Figure 13 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 13.

Distribution of the misfit (both innovations and residuals) with noise level of 10% rms in case 3. The distribution is fitted with a Gaussian (with least square fit, shown in black line), the corresponding average and standard deviation are listed in Table 2.

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