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

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Figure

Table 1. Standard deviations of the residuals to the fit to the data in nT.
Fig. 4. The first component of the XYZ (or equivalently α, β, γ ) Euler rotation angles calculated for CHAMP data for 2001 to 2004 (left part) and lateperiod 2008 and 2009 (right part)

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