Radial 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
Model calculations of Jupiter's electron and proton radiation belts indicate that the Galilean satel...
The intense inner radiation belt at Jupiter (>50 MeV at 1.5 RJ) is generally accepted to be created ...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95607/1/jgre2060.pd
Radial phase space density profiles for equatorially mirroring particles are computed from the data ...
The radial diffusion equation with synchrotron losses was solved by the Laplace transform method for...
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...
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...
Absorption effects of the four innermost moons in the radial transport equations for electrons and p...
In the present investigation, radial diffusion of equatorially trapped electrons in the magnetospher...
The role of plasma waves in shaping the intense Jovian radiation belts is not well understood. In th...
The Voyager 2 cosmic ray experiment observed intense electron fluxes in the middle magnetosphere of ...
Flux maps of energetic ions in Jupiter's outer radiation belt, calculated with the aid of a model of...
Measurements of ≳1 MeV electrons in Neptune's magnetosphere from L ≈ 4 to 14 are well represented by...
Model calculations of Jupiter's electron and proton radiation belts indicate that the Galilean satel...
The intense inner radiation belt at Jupiter (>50 MeV at 1.5 RJ) is generally accepted to be created ...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95607/1/jgre2060.pd
Radial phase space density profiles for equatorially mirroring particles are computed from the data ...
The radial diffusion equation with synchrotron losses was solved by the Laplace transform method for...
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...
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...
Absorption effects of the four innermost moons in the radial transport equations for electrons and p...
In the present investigation, radial diffusion of equatorially trapped electrons in the magnetospher...
The role of plasma waves in shaping the intense Jovian radiation belts is not well understood. In th...
The Voyager 2 cosmic ray experiment observed intense electron fluxes in the middle magnetosphere of ...
Flux maps of energetic ions in Jupiter's outer radiation belt, calculated with the aid of a model of...
Measurements of ≳1 MeV electrons in Neptune's magnetosphere from L ≈ 4 to 14 are well represented by...
Model calculations of Jupiter's electron and proton radiation belts indicate that the Galilean satel...
The intense inner radiation belt at Jupiter (>50 MeV at 1.5 RJ) is generally accepted to be created ...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95607/1/jgre2060.pd
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