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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The Valensole high frequency (HF) radar in the south of France is an ionospheric Doppler sounder which can perform E region coherent backscatter measurements over an azimuthal sector of 86 ø, from 26 ø E to 58 ø W, with -• 2 ø angular resolution. This large azimuthal coverage is taken advantage of in order to study quasiperiodic (QP) echoes in the zonal direction using azimuth-time-intensity (ATI) analysis. ATI plots show sequential sloping striations of scatter reminiscent of those detected routinely in the range-timeintensity (RTI) plots of midlatitude radars which view the medium at a fixed azimuth about the meridian. It was found that ATI striation periods range from a few minutes to less than 30 min, whereas the striation slopes are systematically negative (motions westward) prior to local midnight, and turn positive (motions eastward) in the post-midnight hours. The zonal rates, dx/dt, computed from the striation slopes take values between -• 30 and 160 m/s. These are due to real motions of unstable plasma structures, most likely sporadic E patches that drift along with the neutral wind, that have zonal scale lengths of several tens of kilometers. The present observations imply that the mechanism responsible for QP echoes is independent of azimuth and can basically operate effectively in any direction in the horizontal plane.