Fig. 3.

Download original image
Shown are COCONUT results for the March 9, 2016, solar eclipse (CR2174), with minimum-plasma-β constraining. The inner surface shows the prescribed magnetic field, the contour plot of the radial speed (demonstrating the existence of inexplicable high-speed streams and their removal thanks to the constraining), and the magnetic field lines over and around the active region, causing the high-speed streams plotted.
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.