Model calculations of Jupiter's electron and proton radiation belts indicate that the Galilean satellites can reduce particle fluxes in certain regions of the inner magnetosphere by as much as six orders of magnitude. Average fluxes should be reduced by a factor of 100 or more along the Pioneer 10 trajectory through the heart of Jupiter's radiation belts in early December. This may be enough to prevent serious radiation damage to the spacecraft
28 pages, 3 Tables, 11 FiguresExecutive Summary: Jupiter has the most energetic and complex radiatio...
Absorption effects of the four innermost moons in the radial transport equations for electrons and p...
A detailed account of the Pioneer 10 encounter with Jupiter is presented. Flux time histories of ele...
Solutions are given for the diffusion of trapped particles in a planetary magnetic field in which th...
The Pioneer 10 and Pioneer 11 space probes and their missions to Jupiter are discussed along with th...
Pioneer 10's encounter with Jupiter is discussed along with the interplanetary space beyond the orbi...
A simplified model of the Jovian magnetosphere consists of a thermal plasma with superimposed radiat...
The salient features of the various models of Jupiter's magnetosphere are compared with each other a...
An attempt is made to establish safety limits for space missions near Jovian radio belts. A proton b...
A model of Jupiter's magnetosphere in which there is a circum-Jovian outflow of plasma from an inner...
Pioneer 11, man's second spacecraft to Jupiter, is discussed. A description of the mission is given ...
During the inbound pass of Pioneer 10, a rapid ten-fold increase of the 0.2 to MeV proton flux was o...
Data derived from the plasma, magnetic field, and energetic particle experiments on the December, 19...
28 pages, 3 Tables, 11 FiguresExecutive Summary: Jupiter has the most energetic and complex radiatio...
28 pages, 3 Tables, 11 FiguresExecutive Summary: Jupiter has the most energetic and complex radiatio...
28 pages, 3 Tables, 11 FiguresExecutive Summary: Jupiter has the most energetic and complex radiatio...
Absorption effects of the four innermost moons in the radial transport equations for electrons and p...
A detailed account of the Pioneer 10 encounter with Jupiter is presented. Flux time histories of ele...
Solutions are given for the diffusion of trapped particles in a planetary magnetic field in which th...
The Pioneer 10 and Pioneer 11 space probes and their missions to Jupiter are discussed along with th...
Pioneer 10's encounter with Jupiter is discussed along with the interplanetary space beyond the orbi...
A simplified model of the Jovian magnetosphere consists of a thermal plasma with superimposed radiat...
The salient features of the various models of Jupiter's magnetosphere are compared with each other a...
An attempt is made to establish safety limits for space missions near Jovian radio belts. A proton b...
A model of Jupiter's magnetosphere in which there is a circum-Jovian outflow of plasma from an inner...
Pioneer 11, man's second spacecraft to Jupiter, is discussed. A description of the mission is given ...
During the inbound pass of Pioneer 10, a rapid ten-fold increase of the 0.2 to MeV proton flux was o...
Data derived from the plasma, magnetic field, and energetic particle experiments on the December, 19...
28 pages, 3 Tables, 11 FiguresExecutive Summary: Jupiter has the most energetic and complex radiatio...
28 pages, 3 Tables, 11 FiguresExecutive Summary: Jupiter has the most energetic and complex radiatio...
28 pages, 3 Tables, 11 FiguresExecutive Summary: Jupiter has the most energetic and complex radiatio...
Absorption effects of the four innermost moons in the radial transport equations for electrons and p...
A detailed account of the Pioneer 10 encounter with Jupiter is presented. Flux time histories of ele...