Panels a)–c) show the temperature at τc = 0.95, 0.05 and 0.01, clipped at (5500, 6700), (4600, 5300), and (4300, 5200) K resp., for inversions made assuming depth-independent magnetic field and LOS velocity, and in panels d)−f) the corresponding temperatures obtained with 2 nodes for the velocity and 3 nodes for BLOS. Note the absence of inverse granulation in panel b). Panels g) and h) show the LOS velocity at τc = 0.95 and τc = 0.05 from the inversions corresponding to panels d)−f), and in panel i the LOS velocity from the inversions assuming constant LOS velocity (panels a)−c)). The LOS velocities have been clipped at (− 4.5, 4.5), (− 2.3, 2.3) and (− 2.3, 2.3) km s-1. The bottom row (panels j)−l)) show the LOS magnetic field (with 3 nodes for BLOS) at τc = 0.95, 0.05 and 0.01, clipped at (− 1000, 1500) G. Note the increasing area coverage (expansion with height) of the network field at smaller optical depths. The FOV shown is 25 × 18″.
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.