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Fig. 5 | Earth, Planets and Space

Fig. 5

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

Fig. 5

As in Fig. 2 for an intense high-latitude normal polarity flux patch (HN) in dynamo model 6 (lower polygon in Fig. 4a). The statistics for this patch are: St/Ad = 0.87; \({\mathcal {P}}/{\mathcal {T}}=0.27\); \(H_u=0.95\); \({\text {corr}}(|B_r|,\delta _h^-)=0.58\); \({\text {corr}}(|B_r|,\delta _h^+)=-0.28\); \(\xi _{\text {a}}=0.61\); \(\xi _{\text {s}}=0.88\); \(\xi _{\text {e}}=0.98\)

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