a solar image registration method based on normalized cross-correlation and SIFT
An image registration and cross-correlation matching technology, applied in the fields of astronomy and image processing, to achieve the effects of high accuracy, reduced time overhead, and improved algorithm efficiency
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[0065] Embodiment 1: as Figure 1-10 As shown, in order to prove the universality of this method, four different images are selected for comparison and description in this embodiment.
[0066] A solar image registration method based on normalized cross-correlation and SIFT, comprising the steps of:
[0067] Step 1: Input two solar observation images, one of which is a full-helioscopic observation image from SDO (such as figure 2 shown) as a reference image I 1 , and the other is a local high-resolution observation image of the Sun from NVST (such as image 3 shown), as a floating image I 2 , to preprocess the two images respectively, first down-sampling the two images, the SDO full-day image is reduced by 0.5 times, and the NVST local high-resolution image is reduced by 0.1 times. Using the Rayleigh distribution, the enhancement factor is 0.2 for the two images I 1 , I 2 Performs limited contrast histogram equalization enhancement.
[0068] Step 2: Use the normalized c...
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