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Ørsted and Magsat scalar anomaly fields

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Figure

Fig. 1. The availability of Ørsted vector (MAG-L) data and scalar (OVH)data.
Fig. 2. Number of hits in each 1-degree by 1-degree bin, Ørsted nighttime vector data.
Fig. 4. Frequency distribution of the numerical difference between Ørstedtotal intensity values determined from vector (MAG-L) data and scalar(OVH) data.
Fig. 7. Typical output from the along-track, high-pass filter used for Ørsted OVH data
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