Regulation of temperature anisotropy for solar wind protons and alpha particles by collisions and instabilities

Open Access

Fig. 6.

Combined results of combined dynamical ensemble calculation where the final states, plotted with black dots, are displayed against a background showing the 2D solar wind alpha particle and proton occurrence distributions. The final states are the same as those shown in Figures 3 and 5.

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.