Abstract Local acceleration driven by whistler-mode chorus waves is fundamentally important for accelerating seed electron populations to highly relativistic energies in the outer radiation belt. In this study, we quantitatively evaluate chorus-driven electron acceleration during the 17 March 2013 storm, when the Van Allen Probes observed very rapid electron acceleration up to several MeV within ~12 hours. A clear radial peak in electron phase space density (PSD) observed near L* ~4 indicates that an internal local acceleration process was operating. We construct the global distribution of chorus wave intensity from the low-altitude electron measurements made by multiple Polar Orbiting Environmental Satellites (POES) satellites over a broad...
We report the multi-satellite (LANL, GOES-10 and Cluster) observation data of electron flux evolutio...
We perform a superposed epoch analysis on two groups of selected geospace disturbance events, emergi...
Efforts to model and predict energetic electron fluxes in the radiation belts are highly sensitive t...
Abstract Local acceleration driven by whistler-mode chorus waves is fundamentally important for acce...
Abstract Recent analysis of satellite data obtained during the 9 October 2012 geomagnetic storm iden...
Outer zone radiation belt electrons can undergo gyroresonant interaction with various magnetospheric...
Abstract Local acceleration driven by whistler mode chorus waves largely accounts for the enhancemen...
Electron acceleration inside the Earth's magnetosphere is required to explain increases in the ∼MeV ...
Abstract The recent launching of Van Allen probes provides an unprecedent opportunity to investigate...
International audienceWe use plasma wave and electron data from the Combined Release and Radiation E...
International audience[1] The redistribution of energy during the recovery phase of geomagnetic stor...
Modeling and observations have shown that energy diffusion by chorus waves is an important source of...
Abstract We study the rapid outward extension of the electron radiation belt on a timescale of sever...
Whistler-mode chorus emissions are generated at the geomagnetic equator by injection of energetic el...
Abstract During 18 February to 2 March 2014, the Van Allen Probes encountered multiple geomagnetic s...
We report the multi-satellite (LANL, GOES-10 and Cluster) observation data of electron flux evolutio...
We perform a superposed epoch analysis on two groups of selected geospace disturbance events, emergi...
Efforts to model and predict energetic electron fluxes in the radiation belts are highly sensitive t...
Abstract Local acceleration driven by whistler-mode chorus waves is fundamentally important for acce...
Abstract Recent analysis of satellite data obtained during the 9 October 2012 geomagnetic storm iden...
Outer zone radiation belt electrons can undergo gyroresonant interaction with various magnetospheric...
Abstract Local acceleration driven by whistler mode chorus waves largely accounts for the enhancemen...
Electron acceleration inside the Earth's magnetosphere is required to explain increases in the ∼MeV ...
Abstract The recent launching of Van Allen probes provides an unprecedent opportunity to investigate...
International audienceWe use plasma wave and electron data from the Combined Release and Radiation E...
International audience[1] The redistribution of energy during the recovery phase of geomagnetic stor...
Modeling and observations have shown that energy diffusion by chorus waves is an important source of...
Abstract We study the rapid outward extension of the electron radiation belt on a timescale of sever...
Whistler-mode chorus emissions are generated at the geomagnetic equator by injection of energetic el...
Abstract During 18 February to 2 March 2014, the Van Allen Probes encountered multiple geomagnetic s...
We report the multi-satellite (LANL, GOES-10 and Cluster) observation data of electron flux evolutio...
We perform a superposed epoch analysis on two groups of selected geospace disturbance events, emergi...
Efforts to model and predict energetic electron fluxes in the radiation belts are highly sensitive t...