Fig. 9.
Download original image
ρ 1 histograms of complex (βγ and βγδ) and simple (α and β) regions within the sunspots (a) and the magnetic fragments (b). The simple ARs are generally more correlated within the sunspots but less correlated within the magnetic fragments. The difference between the sunspot distributions, as measured by the Hellinger distance, is statistically significant.
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.