6, which is close to the −5.4 power-law used for the common particle speed distribution.
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.