Eastward sub-auroral ion drifts or ASAID
From satellite data sampling the top ionosphere in the Northern Hemisphere we have identified strong eastward ion drifts, with speeds larger than 1 km/s, widths of 1°–2°, occurring at similar temporal and spatial locations as rapid westward ion drifts known as sub-auroral ion drif...
| Main Authors: | , |
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| Format: | Article |
| Language: | English |
| Published: |
Copernicus Publications
2008-07-01
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| Series: | Annales Geophysicae |
| Online Access: | https://www.ann-geophys.net/26/1955/2008/angeo-26-1955-2008.pdf |
| Summary: | From satellite data sampling the top ionosphere in the Northern Hemisphere we
have identified strong eastward ion drifts, with speeds larger than 1 km/s,
widths of 1°–2°, occurring at similar temporal and spatial
locations as rapid westward ion drifts known as sub-auroral ion drifts
(SAID). We have called these events "abnormal sub-auroral ion drifts"
(ASAID). Two events observed in the 20:00–22:00 MLT interval are discussed: the
first occurring on 21 September 2003 and the other on 12 October 2003.
Tomographic reconstructions of the electron density in the F-region, based on
satellite data, provided by the Scandinavian tomography chain, were also
available. We have observed that ASAID are accompanied by upward flows with
a speed of the same order as that of the zonal ion drift. They coincide with
deep, narrow troughs in the total ion density, both at the altitude of the F15
DMSP satellite (850 km) and in the F-region of the ionosphere, but do not
seem to be a feature of the convective transport. During the entire duration
of ASAID the electron temperature is very high while, contrary to SAID, the
ion temperature has no clear variation. Both events described in this paper
end up turning into classical SAID. Satellite data indicate that the
generator of ASAID could be located inside the plasmasphere close to the
plasmapause and we suggest a possible mechanism for their formation. |
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| ISSN: | 0992-7689 1432-0576 |