A Real-Time Star Tailing Removal Method Based on Fast Blur Kernel Estimations

Figure 11

The reconstruction of simulated star with noise (SNR = −3.2 dB, PSNR = 119.2794, RMSE = 0.0166, L = 20, and angle = 20°): (a) degenerated star points, (b) traditional method, (c) method proposed by Jiang [30], and (d) the proposed method.

(a)

(b)

(c)

(d)