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Inner zone and slot electron radial diffusion revisited
Author(s) -
O'Brien T. P.,
Claudepierre S. G.,
Guild T. B.,
Fennell J. F.,
Turner D. L.,
Blake J. B.,
Clemmons J. H.,
Roeder J. L.
Publication year - 2016
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1002/2016gl069749
Subject(s) - pitch angle , van allen radiation belt , diffusion , physics , scattering , electron , bundle , computational physics , radial velocity , van allen probes , optics , materials science , plasma , astrophysics , geophysics , magnetosphere , quantum mechanics , stars , composite material
Using recent data from NASA's Van Allen Probes, we estimate the quiet time radial diffusion coefficients for electrons in the inner radiation belt ( L < 3) with energies from ~50 to 750 keV. The observations are consistent with dynamics dominated by pitch angle scattering and radial diffusion. We use a coordinate system in which these two modes of diffusion are separable. Then we integrate phase space density over pitch angle to obtain a “bundle content” that is invariant to pitch angle scattering, except for atmospheric loss. We estimate the effective radial diffusion coefficient from the temporal and radial variation of the bundle content. We show that our diffusion coefficients agree well with previously determined values obtained in the 1960s and 1970s and follow the form one expects for radial diffusion caused by exponentially decaying impulses in the large‐scale electrostatic potential.