Research Article
A Real-Time Star Tailing Removal Method Based on Fast Blur Kernel Estimations
Algorithm 1
Angle estimation based on PCA.
| Input: the star image (x, y) | | (1) | Compute the bispectrum transformation of (x, y), | | (2) | Apply Gauss high pass filtering on , and obtain | | (3) | Perform threshold segmentation on , and obtain the position matrix of bright region pixels P | | (4) | Compute the mean of P, µ | | (5) | Compute the covariance matrix C ← | | (6) | Compute the maximum eigenvalue , and its eigenvector | | (7) | | | Output: |
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