Electron temperatures during rapid subauroral ion drift events - Archive ouverte HAL Access content directly
Journal Articles Annales Geophysicae Year : 1998

Electron temperatures during rapid subauroral ion drift events

(1) , (1) , (1) , (2) , (3)
1
2
3

Abstract

Examples of data from DE-2 satellite instruments are presented. These illustrate the behaviour of plasma parameters in the F-region and adjacent topside ionosphere during rapid sub-auroral ion drift (SAID) events. In particular, a variety of behaviours of the electron temperature (Te) is demonstrated, both within and equatorward of the SAID region. The Sheffield University plasmasphere-ionosphere model (SUPIM) is used to perform calculations in which a model SAID is applied to a plasma flux tube. The model results indicate that strongly elevated ion temperature (a recognised signature of SAID events) is on occasion sufficient to raise Te to observed values by ion-electron heat transfer. On other occasions, an additional heat source is required. It is suggested that such a source for the electron gas may be due to interaction between the ring current and the plasmasphere at high altitudes. The magnitude of the downward heat flux is consistent with that necessary to produce sub-auroral red arcs. The resulting strongly heated electron gas causes vibrational excitation of molecular nitrogen in the thermosphere.
Fichier principal
Vignette du fichier
angeo-16-450-1998.pdf (332.13 Ko) Télécharger le fichier
Origin : Explicit agreement for this submission
Loading...

Dates and versions

hal-00316378 , version 1 (01-01-1998)

Identifiers

  • HAL Id : hal-00316378 , version 1

Cite

R. J. Moffett, A. E. Ennis, G. J. Bailey, R. A. Heelis, L. H. Brace. Electron temperatures during rapid subauroral ion drift events. Annales Geophysicae, 1998, 16 (4), pp.450-459. ⟨hal-00316378⟩
120 View
98 Download

Share

Gmail Facebook Twitter LinkedIn More