Figure 14 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 14.

Same as Figure 13, for a latitudinal sampling restricted to the activity band only and a noise level of ϵ = 1%. Note that the distribution of residuals slightly deviates from a Gaussian distribution.

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