Figure 10 from On the Anisotropy in Expansion of Magnetic Flux Tubes in the Solar Corona

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On the Anisotropy in Expansion of Magnetic Flux Tubes in the Solar Corona

Authors: A. Malanushenko and C. J. Schrijver

Malanushenko & Schrijver 2013 The Astrophysical Journal 775 120.

Provider: AAS Journals

Caption: Figure 10.

Value of a _apx/ b _apx does not appear to be strongly correlated with the inclination of the field at the base of the flux tube. Spearman's correlation coefficient is ρ = −0.14.

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