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Article Dans Une Revue Journal of Atmospheric and Solar-Terrestrial Physics Année : 2006

Ionogram height–time–intensity observations of descending sporadic E layers at mid-latitude

Résumé

A new methodology of ionosonde height–time–intensity (HTI) analysis is introduced which allows the investigation of sporadic E layer (Es) vertical motion and variability. This technique, which is useful in measuring descent rates and tidal periodicities of Es, is applied on ionogram recordings made during a summer period from solstice to equinox on the island of Milos (36.71N; 24.51E). On the average, the ionogram HTI analysis revealed a pronounced semidiurnal periodicity in layer descent and occurrence. It is characterized by a daytime layer starting at 120km near 06 h local time (LT) and moving downward to altitudes below 100km by about 18 h LT when a nighttime layer appears above at_125 km. The latter moves also downward but at higher descent rates (1.6–2.2 km/h) than the daytime layer (0.8–1.5 km/h). The nighttime Es is weaker in terms of critical sporadic E frequencies (foEs), has a shorter duration, and tends to occur less during times close to solstice. Here, a diurnal periodicity in Es becomes dominant. The HTI plots often show the daytime and nighttime Es connecting with weak traces in the upper E region which occur with a semidiurnal, and at times terdiurnal, periodicity. These, which are identified as upper E region descending intermediate layers (DIL), play an important role in initiating and reinforcing the sporadic E layers below 120–125 km. The observations are interpreted by considering the downward propagation of wind shear convergent nodes that associate with the S2,3 semidiurnal tide in the upper E region and the S1,1 diurnal tide in the lower E region.
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Dates et versions

hal-00019336 , version 1 (21-02-2006)

Identifiants

Citer

Christos Haldoupis, Chris Meek, Nikolas Christakis, Dora Pancheva, Alain Bourdillon. Ionogram height–time–intensity observations of descending sporadic E layers at mid-latitude. Journal of Atmospheric and Solar-Terrestrial Physics, 2006, 68, pp.539-557. ⟨10.1016/j.jastp.2005.03.020⟩. ⟨hal-00019336⟩
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