1998
DOI: 10.1007/s00585-998-0711-8
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Non-trough <i>fo</i>F2 enhancements at near-equatorial dip latitudes

Abstract: Abstract. Fine resolution series from three equatorial ionosondes of the IEEY network in West Africa have revealed small-scale daytime peak F2 structures, superposed on the slowly varying minimum or``trough'' distribution in the 5°magnetic latitude zone. We report this new morphology, concentrating on foF2 enhancements of two types: near-equatorial crests (which travel either northwards or southwards) and magnetic ®eld-aligned domes, whose onsets last only tens of minutes. Both types are observed to start at m… Show more

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Cited by 7 publications
(6 citation statements)
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“…Electrodynamics and wind e ects of the West African asymmetry in annual solar declination changes should produce a short summer (April-July) and a very long winter (SeptemberMarch), as shown by Sambou et al (1998) for foF2 variations. On ESF, on the contrary, we observe a rather shorter "winter" and a longer "summer" (Figs.…”
Section: Seasonal Esf ÿRst-look Resultsmentioning
confidence: 98%
“…Electrodynamics and wind e ects of the West African asymmetry in annual solar declination changes should produce a short summer (April-July) and a very long winter (SeptemberMarch), as shown by Sambou et al (1998) for foF2 variations. On ESF, on the contrary, we observe a rather shorter "winter" and a longer "summer" (Figs.…”
Section: Seasonal Esf ÿRst-look Resultsmentioning
confidence: 98%
“…Thus there is need for observations at a constant height. Satellite coverage of the upper thermospheric parameters only provide LT constructs of diurnal variations combined together over long series of days, and such samples provide global averages where composite solar time changes are mixed with the poorly known "longitude effects" (Sambou et al, 1998). Thus the needs for simultaneous wind measurements.…”
Section: Resultsmentioning
confidence: 99%
“…Fig. 5 (Sambou et al, 1998) shows the latitude versus local time of f 0 F 2 variations for three successive days in March, 1993 (bottom panels), and the variations of the H magnetic field component (top panels).…”
Section: Morphology and Dynamics Of The Equatorial Plasmasmentioning
confidence: 99%
“…5. Evolution of the f 0 F 2 (bottom panels) and H component of the Earth's magnetic field (top panels), D is for Dakar, O for Ouagadougou and K for Korhogo (from Sambou et al, 1998). cycle years (Faynot and Vila, 1979). These discrepancies are not yet understood.…”
Section: Morphology and Dynamics Of The Equatorial Plasmasmentioning
confidence: 99%