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Temporal and spatial evolution of auroral electron energy spectra in a region surrounding the magnetic zenith
Author(s) -
Tuttle S.,
Gustavsson B.,
Lanchester B.
Publication year - 2014
Publication title -
journal of geophysical research: space physics
Language(s) - English
Resource type - Journals
eISSN - 2169-9402
pISSN - 2169-9380
DOI - 10.1002/2013ja019627
Subject(s) - incoherent scatter , brightness , zenith , electron precipitation , physics , radar , computational physics , electron , spectral line , energy flux , emission spectrum , magnetic field , astrophysics , geophysics , optics , ionosphere , astronomy , magnetosphere , quantum mechanics , telecommunications , computer science
We present a new method for estimating the spatial and temporal evolution of the auroral electron energy spectrum at subkilometer and subsecond scales using optical and incoherent scatter radar data. This method is applied to an event on 12 December 2006 when a thin auroral arc that exhibits subkilometer structuring is observed. The energy spectrum and resultant emission rates are estimated for a 10 s period when the arc was in the field of view of the optical instrumentation. Modeled images of the observed aurora are produced using the estimated emission rates and compared with the optical observations of the aurora. We find the modeled images reproduce the structure and dynamics of the observed aurora to within the uncertainties of the models used. The brightness underestimate of about 30% can be explained by the underestimate of the energy flux from the radar measurements.