Title of article :
Coded source imaging simulation with visible light
Author/Authors :
Wang، نويسنده , , Sheng and Zou، نويسنده , , Yubin and Zhang، نويسنده , , Xueshuang and Lu، نويسنده , , Yuanrong and Guo، نويسنده , , Zhiyu، نويسنده ,
Pages :
5
From page :
187
To page :
191
Abstract :
A coded source could increase the neutron flux with high L/D ratio. It may benefit a neutron imaging system with low yield neutron source. Visible light CSI experiments were carried out to test the physical design and reconstruction algorithm. We used a non-mosaic Modified Uniformly Redundant Array (MURA) mask to project the shadow of black/white samples on a screen. A cooled-CCD camera was used to record the image on the screen. Different mask sizes and amplification factors were tested. The correlation, Wiener filter deconvolution and Richardson–Lucy maximum likelihood iteration algorithm were employed to reconstruct the object imaging from the original projection. The results show that CSI can benefit the low flux neutron imaging with high background noise.
Keywords :
Reconstruction method , MURA mask , Coded source imaging , Neutron imaging , Visible light simulation
Journal title :
Astroparticle Physics
Record number :
2017314
Link To Document :
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