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This is no doubt due to polar gaps in the Swarm orbital coverage.
Discontinuities caused by the polar gaps introduce ringing when local functions are used.
The power spectra and the correlation analysis are presented with the lithospheric field model estimated prior and after the implementation of the post-processing in the polar gaps.
As can be seen most of the errors are found near the polar gaps and at the mid to high-latitude transitions.
The process stops when the spatial resolution of the model over the polar gaps reaches the same resolution as in other regions.
This problem is addressed using a post-processing based on an iterative regional modelling of the vector values computed on the Gauss-Legendre grid above the two polar gaps.
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For example, depending on the cohesive energy of the surface matter, an acceleration zone ("polar gap") above the polar cap of a pulsar may or may not form.
A polar gap at the postoperative radiograph was noted at 25% of the arthroplasties, most of which subsequently filled with bone within 6 months.
Left: power spectrum of the 'true' model (black), the estimated model without polar gap treatment (red), and the estimated model with the polar gap processing (blue).
The Swarm orbital configuration tested in this study has a polar gap of about 5.2°.
Sensitivity matrix between the 'true' model and the model estimated after a polar gap processing.
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