Figure 12 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 12.

Objective function (left) and Δp/p (right) as the minimization evolves, with the reference sampling, at different noise levels. Note that in case 1 when the noise increases, the curves of objective function and Δp/p start to level off at higher values.

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