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Table 3 The identified epochs of rapid SV fluctuations at 2 selected points (at 400 km altitude just above HER and TSU) using the polynomial monthly main field models.

From: Polynomial modelling of CHAMP satellite data to investigate rapid secular variation fluctuations over southern Africa during 2003 and 2004

  

Gradient before [nT/yr2]

Epoch of rapid SV fluctuation

Gradient between the epochs [nT/yr2]

Epoch of rapid SV fluctuation

Gradient after [nT/yr2]

 

X

−5.8

2003.1

14.0

2004.1

−9.9

HER

Y

2.0

2003.4

−4.7

2004.1

1.2

 

Z

−12.2

2003.0

8.4

2004.1

−10.4

 

X

−8.6

2003.1

18.4

2004.1

−9.2

TSU

Y

3 0

2003.2

−4.0

2004.3

1.9

 

Z

−7.0

2002.9

3.7

2004.0

−9.4