Correction to 'Radiation belt electron precipitation by man-made VLF transmissions'

during burst operation mode in the orbit 18910_0 on February 11, 2008, between 2021 UT and 2026 UT: magnetic (first panel) and electric (second panel) field power spectra and polar

Thus, this simulation shows that electrons which were accelerated to ∼1 keV in the parallel electric field of TDS, can be further accelerated to relativistic energies in a small

Effects of plasma density irregularities on the pitch angle scattering of radiation belt electrons by signals from ground based

[ 1 ] We calculated the bounce averaged electron pitch angle diffusion coefficients 〈D a eq a eq 〉 using the statistical characteristics of lower band chorus activity collected by

Satellite Observations of the Radiation Belts [ 10 ] The geomagnetic storm of 11 September 2005 led to an increase in the energetic electron population in the inner edge of the

L’archive ouverte pluridisciplinaire HAL, est destinée au dépôt et à la diffusion de documents scientifiques de niveau recherche, publiés ou non, émanant des

[ 35 ] The detection of consecutive bursts of near loss cone energetic electron flux which correlate with NPM trans- missions suggest that NPM induced significant precipitation at

This study shows that the measured electron bursts show- ing a wisp structure are not associated with earthquakes, but with cyclotron resonance of electrons with monochromatic