Physics
Scientific paper
Apr 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984jgr....89.2348s&link_type=abstract
Journal of Geophysical Research (ISSN 0148-0227), vol. 89, April 1, 1984, p. 2348-2358.
Physics
21
Auroral Ionization, F Region, Ion Temperature, Ionospheric Ion Density, Magnetic Storms, Atmospheric Models, Earth Magnetosphere
Scientific paper
The response of the high-latitude F region to magnetospheric storm inputs is modelled. During the 'storm', the spatial extent of the auroral oval, the intensity of the precipitating auroral electron energy flux, and the plasma convection pattern were varied with time. During the storm growth phase, the auroral oval expanded, the precipitating electron energy flux increased, and the magnetospheric convection pattern changed from a symmetric two-cell pattern with a 20 kV cross-tail potential to an asymmetric two-cell pattern with a total cross-tail potential of 90 kV. During the storm, there were significant changes in the ion temperature, ion composition, and molecular/atomic ion transition height. The storm time asymmetric convection pattern produced an ion temperature hot spot at the location of the dusk convection cell that contained significantly enhanced NO(+) densities. During the storm recovery phase, the decay of these densities closely followed the decrease in the plasma convection speed.
Schunk Robert W.
Sojka Jan J.
No associations
LandOfFree
A theoretical F region study of ion compositional and temperature variations in response to magnetospheric storm inputs does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with A theoretical F region study of ion compositional and temperature variations in response to magnetospheric storm inputs, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A theoretical F region study of ion compositional and temperature variations in response to magnetospheric storm inputs will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1500271