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Electron flux dropouts at Geostationary Earth Orbit: Occurrences, magnitudes, and main driving factors
Author(s) -
Boynton R. J.,
Mourenas D.,
Balikhin M. A.
Publication year - 2016
Publication title -
journal of geophysical research: space physics
Language(s) - English
Resource type - Journals
eISSN - 2169-9402
pISSN - 2169-9380
DOI - 10.1002/2016ja022916
Subject(s) - geosynchronous orbit , geostationary orbit , flux (metallurgy) , electron , earth's magnetic field , range (aeronautics) , physics , solar wind , substorm , computational physics , atomic physics , plasma , nuclear physics , magnetosphere , chemistry , satellite , astronomy , materials science , magnetic field , organic chemistry , quantum mechanics , composite material
Large decreases of daily average electron flux, or dropouts, were investigated for a range of energies from 24.1 keV to 2.7 MeV, on the basis of a large database of 20 years of measurements from Los Alamos National Laboratory (LANL) geosynchronous satellites. Dropouts were defined as flux decreases by at least a factor 4 in 1 day, or a factor 9 in 2 days during which a decrease by at least a factor of 2.5 must occur each day. Such decreases were automatically identified. As a first result, a comprehensive statistics of the mean waiting time between dropouts and of their mean magnitude has been provided as a function of electron energy. Moreover, the Error Reduction Ratio analysis was applied to explore the possible nonlinear relationships between electron dropouts and various exogenous factors, such as solar wind and geomagnetic indices. Different dropout occurrences and magnitudes were found in three distinct energy ranges, lower than 100 keV, 100–600 keV, and larger than 600 keV, corresponding to different groups of drivers and loss processes. Potential explanations have been outlined on the basis of the statistical results.