Add to ORKGRadial phase space density profiles for equatorially mirroring particles are computed from the data of the University of Iowa packages on Pioneer 10. The profiles are only consistent with radial diffusion subject to nonadiabatic losses. It is suggested that these losses are due to pitch angle scattering by whistler turbulence
For decades, ground-based radio observations of Jovian synchrotron radiation have shown emission ori...
Abstract: We present the temporal changes of the diffusion coefficient K of galactic cosmic rays (GC...
Radial diffusion coefficients quantify non-adiabatic transport of energetic particles by electromagn...
Radial phase space density profiles for equatorially mirroring particles are computed from the data ...
Radial diffusion of equatorially mirroring particles of solar wind origin in Jovian inner magnetosph...
WOS: A1992KC64900002Radial diffusion of equatorially mirroring particles of solar wind origin in Jov...
In the present investigation, radial diffusion of equatorially trapped electrons in the magnetospher...
The path-integrated gain of parallel propagating whistlers driven unstable by an anisotropic distrib...
Measurements of ≳1 MeV electrons in Neptune's magnetosphere from L ≈ 4 to 14 are well represented by...
The radial diffusion equation with synchrotron losses was solved by the Laplace transform method for...
Rich observational phenomenology associated with Pulsar B in PSR J0737$-$3039A/B system resembles in...
Flux maps of energetic ions in Jupiter's outer radiation belt, calculated with the aid of a model of...
Solutions are given for the diffusion of trapped particles in a planetary magnetic field in which th...
Using numerical solutions of single-particle dynamics, we consider a chaotic electron-whistler inter...
Context. Spacecraft observations have motivated the need for a refined description of the phase-spac...
For decades, ground-based radio observations of Jovian synchrotron radiation have shown emission ori...
Abstract: We present the temporal changes of the diffusion coefficient K of galactic cosmic rays (GC...
Radial diffusion coefficients quantify non-adiabatic transport of energetic particles by electromagn...
Radial phase space density profiles for equatorially mirroring particles are computed from the data ...
Radial diffusion of equatorially mirroring particles of solar wind origin in Jovian inner magnetosph...
WOS: A1992KC64900002Radial diffusion of equatorially mirroring particles of solar wind origin in Jov...
In the present investigation, radial diffusion of equatorially trapped electrons in the magnetospher...
The path-integrated gain of parallel propagating whistlers driven unstable by an anisotropic distrib...
Measurements of ≳1 MeV electrons in Neptune's magnetosphere from L ≈ 4 to 14 are well represented by...
The radial diffusion equation with synchrotron losses was solved by the Laplace transform method for...
Rich observational phenomenology associated with Pulsar B in PSR J0737$-$3039A/B system resembles in...
Flux maps of energetic ions in Jupiter's outer radiation belt, calculated with the aid of a model of...
Solutions are given for the diffusion of trapped particles in a planetary magnetic field in which th...
Using numerical solutions of single-particle dynamics, we consider a chaotic electron-whistler inter...
Context. Spacecraft observations have motivated the need for a refined description of the phase-spac...
For decades, ground-based radio observations of Jovian synchrotron radiation have shown emission ori...
Abstract: We present the temporal changes of the diffusion coefficient K of galactic cosmic rays (GC...
Radial diffusion coefficients quantify non-adiabatic transport of energetic particles by electromagn...