Low- and mid-latitude residuals of the geomagnetic field representing the ionospheric and the unmodelled magnetospheric contributions are investigated, in the Solar Magnetic frame, according to the polarity of IMF B y (azimuthal) and B z (north south) components and to different geomagnetic activity levels.
All stimulus periods lasted 3 min and were presented on a single Peltier element (6 x 9 cm) covered with a piece of standard white letter size printer paper (extra bright, Navigator; Office Depot/Office Max, Cleveland, OH) cut to 15 × 17 cm and held taut by a magnetic frame.
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The field is decomposed into contributions from sources in the solar-magnetic frame, and those in the geocentric-solar-magnetospheric frame.
The precipitating electron fluxes and distribution of the field-aligned currents in the first- and second high-latitude region are specified in the solar-magnetic frame.
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In a local magnetic field frame the oscillations were transversal and mainly in the west-east direction.
Also shown in parenthesis are the metrics calculated for the and coefficients in the Solar Magnetic (SM) frame.
This controversy has brought us to study the features of residuals in the Solar Magnetic (SM) frame when Swarm data are used.
Also shown in Table 3 are the metrics for one order zero and one order one coefficient given in the Solar Magnetic (SM) frame (Section 2.9), defined using IGRF-11 at the model dates, which are indicative of the quality of the other degree 1 coefficients.
