Table 2 The first four columns show probabilities for each classification made for the presented events (Fig. 3) through a Gaussian process (GP) supervised machine learning model38

From: Revealing an unexpectedly low electron injection threshold via reinforced shock acceleration

 

Ejecta (EJ)

Coronal Hole (CH)

Sector Reversal (SR)

Sector Reversal (SR)

δB/B0

#1 seed

0.07

0.78

0.09

0.06

0.0596

#2 seed

0.10

0.40

0.15

0.23

0.0375

#3 seed

0.07

0.79

0.09

0.05

0.0420

#4 seed

0.13

0.39

0.12

0.37

0.0570

#5 seed

0.07

0.77

0.10

0.07

0.0779

#6 seed

0.06

0.79

0.09

0.06

0.1314

#1 no-seed

0.02

0.09

0.09

0.80

0.0145

#2 no-seed

0.35

0.18

0.05

0.42

0.0789

#3 no-seed

0.56

0.06

0.14

0.23

0.0209

#4 no-seed

0.13

0.12

0.31

0.44

0.0597

#5 no-seed

0.20

0.01

0.63

0.16

0.0493

#6 no-seed

0.25

0.05

0.24

0.46

0.0528

  1. The bold text indicates the most probable (i.e., dominant) class.
  2. Each cell indicates the probability in decimal number format. For this table, we used the OMNI 1 h dataset. The last column indicates wave amplitude with respect to the background magnetic field for each of the events shown in Fig. 3.
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