Image Details
Caption: Figure 2.
Focused object (a), original MHD simulation (b), restored objects using K = 2, 3, 5, 7, 9 ((c), (e), (g), (i), (k)), and residual of the restored object compared to the original MHD simulation ((d), (f), (h), (j), (l)). The focused and the restored scenes have been normalized to the average continuum intensity of the quiet Sun, I QS. Values in the frames correspond to the contrasts (left column) and rms of the residuals (right column).
© 2022. The Author(s). Published by the American Astronomical Society.