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Earth, Planets and Space
Fig. 8 | Earth, Planets and Space

Fig. 8

From: A secular variation candidate model for IGRF-13 based on Swarm data and ensemble inverse geodynamo modelling

Fig. 8

Huber weights attributed to IPGP’s candidate. Top left: their distribution for the three components of the secular variation taken together (note that the y-scale is logarithmic). Top right: their spatial distribution for the vertical component of the secular variation. Bottom left: same for the North–South component. Bottom right: same for the East–West component. Mollweide projection for the three components

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