Abstract
Table 2 Correlation coefficients of GLE peaks and overall CRI of each GLE with simultaneous geomagnetic indices (SymH), interplanetary magnetic field (IMF-Btot), solar wind plasma velocity (Vsw), X-ray flux, and different energy channels of SEP fluxes. The correlations of GLE peaks (n = 6) with simultaneous solar, interplanetary and geophysical factors are examined. The data points (n = 6) of the GLE peak are taken for the rising part (n = 3) before peak point, peak point (n = 1) and descending after peak point (n = 2). The whole window of GLE event is taken as 24 hours that counted data number as n = 24 × 12 = 288 for 5-minute resolution. The correlations of the overall CRI of the selected GLE events are examined for the whole time window (n = 288)
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