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The terdiurnal tide in the mesosphere and lower thermosphere over Wuhan (30◦ N, 114◦ E)

Earth Planets and Space (Impact Factor: 3.06). 01/2005; 57:393-398. DOI: 10.1186/BF03351823

ABSTRACT Winds measured by an all-sky meteor radar have been used to investigate the terdiurnal tide in the mesosphere and lower thermosphere (MLT) region over Wuhan (30.6 • N, 114.4 • E). We present a climatology of the terdiurnal tide at low-mid latitude site during the period of April 2002 to December 2004. The terdiurnal peak is distinct in the long-term power spectrum of the wind. The monthly and seasonal mean maximum amplitudes have values of 7 m/s and 5 m/s, respectively. The short-term amplitudes can occasionally reach up to 30 m/s, and at times the terdiurnal tide is as large as the diurnal and semidiurnal ones. It seems that the meridional component is more regular than the zonal one. An obvious annual variation is observed in the meridional phases with a phase leading in winter than that in summer. The annual variation for the terdiurnal tidal amplitude is not obvious, and is variable from year to year in our observations. This seasonal trend is slightly different from earlier studies at other locations.

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    • "Satellite observations of the migrating and nonmigrating modes and the global nature of TDT have also been reported by Smith [2000] and Forbes et al. [2008]. In the MLT region, the amplitude of TDT is generally smaller than but can be comparable to the diurnal or semidiurnal tide [e.g., Zhao et al., 2005]. TDT exhibits strong latitudinal and seasonal variation. "
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