The role of injection and fast radial diffusion during disturbed magnetospheric conditions in creating the energetic electron population of the inner zone is discussed. The great magnetic storm of February 1986 provides an example of these dramatic processes : energetic electrons were injected and rapidly diffused into the magnetosphere; the old inner zone electron population was depleted; and a new inner zone electron population was created. These injection and rapid diffusion processes also provide a possible explanation for the large flux of high energy (similar to several tens MeV) electrons observed in the inner zone. Such electrons cannot be explained by slow magnetic radial diffusion (D-o = 10(-13) s(-1)) because of synchrotron energ...
We have quantitatively investigated the radiation belt's dynamic variations of 1.5-6.0 MeV elec...
Radiation belt dynamics have been modeled by the modified Fokker-Planck diffusion equation with sour...
Substorms generally inject tens to hundreds of keV electrons, but intense substorm electric fields h...
A large flux of > 100 MeV electrons were registered in the inner radiation belt on low-altitude sate...
A large flux of > 100 MeV electrons were registered in the inner radiation belt on low-altitude s...
Our society increasingly relies on spacecraft operations in the Earth's inner magnetosphere, particu...
International audienceModeling the spatiotemporal evolution of relativistic electron fluxes trapped ...
During moderate magnetic storms, an electron channel (300–1100 keV) of the NOAA satellite has...
Understanding the formation of the seed population for the energetic electrons trapped within the Ea...
The paper discusses the outer electron belt dynamics, adiabatic and nonadiabatic mechanisms of incre...
It is shown that narrow channels of high electric field are an effective mechanism for injecting pl...
Major magnetic storm produces a big change in relativistic (> a few hundred keV) electron flux in...
Energetic electron intensities radial flow diffusion in outer radiation belt near geomagnetic equato
Energetic electrons (≥50 keV) are injected into the slot region (2 < L < 4) between the inner and ou...
[1] Using recently published electron phase space densities (PSD) as a function of L * (L* is approx...
We have quantitatively investigated the radiation belt's dynamic variations of 1.5-6.0 MeV elec...
Radiation belt dynamics have been modeled by the modified Fokker-Planck diffusion equation with sour...
Substorms generally inject tens to hundreds of keV electrons, but intense substorm electric fields h...
A large flux of > 100 MeV electrons were registered in the inner radiation belt on low-altitude sate...
A large flux of > 100 MeV electrons were registered in the inner radiation belt on low-altitude s...
Our society increasingly relies on spacecraft operations in the Earth's inner magnetosphere, particu...
International audienceModeling the spatiotemporal evolution of relativistic electron fluxes trapped ...
During moderate magnetic storms, an electron channel (300–1100 keV) of the NOAA satellite has...
Understanding the formation of the seed population for the energetic electrons trapped within the Ea...
The paper discusses the outer electron belt dynamics, adiabatic and nonadiabatic mechanisms of incre...
It is shown that narrow channels of high electric field are an effective mechanism for injecting pl...
Major magnetic storm produces a big change in relativistic (> a few hundred keV) electron flux in...
Energetic electron intensities radial flow diffusion in outer radiation belt near geomagnetic equato
Energetic electrons (≥50 keV) are injected into the slot region (2 < L < 4) between the inner and ou...
[1] Using recently published electron phase space densities (PSD) as a function of L * (L* is approx...
We have quantitatively investigated the radiation belt's dynamic variations of 1.5-6.0 MeV elec...
Radiation belt dynamics have been modeled by the modified Fokker-Planck diffusion equation with sour...
Substorms generally inject tens to hundreds of keV electrons, but intense substorm electric fields h...