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作者:

Han, Ji (Han, Ji.) | Wang, Da-Yong (Wang, Da-Yong.) (学者:王大勇) | Liu, Han-Cheng (Liu, Han-Cheng.) | Fu, Xi-Yang (Fu, Xi-Yang.) | Guo, Hong-Feng (Guo, Hong-Feng.) | Tao, Shi-Quan (Tao, Shi-Quan.)

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摘要:

Optical sparse-aperture system can be designed to obtain high resolution in astronomical object imaging with several. Maximal and minimum fill factors of the sparse-aperture systems are presented, with the examples of annulus, Golay6 and tri-arm. A novel model named sparse-aperture multiple-array system is also proposed, and three kinds of configuration models have been illustrated. We compare the imaging performance of different multiple-array configurations by using the modulation transfer function (MTF). The results show that the variety of space between sub-aperture and the rotation of sub-array of multiple-array configurations have the effects on multiple-array MTF, and the multiple-array configurations have the advantages of firm configuration and easy fabrication.

关键词:

Imaging systems Optical transfer function

作者机构:

  • [ 1 ] [Han, Ji]College of Applied Sciences, Beijing University of Technology, Beijing 100022, China
  • [ 2 ] [Wang, Da-Yong]College of Applied Sciences, Beijing University of Technology, Beijing 100022, China
  • [ 3 ] [Liu, Han-Cheng]College of Applied Sciences, Beijing University of Technology, Beijing 100022, China
  • [ 4 ] [Fu, Xi-Yang]National Astronomical Observatories, Chinese Acad. of Sci., Beijing 100012, China
  • [ 5 ] [Guo, Hong-Feng]National Astronomical Observatories, Chinese Acad. of Sci., Beijing 100012, China
  • [ 6 ] [Tao, Shi-Quan]College of Applied Sciences, Beijing University of Technology, Beijing 100022, China

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来源 :

Journal of Optoelectronics Laser

ISSN: 1005-0086

年份: 2007

期: 6

卷: 18

页码: 649-652

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