Mesospheric Waves Observed By The Superdarn Radars At Sanae And Halley, Antarctica: Preliminary Results

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We present early results of mesospheric waves using the Super Dual Auroral Radar Network (SuperDARN) HF radars at the South African National Antarctic Expedition (SANAE, 71^o40'S,2^o50'W) and Halley (75^o35'S, 26^o34'W), Antarctica. The longitudinal spread of the SuperDARN radars provides an opportunity to study mesospheric dynamics at high latitudes and, in particular, the associated longitudinal differences. At both sites, the observations show a wide spectrum of atmospheric waves ranging from tidal to planetary frequencies. SANAE has a stronger tidal activity with both the diurnal and semidiurnal tides reaching maximum amplitudes of about 20 ms-1 compared to amplitude peaks of about 8 ms-1 at Halley. In general, tidal amplitudes show planetary scale variations that are superimposed on seasonal trends. Part of the planetary modulation of tides is due to non-linear interactions between tides and planetary waves leading to quadratic phase coupling.

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