Physics
Scientific paper
Dec 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agufmsa41a1540l&link_type=abstract
American Geophysical Union, Fall Meeting 2008, abstract #SA41A-1540
Physics
3332 Mesospheric Dynamics, 3384 Acoustic-Gravity Waves, 3389 Tides And Planetary Waves
Scientific paper
During the 9-day continuous campaign in September 2003, the Colorado State University sodium lidar observed significant short-term tidal variability in both diurnal and semidiurnal tides above 85 km in days 265- 268. Both diurnal and semidiurnal amplitudes dramatically increased on day 267 with a continuous phase advance in diurnal tidal harmonics, causing local atmosphere to become dynamically unstable. Following the dynamical instability associated with tides, we observed equally dramatic decrease in diurnal amplitude, which was accompanied by rapid and continuous phase retardation at 87 km on day 268; the accompanying diurnal phase profiles changed from propagating mode to evanescent mode. Since the time scale of the observed variability during days 265-268 is less than one day, gravity wave/tidal interaction at least is partially responsible for the observed variability. The observed changes in tidal amplitudes and phases are correlated with gravity wave activities concurrently observed by an OH all-sky imager at nearby Yucca Ridge station, as suggested by well known models of tidal/gravity wave interactions. The stability analysis in the night of 267, when both diurnal and semidiurnal reached the maximum amplitudes, revealed that the running daily tidal waves alone, superimposed with the associated mean state, are able to push the atmosphere into local dynamical instability near 90-95 km. The eddy diffusion associated with the instability is believed to have caused a strong dissipation of diurnal tide as observed on day 268.
Dou Xu
Krueger David
Li Tiancheng
Liu Hongya
Nakamura Takashi
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