Indoor calibration method for star sensor interior orientation elements
A technology of inner orientation element and star sensor, which is applied in the field of aerospace measurement and can solve problems such as affecting the accuracy of star sensor parameters.
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[0121] In this section, the effectiveness of the method is verified through simulation and measured data. For an example of a specific implementation process, refer to the section "Specific Implementation Mode" above. In order to verify the generalization ability of the method, the data used for fitting (used to calculate internal parameters) and the data used for verification (used to calculate the angular spacing error between stars) do not overlap.
[0122] In the first test case, the basic parameters of the simulated star sensor are:
[0123] Field of view: Φ20°
[0124] Pixel array: 1536×1536
[0125] Principal point position: (758, 775)
[0126] Pixel size: 5.5um×5.5um
[0127] Focal length: 24.0955mm
[0128] Assuming that the centroid noise of the star point is Gaussian distribution noise with a mean value of zero and a standard deviation of 0.05 pixels, since the number of acquisitions at each data collection location is n=10, the noise level decreases after aver...
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