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Fig. 3 | Earth, Planets and Space

Fig. 3

From: Magnetic field stretching at the top of the shell of numerical dynamos

Fig. 3

As in Fig. 2 for another intense high-latitude normal polarity magnetic flux patch (HN) in dynamo model 4 (lower polygon in Fig. 1a). The statistics for this patch are: St/Ad = 1.23; \({\mathcal {P}}/{\mathcal {T}}=0.28\); \(H_u=0.97\); \({\text {corr}}(|B_r|,\delta _h^-)=0.74\); \({\text {corr}}(|B_r|,\delta _h^+)=-0.47\); \(\xi _{\text {a}}=0.67\); \(\xi _{\text {s}}=0.68\); \(\xi _{\text {e}}=0.87\)

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