Table 2 Pairwise MFD comparison of temporal subsets

From: Revealing the spatiotemporal complexity of the magnitude distribution and b-value during an earthquake sequence

 

Cluster 1

Cluster 2

Cluster 3

 

(pre-V.)

(pre-N.)

(pre-C.)

(pre-V.)

(pre-N.)

(pre-C.)

(pre-V.)

(pre-N.)

(pre-C.)

C1 (pre-Visso)

 

0.0037

0.33

0.59

0.74

0.03

2.1e-05

0.86

0.79

C1 (pre-Norcia)

0.0037

 

0.23

0.01

0.72

0.044

1.3e-09

0.0056

0.052

C1 (pre-Campotosto)

0.33

0.23

 

0.52

0.42

0.21

5.8e-06

0.62

0.013

C2 (pre-Visso)

0.59

0.01

0.52

 

0.78

0.28

2.5e-06

0.51

0.068

C2 (pre-Norcia)

0.74

0.72

0.42

0.79

 

0.51

0.093

0.42

0.26

C2 (pre-Campotosto)

0.03

0.044

0.21

0.28

0.5

 

7.6e-08

0.0087

0.018

C3 (pre-Visso)

2.1e-05

1.3e-09

5.8e-06

2.5e-06

0.093

7.6e-08

 

3.2e-06

0.012

C3 (pre-Norcia)

0.86

0.0056

0.62

0.51

0.42

0.0087

3.2e-06

 

0.099

C3 (pre-Campotosto)

0.79

0.052

0.013

0.068

0.26

0.018

0.012

0.099

 
  1. Statistically significant p-values are highlighted in bold.
  2. Like Table 1, but for three periods of Cluster 1, 2, and 3 that exclude short-term incompleteness (STAI).
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