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We also report clear evidence for the occurrence of resonant coupling (at f ≈ 2.2 and 3.2 mHz) between such modes and high latitude field lines.
The local time and latitudinal dependence of the observed pattern can be tentatively interpreted in terms of a latitude of resonant field lines reaching λ ∼ 80° in the noon sector; on the other hand, resonance effects of lower latitude field lines can be clearly identified also far from the noon meridian when the station moves into the deep polar cap.
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The time change of the sectorial coefficients which represent low-latitude field changes, are better resolved, as indicated by the lower scatter.
The flux patches in this case sample the high-latitude field lobes of main field models, and represent the fine structure of the lobes.
A case study for southward IMF conditions agrees with a model in which the mantle is populated via entry along open high-latitude field lines.
The violation takes place at the separatrix dividing a region of transequatorial bounce oscillations from that of oscillations about high-latitude field minima.
Despite uncertainties in understanding the excitation of FLRs throughout the magnetosphere, they can be used to estimate the equatorial mass density on high latitudes field lines.
The mid-latitude field-aligned irregularity (FAI) along the magnetic field line is a common phenomenon in the ionosphere.
For the first time we propose a method for detecting the mid-latitude field-aligned disturbances (FADs) prolated on the magnetic field.
Results show, on one side, the existence of a relation between the analysed residuals and IMF components B y and B z, possibly due to the long distance effect of high-latitude field-aligned currents.
First, we take the electrostatic potential arising from the interaction of the solar wind with the Earth's magnetosphere derived from an experimental data-based model of the high-latitude field-aligned currents.
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