Figure 1 from ESTIMATING THE DEEP SOLAR MERIDIONAL CIRCULATION USING MAGNETIC OBSERVATIONS AND A DYNAMO MODEL: A VARIATIONAL APPROACH

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ESTIMATING THE DEEP SOLAR MERIDIONAL CIRCULATION USING MAGNETIC OBSERVATIONS AND A DYNAMO MODEL: A VARIATIONAL APPROACH

Authors: Ching Pui Hung, Laurène Jouve, Allan Sacha Brun, Alexandre Fournier, and Olivier Talagrand

2015 The Astrophysical Journal 814 151.

Provider: AAS Journals

Caption: Figure 1.

Stream functions for the three cases studied ((a)–(c) for cases 1–3, respectively). Case 1 is the unicellular model, case 2 is the four-cell model, and case 3 is the asymmetric model. We indicate the base of the convection zone at r = 0.7R_s with a broken line in each plot.

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