Recently, investigating the behavior of some geomagnetic indices (AE indices, SYM-H and ASY-H), the Perreault-Akasofu coupling function and the Bz component of the interplanetary magnetic field, it has been displayed (Alberti et al., 2017) that the magnetic time series, associated with the geomagnetic indices, are characterized by fluctuations which present a different amount of shared information (which
AbstractWe analyze the geomagnetic data recorded at 78 stations from 13 to 31 March 2015. Using the empirical mode decomposition (EMD) method, we focus our attention on geomagnetic signal due to sources which are external to the Earth, that is, due to current systems flowing in the ionosphere and magnetosphere. We analyze the short timescale fluctuations (τ < 200 min) of this magnetic signal, their dependence on magnetic latitude, magnetic local time, and geomagnetic activity. At high geomagnetic latitudes (>|60°|), these short timescale fluctuations constitute more than 30% of the external magnetic field. Their maximum contribution occurs along the auroral oval suggesting that they are mainly triggered by the ionospheric electric current systems active in these regions. A discussion of the relevance of these short timescale magnetic fluctuations to result in a more significant modeling and prediction of geomagnetically induced currents in the auroral zones is also provided. SANTARELLI ET AL.