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Fig. 10 | Earth, Planets and Space

Fig. 10

From: Method for modeling of the components of ionospheric parameter time variations and detection of anomalies in the ionosphere

Fig. 10

Processing results of the geomagnetic and ionospheric data for 29 September–5 October 2013: a H-component of the Earth’s magnetic field, b assessment of the geomagnetic disturbance intensities, c identification of the periods of weak and strong geomagnetic disturbances, d identification of the periods of strong geomagnetic disturbances, e solar wind speed, f observed f o F2, g absolute smoothed component model errors, h absolute detailing component model errors, i estimation of the anomaly intensity, and j detected anomalies for a threshold coefficient U of 2.5 and a moving time window length Φ of 336 h. Graphs g and h show the standard deviations of the component model errors (dashed lines)

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