A method for detecting multiple concomitant phenomena of coronal mass ejections
A technology that accompanies phenomena and detection methods, applied in the field of solar physics, can solve the problems of not using phenomenon correlation, unable to detect multiple phenomena at the same time, etc., to achieve the effect of reducing the amount of calculation
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[0031] The specific implementation steps are as follows:
[0032] Step 1: Obtain n times of CME phenomena according to the event record catalog, and record the occurrence time period of each CME (t p,1 ,t p,2 ) and central position angle CPA p , where 1≤p≤n represents the pth CME; for each CME phenomenon, use steps 2 and 3 to extract the label Y p and the eigenvector x p .
[0033] Step 2: Take a certain time period t=(t p,1 ',t p,2 '),t p,1 ≤t p,1 'p,2 '≤t p,2 , record the occurrence of six accompanying phenomena (record Y={coronal dimming, coronal hole, coronal wave, dark streak eruption, flare, "S" shape}) in the catalog data during the time period t Will Y p as the tag set for this CME;
[0034] Step 3: Extract texture feature vector x for CME within t time period p ; According to catalog, randomly select k pieces of images I={I 1 , I 2 ,…I k}, for each image I q , 1≤q≤k Go to steps 3.1-3.3 to get 56×k-dimensional feature vector x p ;
[0035] Step 3.1: Ex...
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