Results 241 to 250 of about 110,170 (299)

A slot region in the magnetosphere of Jupiter. [PDF]

open access: yesNat Commun
Long M   +11 more
europepmc   +1 more source

Comprehensive Observations of Magnetospheric Particle Acceleration, Sources, and Sinks (COMPASS): A Mission Concept to Explore the Extremes of Jupiter's Magnetosphere. [PDF]

open access: yesSpace Sci Rev
Clark G   +54 more
europepmc   +1 more source

Toward Nanodisc Tailoring for SANS Study of Membrane Proteins. [PDF]

open access: yesBioengineering (Basel)
Batchu KC, Tully MD, Martel A.
europepmc   +1 more source

Exploration of Copper Halide Linear-Array Detector Prototype for Security Checks. [PDF]

open access: yesSmall
Zhou Y   +7 more
europepmc   +1 more source

Radiation Belts of Jupiter

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 W, Fillius, C E, McIlwain
openaire   +2 more sources

Radiation Belts of Jupiter

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.
K G, Stansberry, R S, White
openaire   +2 more sources

The radiation belts

Radiation Physics and Chemistry, 1994
Abstract The Earth's radiation belts, formed by energetic electrons and ions (principally protons) trapped in the Earth's quasi-dipolar field, are reviewed. The magnitudes of particle energies and fluxes encountered make this a very severe environment in which to conduct space missions.
openaire   +1 more source

The Jovian Radiation Belt

1974
Jupiter is a copious source of radiowaves having a wavelength of 3–75 cm. The radiation is 20% or so linearly polarized perpendicular to the planet rotation axis, does not vary much in intensity over the entire range of observed frequencies, and changes slowly in intensity over a time interval of the order of a few years.
D. B. Beard, J. L. Luthey
openaire   +1 more source

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