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Quasi-90-day oscillation observed in the MLT region at low latitudes from the Kunming meteor radar and SABER 被引量:7

Quasi-90-day oscillation observed in the MLT region at low latitudes from the Kunming meteor radar and SABER
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摘要 Observations of a quasi-90-day oscillation in the mesosphere and lower thermosphere(MLT) region from April 2011 to December 2014 are presented in this study. There is clear evidence of a quasi-90-day oscillation in temperatures obtained from the Kunming meteor radar(25.6°N, 103.8°E) and Sounding of the Atmosphere using Broadband Emission Radiometry(SABER), as well as in wind observed by the Kunming meteor radar. The quasi-90-day oscillation appears to be a prominent feature in the temperatures and meridional wind tides and presents quite regular cycles that occur approximately twice per year. The amplitudes and phases of the quasi-90-day oscillation in the SABER temperature show a feature similar to that of upward-propagated diurnal tides, which have a vertical wavelength of ~20 km above 70 km. In the lower atmosphere, a similar 90-day variability is presented in the surface latent heat flux and correlates with the temperature in the MLT region. Similar to the quasi-90-day oscillation in temperature, a 90-day variability of ozone(O3) is also present in the MLT region and is considered to be driven by a similar variability in the upwardly-propagated diurnal tides generated in the lower atmosphere. Moreover, the 90-day variability in the absorption of ultraviolet(UV) radiation by daytime O3 in the MLT region is an in situ source of the quasi-90-day oscillation in the MLT temperature. Observations of a quasi-90-day oscillation in the mesosphere and lower thermosphere(MLT) region from April 2011 to December 2014 are presented in this study. There is clear evidence of a quasi-90-day oscillation in temperatures obtained from the Kunming meteor radar(25.6°N, 103.8°E) and Sounding of the Atmosphere using Broadband Emission Radiometry(SABER), as well as in wind observed by the Kunming meteor radar. The quasi-90-day oscillation appears to be a prominent feature in the temperatures and meridional wind tides and presents quite regular cycles that occur approximately twice per year. The amplitudes and phases of the quasi-90-day oscillation in the SABER temperature show a feature similar to that of upward-propagated diurnal tides, which have a vertical wavelength of ~20 km above 70 km. In the lower atmosphere, a similar 90-day variability is presented in the surface latent heat flux and correlates with the temperature in the MLT region. Similar to the quasi-90-day oscillation in temperature, a 90-day variability of ozone(O3) is also present in the MLT region and is considered to be driven by a similar variability in the upwardly-propagated diurnal tides generated in the lower atmosphere. Moreover, the 90-day variability in the absorption of ultraviolet(UV) radiation by daytime O3 in the MLT region is an in situ source of the quasi-90-day oscillation in the MLT temperature.
出处 《Earth and Planetary Physics》 CSCD 2019年第2期136-146,共11页 地球与行星物理(英文版)
基金 supported by Project(KJCX2-EW-J01,KZZD-EW-0101)of the Chinese Academy of Sciences the National Natural Science Foundation of China(41322029,41474129,41421063 and41804147) the National Basic Research Program of China(2012CB825605) the Youth Innovation Promotion Association of the Chinese Academy of Sciences(2011324) the Fundamental Research Funds for the Central Universities the open research project of Chinese Academy of Sciences Large Research Infrastructures the Chinese Meridian Project the Open Research Program of National Key Laboratory of Electromagnetic Environment of the China Research Institute of Radiowave Propagation
关键词 quasi-90-day OSCILLATION METEOR radar TEMPERATURES SABER TEMPERATURES tides latent heat release SABER ozone quasi-90-day oscillation meteor radar temperatures SABER temperatures tides latent heat release SABER ozone
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