Comparison of model high-latitude electron densities with Millstone Hill observations

Citation data:

Journal of Geophysical Research, ISSN: 0148-0227, Vol: 88, Issue: A10, Page: 7783-7793

Publication Year:
1983
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Repository URL:
https://works.bepress.com/jan_sojka/139; https://digitalcommons.usu.edu/physics_facpub/103
DOI:
10.1029/ja088ia10p07783
Author(s):
Sojka, Jan Josef; Schunk, Robert W.; Evans, J. V.; Holt, J. M.; Wand, R. H.
Publisher(s):
Wiley-Blackwell; American Geophysical Union (AGU); American Geophysical Union
Tags:
Earth and Planetary Sciences; Agricultural and Biological Sciences; Environmental Science; Physics and Astronomy; Chemistry; Materials Science; comparison; model; high-latitude; electron densities; Millston Hill; observations; Physics
article description
Model predictions of the diurnal variations of plasma convection velocities and electron densities in the high-latitude ionosphere were compared with Millstone Hill incoherent scatter radar observations for an equinox day on which there was moderate magnetic activity. The model was able to reproduce two features quite accurately. Except for a discrete arc region in the dusk sector, the enhanced electron densities in the auroral zone were adequately described by the average precipitation fluxes used in the model. The observed plasma drift velocities were consistent with a two-cell, asymmetric convection pattern with enhanced flow in the dusk sector. Outside the polar cap, the fall-off of the magnetospheric potential with latitude was proportional to the inverse of the sine of colatitude to the fourth power.