A theoretical study of solar cycle variations of electron density and temperature in stable auroral red arcs

Details A theoretical study of solar cycle variations of electron density and temperature in stable auroral red arcs A theoretical study of solar cycle variations of electron density and temperature in stable auroral red arcs

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997adspr..20.1727p&link_type=abstract

Advances in Space Research, Volume 20, Issue 9, p. 1727-1730.

Physics

Scientific paper

It is shown that for a fixed efficiency of converted ring current energy model stable aurora red (SAR) arcs are stronger at solar maximum than at solar minimum. The modeled SAR arc electron temperature does not vary significantly with solar cycle in agreement with observational data. The depletion of the plasmasphere during the main phase of geomagnetic storms significantly affects the modeled SAR arc electron densities in the altitude range 200 to 1000 km at solar minimum but not at solar maximum.

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