Photospheric plasma and magnetic field dynamics during the formation of solar AR 11190

Free Access

Fig. A.3.

Open with DEXTER Download original image

Similar to Fig. 6, but for the quiet Sun region as outlined in Fig. A.1 and only showing the continuum proper motion case (due to quiet Sun conditions, not enough moving magnetic elements are available to obtain velocity distributions).

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.