The solar wind is a highly turbulent medium exhibiting scalings of the fluctuations ranging
over several decades of scales from the correlation length down to proton and electron …

A generalization of the traditional 12‐station auroral electrojet (AE) index to include more
than 100 magnetometer stations, SME, is an excellent predictor of global auroral power …

We present a new quantitative technique that determines the times and durations of
substorm expansion and recovery phases and possible growth phases based on percentiles …

On 25 August 2018 the interplanetary counterpart of the 20 August 2018 coronal mass
ejection (CME) hit Earth, giving rise to a strong G3 geomagnetic storm. We present a …

Magnetospheric substorms represent the primary mode of energy circulation and topological
reconfiguration of the plasma environment in the Earth's vicinity. They occur when there is …

The probability distribution functions (PDFs) of the differences of any physical variable in the
intermittent, turbulent interplanetary medium are scale dependent. Strong non-Gaussianity …

The rapid changes of magnetic fields associated with large, isolated magnetic perturbations
with amplitudes| ΔB| of hundreds of nanotesla and 5‐to 10‐min periods can induce bursts of …

На основе данных за 2015 г. магнитных обсерваторий сети IMAGE и станции по
регистрации геоиндуцированных токов (ГИТ) в линии электропередачи исследуются …

Using observations from the IMAGE magnetic observatories and the station for recording
geomagnetically induced currents (GIC) in the electric transmission line in 2015, we …

Most substorm researchers assume substorms to be caused by a unique large-scale
process. However, a critical evaluation of substorm observations indicates that a new …