A Method for Correcting Misalignment Errors of Large Aperture and Large Field of View Telescopes
An error correction and telescope technology, which is applied in the field of integrated adjustment of telescope systems, can solve problems such as cumbersome implementation process, complex calculation process, and complex algorithm, and achieve the effects of wide application range, simplified measurement system, and reduced algorithm complexity
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[0037] The RC optical system with a clear aperture of 4m and F#=3 is used for simulation analysis. The system parameters are shown in Table 1. The selected field of view is shown in Table 1. figure 2 shown.
[0038] Table 1 Some parameters of the telescope system
[0039] System parameters Radius Semi-diameter Conic PM -12000 2000 -1.004 SM -2125 330 -1.626
[0040] Taking the central wavelength as 0.55μm, the full width at half maximum of the Airy disk corresponding to the optical system is:
[0041]
[0042] Assuming that the selected detector pixel size is 15μm, take the undersampling factor Q:
[0043]
[0044] It can be seen from the above results that the under-sampling magnification of the under-sampling image obtained by the optical system on the detector is a serious under-sampling image because Q=18. The undersampled imaging spot shape in the ideal imaging state of the optical system is as follows: image 3shown. For la...
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