Fig. 6


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Comparison of the 5 days of recordings from UAH-MAG and SPT observatory during a geomagnetic event. From top to bottom: temperature recorded at a weather station (3170Y), the recorded raw data from the magnetometer sensor, magnetometer signal corrected for temperature and noise, data from SPT observatory and scatter plot of UAH-MAG vs. SPT data with the regression fitting line and parameters obtained.

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