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  4. Vol 3, Issue 1, 2022

Application of Wavefront Imaging Detection System in Astronomy

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DOI: 10.23977/infkm.2022.030106 | Downloads: 6 | Views: 685

Author(s)

Jiayan Yang 1

Affiliation(s)

1 School of Physics, Nankai University, Tianjin 300071, China

Corresponding Author

Jiayan Yang

ABSTRACT

Fast measurement of light source orientation is one of the research hotspots in the field of photoelectric tracking telemetry and command. In terms of the current light source detection technology, the multi-point detector layout is adopted, the intensity difference of incoming light is obtained by different detectors, then the direction of the light source is resolved. The technical route of wavefront imaging detection is studied from the perspective of practical application in this paper, and the calculation method of focal length, defocusing distance, and other parameters are provided, which provides a theoretical basis for the practical application and optical design of azimuth detection system based on wavefront imaging.

KEYWORDS

Wavefront Imaging, Defocusing Distance, Astronomy

CITE THIS PAPER

Jiayan Yang, Application of Wavefront Imaging Detection System in Astronomy. Information and Knowledge Management (2022) Vol. 3: 41-45. DOI: http://dx.doi.org/10.23977/infkm.2022.030106.

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