International audienceA time dependent radial diffusion model is used to quantify the competing effects of inward radial diffusion and losses on the distribution of the outer zone relativistic electrons. The rate of radial diffusion is parameterized by Kp with the loss time as an adjustable parameter. Comparison with HEEF data taken over 500 Combined Release and Radiation Effects Satellite (CRRES) orbits indicates that 1-MeV electron lifetimes near the peak of the outer zone are less than a day during the storm main phase and few days under less disturbed conditions. These values are comparable to independent estimates of the storm time loss rate due to scattering by EMIC waves and chorus emission, and also provide an acceptable representat...
Energetic electrons (≥50 keV) are injected into the slot region (2 < L < 4) between the inner and ou...
To advance our understanding of the magnetic storm dynamics of the outer radiation belt relativistic...
Radial diffusion is one of the dominant physical mechanisms driving acceleration and loss of radiati...
A time dependent radial diffusion model is used to quantify the competing effects of inward radial ...
Relativistic (>1 MeV) electron flux increases in the Earth's radiation belts are significantly under...
We simulate the behaviour of relativistic (976 keV) electrons in the outer radiation belt (3 ≤ L ≤ 7...
Many modern outer radiation belt models simulate the long‐time behavior of high‐energy electrons by ...
[1] Using recently published electron phase space densities (PSD) as a function of L * (L* is approx...
International audienceModeling the spatiotemporal evolution of relativistic electron fluxes trapped ...
In the Earth's radiation belts the flux of relativistic electrons is highly variable, sometimes chan...
Radiation belt dynamics have been modeled by the modified Fokker-Planck diffusion equation with sour...
The outer radiation belt is a region of space comprising highly energetic electrons. During periods...
International audienceData assimilation aims to smoothly blend incomplete and inaccurate observation...
[1] On the basis of the correlation between the solar wind and radiation belt electron fluxes, we de...
In this paper, we study electron radial diffusion coefficients derived from Pc4‐Pc5 ultralow frequen...
Energetic electrons (≥50 keV) are injected into the slot region (2 < L < 4) between the inner and ou...
To advance our understanding of the magnetic storm dynamics of the outer radiation belt relativistic...
Radial diffusion is one of the dominant physical mechanisms driving acceleration and loss of radiati...
A time dependent radial diffusion model is used to quantify the competing effects of inward radial ...
Relativistic (>1 MeV) electron flux increases in the Earth's radiation belts are significantly under...
We simulate the behaviour of relativistic (976 keV) electrons in the outer radiation belt (3 ≤ L ≤ 7...
Many modern outer radiation belt models simulate the long‐time behavior of high‐energy electrons by ...
[1] Using recently published electron phase space densities (PSD) as a function of L * (L* is approx...
International audienceModeling the spatiotemporal evolution of relativistic electron fluxes trapped ...
In the Earth's radiation belts the flux of relativistic electrons is highly variable, sometimes chan...
Radiation belt dynamics have been modeled by the modified Fokker-Planck diffusion equation with sour...
The outer radiation belt is a region of space comprising highly energetic electrons. During periods...
International audienceData assimilation aims to smoothly blend incomplete and inaccurate observation...
[1] On the basis of the correlation between the solar wind and radiation belt electron fluxes, we de...
In this paper, we study electron radial diffusion coefficients derived from Pc4‐Pc5 ultralow frequen...
Energetic electrons (≥50 keV) are injected into the slot region (2 < L < 4) between the inner and ou...
To advance our understanding of the magnetic storm dynamics of the outer radiation belt relativistic...
Radial diffusion is one of the dominant physical mechanisms driving acceleration and loss of radiati...