TY - JOUR
T1 - Parameter estimation of Gaussian gray diffusion model of static image spot
AU - Wang, Haiyong
AU - Zhou, Wenrui
AU - Lin, Haoyu
AU - Wang, Xinlong
PY - 2012/3
Y1 - 2012/3
N2 - In order to estimate the parameters in Gaussian gray diffusion model, experiments with collimator are carried out while the parameter calibration algorithm is proposed. Equations which take the Gaussian diffusion radius and the deviation values of the centroid coordinate as variables are established and solved, furthermore, the energy-gray coefficient is obtained. Then, series of photos are taken under the same condition in three different orientations, and parameters whose mean values are taken as their estimates are calculated respectively using these gray data of photos. Finally, all the estimated parameters are put into the simulating model, and a model-generated star image spot is therefore got, the similarity between which and real shot ones is calculated in three different windows under the condition that noise is bound to exist. The similarity is a value of more than 0.97 within the window of 3 pixel×3 pixel, more than 0.98 for a 5 pixel×5 pixel, and more than 0.98 for a 7 pixel×7 pixel. The experimental results show that the solution formulas about σ, A and the deviation Δx and Δy are right.
AB - In order to estimate the parameters in Gaussian gray diffusion model, experiments with collimator are carried out while the parameter calibration algorithm is proposed. Equations which take the Gaussian diffusion radius and the deviation values of the centroid coordinate as variables are established and solved, furthermore, the energy-gray coefficient is obtained. Then, series of photos are taken under the same condition in three different orientations, and parameters whose mean values are taken as their estimates are calculated respectively using these gray data of photos. Finally, all the estimated parameters are put into the simulating model, and a model-generated star image spot is therefore got, the similarity between which and real shot ones is calculated in three different windows under the condition that noise is bound to exist. The similarity is a value of more than 0.97 within the window of 3 pixel×3 pixel, more than 0.98 for a 5 pixel×5 pixel, and more than 0.98 for a 7 pixel×7 pixel. The experimental results show that the solution formulas about σ, A and the deviation Δx and Δy are right.
KW - Gray proliferation
KW - Image processing
KW - Navigation technique
KW - Parameter estimation
KW - Star-image simulation
UR - https://www.scopus.com/pages/publications/84859397957
U2 - 10.3788/AOS201232.0323004
DO - 10.3788/AOS201232.0323004
M3 - 文章
AN - SCOPUS:84859397957
SN - 0253-2239
VL - 32
JO - Guangxue Xuebao/Acta Optica Sinica
JF - Guangxue Xuebao/Acta Optica Sinica
IS - 3
M1 - 0323004
ER -