Priorité des Opérations sur les Fractions Positives et à Trois Étapes (A)

Applying criteria 1 and 2, we count the magnetopause crossings with electron heat flux. Thereby, we do not dis- tinguish whether the heat flux is due to a streaming of ring

Variable Estimates Std. The remaining 55 events were divided into two sets, namely, a training set and a validation set. The training dataset, comprising of 46 events, which included

The results for 1.6±48 MeV protons show that, compared to a much more intensive and faster CME during the previous solar maximum (the event on October 19, 1989), the injection rate

The observed decrease of the nighttime NmF2 peak amplitude withsolar activity is due to faster increasing of the recombination eciency compared to the plasmaspheric ¯ux increase..

Using the method of characteristics to invert ground-based data of the ground magnetic ®eld distur- bance and of the ionospheric electric ®eld, we obtain spatial distributions

Figure 8 shows these amplitudes as func- tions of month and height, with a set of three panels (the two wind components and the energy dissipation rate) for each of the four

Assuming a wave source at the auroral electrojet height of ∼125 km, and wave ascent an- gles consistent with the properties of gravity waves, we find source locations for the

Accordingly, the proposed research ®rstly derives and models a stable surrogate pattern for the long-term solar activity, secondly introduces a transfer-function algorithm for