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IEEE Aerospace Conference, 2022
The experiment for space radiation analysis is an upcoming project for Los Alamos National Laboratory. This 12U CubeSat will be placed in a geosynchronous transfer orbit to make measurements of the charged particle populations in the radiation belts ...
J. Barney +11 more
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The experiment for space radiation analysis is an upcoming project for Los Alamos National Laboratory. This 12U CubeSat will be placed in a geosynchronous transfer orbit to make measurements of the charged particle populations in the radiation belts ...
J. Barney +11 more
semanticscholar +1 more source
Radiation Belts of Jupiter [PDF]
Science, 1974 Pioneer 10 counted relativistic electrons throughout the magnetosphere of Jupiter, with the greatest fluxes being inside 20 Jupiter radii. The peak flux of electrons with energy greater than 50 million electron volts was 1.3 × 10 7 per square centimeter per second at the innermost penetration of the radiation belts.
R. Walker Fillius, Carl E. McIlwain
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Galactic Radiation Belts. [PDF]
Nature, 1979 Abstract : This report suggests that electrons trapped in a dipolar field can reproduce some of the observed distributions of emission from extended extragalactic radio sources if the electron pitch-angle distributions are sufficiently anisotropic.
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Science, 1973
Predictions of Jupiter's electron and proton radiation belts are based mainly on decimeter observations of 1966 and 1968. Extensive calculations modeling radial diffusion of particles inward from the solar wind and electron synchrotron radiation are used to relate the predictions and observations.
R. Stephen White, Kent G. Stansberry
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Predictions of Jupiter's electron and proton radiation belts are based mainly on decimeter observations of 1966 and 1968. Extensive calculations modeling radial diffusion of particles inward from the solar wind and electron synchrotron radiation are used to relate the predictions and observations.
R. Stephen White, Kent G. Stansberry
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Journal of Geophysical Research, 1974
Fluxes of electrons and protons in Jupiter's radiation belts are calculated with the source (radial diffusion inward from the solar wind) and the loss (synchroton radiation). The calculations are tested against the measured radio-wave wavelength distribution, the radio-wave distribution with distance from Jupiter, and the degree of polarization of ...
R. Stephen White, Kent G. Stansberry
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Fluxes of electrons and protons in Jupiter's radiation belts are calculated with the source (radial diffusion inward from the solar wind) and the loss (synchroton radiation). The calculations are tested against the measured radio-wave wavelength distribution, the radio-wave distribution with distance from Jupiter, and the degree of polarization of ...
R. Stephen White, Kent G. Stansberry
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Icarus, 1973
A model for the production and loss of energetic electrons in Jupiter's radiation belt is presented. It is postulated that the electrons originate in the solar wind and are diffused in toward the planet by perturbations which violate the particles' third adiabatic invariant.
Thomas R. McDonough, Neil Brice
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A model for the production and loss of energetic electrons in Jupiter's radiation belt is presented. It is postulated that the electrons originate in the solar wind and are diffused in toward the planet by perturbations which violate the particles' third adiabatic invariant.
Thomas R. McDonough, Neil Brice
openaire +2 more sources