Figure 3 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 3.

Typical synthetic data generated in case 3, here we show the surface vector potential of the poloidal field at a fixed latitudinal location as a function of time.

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