title: Radiation belts of jupiter: a second look.
abstract: The outbound leg of the Pioneer 11 Jupiter flyby explored a region farther from the equator than that traversed by Pioneer 10, and the new data require modification or augmentation of the magnetodisk model based on the Pioneer 10 flyby. The inner moons of Jupiter are sinks of energetic particles and sometimes sources. A large spike of particles was found near lo. Multiple peaks occurred in the particle fluxes near closest approach to the planet; this structure may be accounted for by a complex magnetic field configuration. The decrease in proton flux observed near minimum altitude on the Pioneer 10 flyby appears attributable to particle absorption by Amalthea.
authors.forename: R W
authors.initials: RW
authors.lastname: Fillius
authors.forename: C E
authors.initials: CE
authors.lastname: McIlwain
authors.forename: A
authors.initials: A
authors.lastname: Mogro-Campero