On fast and slow Earth’s magnetospheric dynamics during geomagnetic storms: a stochastic Langevin approach | Journal of Space Weather and Space Climate

System Science: Application to Space Weather Analysis, Modelling, and Forecasting

Open Access

Fig. 5.

Marginal Hilbert power spectral density for the three different selected periods: period A (black dots), period B (red dots), and period C (green dots), respectively. The black dashed line is used as a reference to the spectral slopes.

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