Journal of Geophysical Research: Space Physics

The table shows the following, in columns from left to right: The date of each event, whether or not UVI is available, the IMF B y at onset, the dipole tilt

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

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

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

The closed field lines on the dayside get twisted by the combination of erosion of flux at high-latitude flanks and by the increase of magnetic pressure in the northern dawn and