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Direct observation of the CRAND proton radiation belt source
Author(s) -
Selesnick R. S.,
Hudson M. K.,
Kress B. T.
Publication year - 2013
Publication title -
journal of geophysical research: space physics
Language(s) - English
Resource type - Journals
eISSN - 2169-9402
pISSN - 2169-9380
DOI - 10.1002/2013ja019338
Subject(s) - cosmic ray , physics , computational physics , proton , van allen radiation belt , neutron , intensity (physics) , geomagnetic storm , monte carlo method , diffusion , radiation , earth's magnetic field , nuclear physics , solar wind , magnetic field , magnetosphere , optics , plasma , statistics , mathematics , quantum mechanics , thermodynamics
Observations of geomagnetically trapped 27–45 MeV protons following the November 2003 magnetic storm show a gradual intensity rise that is interpreted as a direct measurement of the cosmic ray albedo neutron decay (CRAND) source strength. The intensity rise is simulated by combining the detector response function with a model CRAND source, obtained by drift‐averaging neutron intensity from Monte Carlo simulation of cosmic ray interactions in the atmosphere. The simulation, for 2.4< L <2.7, matches the data within statistical uncertainties, verifying the CRAND model. Another simulation includes the effects of solar proton trapping and other known radiation belt processes. It further shows that the CRAND source was predominant, while radial diffusion and magnetic storm losses effected minor corrections in certain L ranges.