Journal of Geophysical Research: Space Physics

For electric fields close to the electric field threshold ( < 500 kV/m) the LBE results show that 18% shorter avalanche regions than that in the case of LHEP are required for

The phase scintillation follows the intense poleward edge of the aurora as it expands northward (across the patch) and reaches values

Figure 2 shows a 20 ms window with reference time 25 October 2012 13:27:13.221 UT. The RHESSI counts are shown as blue dots with a logarithmic energy scale on the y axis. The

The phase scintillation follows the intense poleward edge of the aurora as it expands northward (across the patch) and reaches values

In this article, we introduced a new algorithm that automatically detects polar cap patches using the in situ plasma density measurements obtained by the Swarm satellites, which offer

We find that (1) the amplitude of high-frequency fluctuations in both R1 and R2 increases as the large-scale R1 and R2 FACs intensify; (2) high-frequency fluctuations in R1 peak

By sorting all measurements from DMSP and POES spacecraft overpasses in time, we generate MLT evo- lution of the precipitating electrons energy flux spectra.. We binned the energy

Following the above selection, the patch can easily be extracted as all pixels within the closed contour. Each contour is considered valid over the fluctuation. If we are not able