| Article ID | Journal | Published Year | Pages | File Type | 
|---|---|---|---|---|
| 1767548 | Advances in Space Research | 2009 | 5 Pages | 
Abstract
												In viewpoint of signal processing, we describe the principle of collimator-based Fourier-transform imaging, from verifying Fourier-transform function of collimator to presenting theoretical model of dirty image. This gives us a guideline in designing collimator imager, that is configuring the subcollimators properly to improve the quality of the dirty image. Here we optimize the arrangement of the subcollimators of YOHKOH Hard X-ray Telescope (HXT) to get the Point Spread Function of sidelobes as small as possible and simulate that with MATLAB.
											Keywords
												
											Related Topics
												
													Physical Sciences and Engineering
													Earth and Planetary Sciences
													Space and Planetary Science
												
											Authors
												Qiang Gu, Jin Chang, 
											