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Table 3 Dimensional r.m.s. of the residuals to an AR-2 fit at several observatory sites

From: Geomagnetic observatory monthly series, 1930 to 2010: empirical analysis and unmodeled signal estimation

\(\sqrt {\eta }\)

(nT)

3.3

10.0

33.3

\(\sqrt {\eta }\)

(nT)

3.3

10.0

33.3

 

X

9.3

10.1

11.9

 

X

8.1

8.6

9.6

KAK

Y

2.5

2.9

4.3

HER

Y

1.8

2.6

4.5

 

Z

7.3

8.2

10.4

 

Z

3.2

3.4

6.6

 

X

8.1

8.4

9.1

 

X

13.7

14.3

15.0

ESK

Y

4.1

4.5

5.3

SIT

Y

6.1

6.4

7.4

 

Z

9.4

11.0

13.1

 

Z

13.5

14.9

16.4

 

X

11.0

12.5

15.2

 

X

10.6

11.2

12.7

ABG

Y

4.4

4.9

6.4

GUA

Y

1.9

2.2

3.5

 

Z

8.7

9.7

13.0

 

Z

3.4

4.3

8.4

  1. To the X, Y, and Z components (in nT), for several values η of the a priori noise variance.