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Rethinking Pulmonary Function Tests in Patients with Neuromuscular Disease: The Potential Role of Electrical Impedance Tomography. [PDF]
J Clin MedVianello A, Guarnieri G, Lionello F.
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Late Holocene fast-ice dynamics around the Northern Victoria Land coast, Antarctica. [PDF]
Nat CommunTesi T +16 more
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Reveal the deployable solar energy potential and emission reduction benefits in the arid areas of Xinjiang. [PDF]
Sci RepLi N +5 more
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Structures control gold mineralization in the western Allaqi shear belt of Egypt from high-precision geophysical and remote sensing datasets. [PDF]
Sci RepEldosouky AM +3 more
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Research on the network structure evolution characteristics of outdoor sports tourism flow in the Yangtze River Economic belt based on online travel notes. [PDF]
Sci RepXiao N, Zhao B.
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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.
K G, Stansberry, R S, White
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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.
K G, Stansberry, R S, White
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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
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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
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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 ...
Kent G. Stansberry, R. Stephen White
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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 ...
Kent G. Stansberry, R. Stephen White
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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.
Neil Brice, Thomas R. Mcdonough
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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.
Neil Brice, Thomas R. Mcdonough
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2006
The effects induced by the space environment on space vehicles and astronauts no longer need to be demonstrated. The nature of this environment varies greatly between low orbits and higher orbits such as the geostationary orbit and beyond. In this chapter, we attempt to describe the space environment relative to ionizing particles.
Sébastien Bourdarie, Daniel Boscher
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The effects induced by the space environment on space vehicles and astronauts no longer need to be demonstrated. The nature of this environment varies greatly between low orbits and higher orbits such as the geostationary orbit and beyond. In this chapter, we attempt to describe the space environment relative to ionizing particles.
Sébastien Bourdarie, Daniel Boscher
openaire +1 more source