X-ray pulsar recognition method based on Hilbert transformation
An identification method and X-ray technology, applied in astronomical navigation and other directions, can solve problems such as a large amount of computing time and storage space, and achieve the effect of less computing space and storage space, effective identification effect, and suppression of high-frequency noise.
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[0020] The specific implementation of the present invention will be described below in conjunction with the embodiments and the drawings.
[0021] Implementation step 1: First, the standard profile data of 11 observed X-ray pulsars provided by EPN are included in the navigation database. Therefore, the set of observed X-ray pulsars is: {B1257+12, B1953+29, J0621+1002, J1012+5307, J1518+4904, J1640+2224, J1643-1224, J1713+0747, J1730-2304, J1744- 24A, J2051-0827}, the samples of this set are classified into classes numbered {1,...,11}.
[0022] Step 2: Extract the instantaneous amplitude feature vector of the observed contour signal, use the minimum distance classifier to calculate the distance between it and each standard contour feature vector, and obtain a set of identification space distances.
[0023] Perform step 3: Select the X-ray pulsar sequence number corresponding to the smallest value in the set as the identification result.
[0024] Table 1 The calculation results of the ...
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