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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 5.

Vector potential of the poloidal field at a given location as a function of time for case 3 (asymmetric meridional circulation). Shown are the time series of the reference (dashed orange line), the initial guess before assimilation (in green), the final estimate after assimilation (in blue), and the synthetic observations made at that location (red crosses).

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