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Al(ii) transfer harnessing a well-defined cadmium precursor. [PDF]
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Energetic electron precipitation in Jupiter's upper atmosphere
Journal of Geophysical Research: Planets, 1992Energy deposition by electrons having a Maxwellian energy distribution with characteristic energies 10, 30, and 100 keV, precipitating in the high‐latitude upper atmosphere of Jupiter, has been studied using a continuous slowing down approximation. Electron fluxes, volume excitation, and ionization rates have been calculated.
R. P. Singhal +3 more
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Precipitation of energetic electrons into the atmosphere
Journal of Geophysical Research, 1964Measurements were made of electron fluxes and spectrums above 900 kev at altitudes between 200 and 700 km in early September and October 1962 aboard two near-polar Air Force satellites. The particle fluxes were observed with shielded solid-state detectors having a 2π solid angle.
George A. Paulikas, Stanley C. Freden
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Precipitation of energetic electrons at middle latitudes
Journal of Geophysical Research, 1966Measurements of quasi-trapped electrons with energies greater than 300 kev in August 1964 have extended the temporal observations of these precipitating particles. These electrons are lost in the atmosphere as they drift into the South Atlantic magnetic anomaly.
G. A. Paulikas +2 more
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Pulsations of precipitating energetic electrons: ACTIVE satellite data
Journal of Atmospheric and Solar-Terrestrial Physics, 1998We present the patterns of high frequency energetic electron (~ 20 to ~ 300 keV) pulsations in middle latitudes, in subauroral and auroral regions, based on low altitude nearly polar orbiting satellite (Intercosmos-24, project ACTIVE) measurements.
K. Kudela +4 more
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Test particle modeling of wave‐induced energetic electron precipitation
Journal of Geophysical Research: Space Physics, 1985A test particle computer model of the precipitation of radiation belt electrons is extended to compute the dynamic energy spectrum of transient electron fluxes induced by short‐duration VLF wave packets traveling along the geomagnetic field lines. The model is adapted to estimate the count rate and associated spectrum of precipitated electrons that ...
Inan, U. S., Chang, Hung-Chun
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Pc 3 magnetic pulsations and precipitation of energetic electrons
Journal of Geophysical Research: Space Physics, 1979Data from the synchronous altitude satellite ATS 1 and near‐conjugate measurements of bremsstrahlung X rays and ground magnetic variations have been used to analyze an event of modulated auroral zone electron precipitation and magnetic pulsations in the Pc 3 range.
C.W. Arthur, J. Bjordal, T.J. Rosenberg
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Energetic electron precipitation induced by space based VLF transmitters
Journal of Geophysical Research: Space Physics, 2008Numerical raytracing with Landau damping is used to calculate electron precipitation that would be induced by in situ sources located at L = 2 and L = 2.5, at the geomagnetic equator and also at a geomagnetic latitude of 20° along each field line. In accordance with the Wang and Bell (1970) model of antenna radiation in a magnetoplasma, we consider ...
P. Kulkarni, U. S. Inan, T. F. Bell
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Modeling energetic electron precipitation near the South Atlantic anomaly
Journal of Geophysical Research: Space Physics, 1999A numerical simulation of electron pitch angle scattering in an asymmetric magnetic field environment has been applied to the Earth's inner radiation belt to obtain a global pattern of energetic electron precipitation. Under conditions of weak pitch angle scattering, which characterize the region L ≤ 2, the flux of electrons precipitated into the ...
Bob Abel, Richard M. Thorne
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Precipitation of energetic magnetospheric electrons and accompanying solar wind characteristics
Geomagnetism and Aeronomy, 2017From 1957 up to the present time, the Lebedev Physical Institute (LPI) has performed regular monitoring of ionizing radiation in the Earth’s atmosphere. There are cases when the X-ray radiation generated by energetic magnetospheric electrons penetrates the atmosphere and is observed at polar latitudes.
G. A. Bazilevskaya +9 more
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