Add to ORKGThe radial diffusion equation with synchrotron losses was solved by the Laplace transform method for near-equatorially mirroring relativistic electrons. The evolution of a power law distribution function was found and the characteristics of synchrotron burn-off are stated in terms of explicit parameters for an arbitrary diffusion coefficient. Emissivity from the radiation belts of Jupiter was studied. Asymptotic forms for the distribution in the strong synchrotron loss regime are provided
Radial diffusion coefficients quantify non-adiabatic transport of energetic particles by electromagn...
For decades, ground-based radio observations of Jovian synchrotron radiation have shown emission ori...
The Voyager 2 cosmic ray experiment observed intense electron fluxes in the middle magnetosphere of ...
Radial phase space density profiles for equatorially mirroring particles are computed from the data ...
Solutions are given for the diffusion of trapped particles in a planetary magnetic field in which th...
The path-integrated gain of parallel propagating whistlers driven unstable by an anisotropic distrib...
In the present investigation, radial diffusion of equatorially trapped electrons in the magnetospher...
International audienceModeling the spatiotemporal evolution of relativistic electron fluxes trapped ...
A simplified model of the Jovian magnetosphere consists of a thermal plasma with superimposed radiat...
Measurements of ≳1 MeV electrons in Neptune's magnetosphere from L ≈ 4 to 14 are well represented by...
In this paper, we focus on the modeling of radial transport in the Earth's outer radiation belt. A h...
International audienceA time dependent radial diffusion model is used to quantify the competing effe...
Flux maps of energetic ions in Jupiter's outer radiation belt, calculated with the aid of a model of...
We report the first comprehensive observations of Jovian synchrotron radiation (JSR) and H3+ emissio...
A theory of the Io-independent decameter radiation is developed. The radiation results from excitati...
Radial diffusion coefficients quantify non-adiabatic transport of energetic particles by electromagn...
For decades, ground-based radio observations of Jovian synchrotron radiation have shown emission ori...
The Voyager 2 cosmic ray experiment observed intense electron fluxes in the middle magnetosphere of ...
Radial phase space density profiles for equatorially mirroring particles are computed from the data ...
Solutions are given for the diffusion of trapped particles in a planetary magnetic field in which th...
The path-integrated gain of parallel propagating whistlers driven unstable by an anisotropic distrib...
In the present investigation, radial diffusion of equatorially trapped electrons in the magnetospher...
International audienceModeling the spatiotemporal evolution of relativistic electron fluxes trapped ...
A simplified model of the Jovian magnetosphere consists of a thermal plasma with superimposed radiat...
Measurements of ≳1 MeV electrons in Neptune's magnetosphere from L ≈ 4 to 14 are well represented by...
In this paper, we focus on the modeling of radial transport in the Earth's outer radiation belt. A h...
International audienceA time dependent radial diffusion model is used to quantify the competing effe...
Flux maps of energetic ions in Jupiter's outer radiation belt, calculated with the aid of a model of...
We report the first comprehensive observations of Jovian synchrotron radiation (JSR) and H3+ emissio...
A theory of the Io-independent decameter radiation is developed. The radiation results from excitati...
Radial diffusion coefficients quantify non-adiabatic transport of energetic particles by electromagn...
For decades, ground-based radio observations of Jovian synchrotron radiation have shown emission ori...
The Voyager 2 cosmic ray experiment observed intense electron fluxes in the middle magnetosphere of ...