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Table 1. Standard deviations of the residuals to the fit to the data in nT.

From: An algorithm for deriving core magnetic field models from the Swarm data set

Satellite ABC A B C
Type     
X (SM) 2.76 2.73 2.72 2.84
Y (SM) 2.93 2.87 2.87 3.06
X (HL) 7.51 7.67 7.67 7.16
Y (HL) 6.05 6.18 6.21 5.72
Z (HL) 6.23 6.35 6.38 5.91