Empirically Estimated Electron Lifetimes in the Earth's Radiation Belts: Comparison With Theory [PDF]
We compute quasilinear diffusion rates due to pitch angle scattering by various mechanisms in the Earth's electron radiation belts. The calculated theoretical lifetimes are compared with observed decay rates, and we find excellent qualitative agreement ...
S. G. Claudepierre +5 more
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Empirically Estimated Electron Lifetimes in the Earth's Radiation Belts: Van Allen Probe Observations [PDF]
We use measurements from NASA's Van Allen Probes to calculate the decay time constants for electrons over a wide range of energies (30 keV to 4 MeV) and L values ( L = 1.3–6.0) in the Earth's radiation belts.
S. G. Claudepierre +5 more
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Chorus wave power at the strong diffusion limit overcomes electron losses due to strong diffusion [PDF]
Earth’s radiation belts consist of high-energy charged particles trapped by Earth’s magnetic field. Strong pitch angle diffusion of electrons caused by wave-particle interaction in Earth’s radiation belts has primarily been considered as a loss process ...
T. A. Daggitt +4 more
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Correction: Publisher Correction: Wave energy budget analysis in the Earth’s radiation belts uncovers a missing energy [PDF]
Nature Communications 6: Article number: 7143 (2015); Published: 15 May 2015; Updated: 26 March 2018 The original HTML version of this Article had an incorrect article number of 8143; it should have been 7143. This has now been corrected in the HTML; the
A. V. Artemyev +4 more
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Lightning-induced relativistic electron precipitation from the inner radiation belt [PDF]
The Earth’s radiation belts are maintained by a number of acceleration, loss and transport mechanisms, and the electron fluxes at any given time are highly variable.
Max Feinland +5 more
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A slot region in the magnetosphere of Jupiter [PDF]
Understanding the balance between charged particle acceleration and loss is central to radiation belt research. Jupiter’s Galilean moons orbit within its intense radiation environment and can act both as sources and sinks of energetic particles.
Minyi Long +11 more
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Influence of solar extreme ultraviolet radiations on artificial very-low-frequency waves in near-earth space [PDF]
Ground-based very low frequency (VLF) transmitter waves (3 – 30 kHz) can cause the precipitation loss of high-energy electrons in Earth’s radiation belts.
K. X. Cheng +5 more
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EVIDENCE OF THE EARTH’S INNER RADIATION BELTS DURING THE LOW SOLAR AND GEOMAGNETIC ACTIVITY OBTAINED WITH THE STEP-F INSTRUMENT [PDF]
Purpose: The subject of research is the spatio-temporal charged particles in the Earth’s magnetosphere outside the South Atlantic magnetic Anomaly during the 11-year cycle of solar activity minimum.
O. V. Dudnik, O. V. Yakovlev
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Distribution of Earth's radiation belts' protons over the drift frequency of particles [PDF]
Using data on the proton fluxes of the Earth's radiation belts (ERBs) with energy ranging from 0.2 to 100 MeV on the drift L shells ranging from 1 to 8, the quasi-stationary distributions over the drift frequency fd of protons around the Earth are ...
A. S. Kovtyukh
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An operational approach to forecast the Earth’s radiation belts dynamics
The Ca index is a time-integrated geomagnetic index that correlates well with the dynamics of high-energy electron fluxes in the outer radiation belts.
Bernoux Guillerme +4 more
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