Results 1 to 10 of about 114,782 (336)
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
doaj +2 more sources
Processes in auroral oval and outer electron radiation belt [PDF]
We have analyzed the role of auroral processes in the formation of the outer radiation belt, considering that the main part of the auroral oval maps to the outer part of the ring current, instead of the plasma sheet as is commonly postulated.
Elizaveta E. Antonova +6 more
doaj +2 more sources
In this paper, we examined the combined effects of equatorial chorus waves and high‐latitude Z‐mode waves on the energy and pitch angle distribution of Saturn's radiation belt electrons.
J. Yu +4 more
doaj +2 more sources
Drift phase resolved diffusive radiation belt model: 1. Theoretical framework
Most physics-based models provide a coarse three-dimensional representation of radiation belt dynamics at low time resolution, of the order of a few drift periods. The description of the effect of trapped particle transport on radiation belt intensity is
Solène Lejosne, Jay M. Albert
doaj +1 more source
A data assimilation-based forecast model of outer radiation belt electron fluxes
Because radiation belt electrons can pose a potential threat to the safety of satellites orbiting in space, it is of great importance to develop a reliable model that can predict the highly dynamic variations in outer radiation belt electron fluxes.
Yuan Lei +5 more
doaj +1 more source
Dynamics of the inner electron radiation belt: A review
The Van Allen radiation belts are an extraordinary science discovery in the Earth magnetosphere and consist of two electron belts. The inner Van Allen belt contains electrons of 10s to 100s keV; the outer belt consists mainly of 0.1−10 MeV electrons ...
YuXuan Li +5 more
doaj +1 more source
The magnetic field of the solar corona has a large-scale dipole character, which maps into the bipolar field in the solar wind. Using standard representations of the coronal field, we show that high-energy ions can be trapped stably in these large-scale closed fields.
Hudson, H. S. +3 more
openaire +2 more sources
Differentiating Between the Leading Processes for Electron Radiation Belt Acceleration
Many spacecraft fly within or through a natural and variable particle accelerator powered by the coupling between the magnetosphere and the solar wind: the Earth’s radiation belts.
Solène Lejosne +10 more
doaj +1 more source
Quantitative assessment of Earth’s radiation belt modeling [PDF]
The “Quantitative Assessment of Radiation Belt Modeling” focus group was in place at Geospace Environment Modeling from 2014 to 2018. The overarching goals of this focus group were to bring together the current state‐of‐the‐art models for the ...
Albert, J. M. +3 more
core +3 more sources
Reconstruction of the Radiation Belts for Solar Cycles 17–24 (1933–2017)
We present a reconstruction of the dynamics of the radiation belts from solar cycles 17 to 24 which allows us to study how radiation belt activity has varied between the different solar cycles.
A. A. Saikin +5 more
doaj +1 more source

