Method for cleaning solar photosphere bright spot in astronomical image
A technology of astronomical images and sunlight, applied in instruments, character and pattern recognition, computer parts and other directions, can solve problems such as misrecognition
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Embodiment 1
[0024] Embodiment 1: as Figure 1-5 As shown, a method for cleaning the bright spots of the solar photosphere in astronomical images, first preprocesses the sequence images, and then uses a method combining Laplacian filtering and morphological dilation to identify the bright spots; and then through the three-dimensional connected The method tracks bright spots; then extracts multiple low-correlation eigenvalues of bright spots as cleaned data; then, performs z-score standardization on the cleaned data; then uses principal component analysis to convert high-dimensional standardized data Carry out dimensionality reduction; finally, the data after dimensionality reduction is cleaned by DBSCAN method, so as to eliminate non-bright spot structures.
[0025] The specific steps of the method for cleaning the bright spots of the solar photosphere in the astronomical image are as follows:
[0026] Step1. Bright spot data identification; first, preprocess the sequence image, includi...
Embodiment 2
[0033] Embodiment 2: as Figure 1-5 As shown, a method for cleaning the bright spots of the solar photosphere in astronomical images, first preprocesses the sequence images, and then uses a method combining Laplacian filtering and morphological dilation to identify the bright spots; and then through the three-dimensional connected The method tracks bright spots; then extracts multiple low-correlation eigenvalues of bright spots as cleaned data; then, performs z-score standardization on the cleaned data; then uses principal component analysis to convert high-dimensional standardized data Carry out dimensionality reduction; finally, the data after dimensionality reduction is cleaned by DBSCAN method, so as to eliminate non-bright spot structures.
[0034] The specific steps of the method for cleaning the bright spots of the solar photosphere in the astronomical image are as follows:
[0035] Step 1. Bright spot data identification; first, use the alignment method of maximum l...
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