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Gravity wave parameters and their seasonal variations derived from Na lidar observations at 23°S

机译:重力波参数及其季节性变化是从23°S的Na激光雷达观测得出的

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The nightly and seasonal variability of gravity wave activity and spectra in the mesopause region are studied with 10 years of sodium lidar observations. From the linear layer density response to gravity wave forcing, the lidar data were analyzed to get the atmospheric density perturbations and their spectra. The atmospheric density perturbation, density variance for fluctuations with vertical scales between 2 and 10 km, and amplitudes of density perturbation spectra at m = 2π/8 km and 2π/4 km all exhibit large nightly variability as well as large seasonal variations, with the semiannual maxima occurring near the equinoxes. The mean RMS atmospheric density perturbation and the mean RMS horizontal wind perturbations over our site are 5.1% and 25 m/s, respectively. The growth lengths of the density perturbations in spring and autumn are lower than those in summer and winter, and the annual mean value is 38 km. The annual mean density shear variance is about 15 (%/km)2, and the maxima occur near the equinoxes. The mean Richardson number is about 1.0. The mean value of the RMS vertical wind perturbation is 0.85 m/s with a maximum occurring at the end of the year. The m spectra show power law shapes, and their range of variation is between ?2.06 and ?3.81 with an annual mean value of ?2.93. The ω spectra also show power law shapes, and their range of variation is between ?1.06 and ?2.32, with an annual mean of ?1.64. The mean amplitudes of density perturbation spectrum, Fa(m) (m = 2π/4 km), and of the horizontal wind fluctuation, Fu(m) (m = 2π/4 km), are 1.35(m/cycles) and 3 × 105(m2 s?2/(cycles/m)), respectively. The value of λ z* averaged around autumn equinox is 14.8 km, which is lower than the value of 16.8 km, averaged around spring equinox. The annual mean of T* is 23.5 hours. The fact that the joint (m,ω) spectra are not separable, together with the large variability found in the m spectra slopes, is not compatible with linear instability theory but is compatible with Doppler spreading theories and diffusive filtering theory.
机译:通过对十年的钠激光雷达观测,研究了更年期地区重力波活动和光谱的夜间和季节性变化。从线性层密度对重力波强迫的响应,分析了激光雷达的数据,得到了大气密度扰动及其光谱。大气密度扰动,垂直尺度在2至10 km之间波动的密度方差以及m =2π/ 8 km和2π/ 4 km处的密度扰动谱的振幅均表现出较大的夜间变化和较大的季节性变化,其中半年最大值出现在春分点附近。我们站点的平均RMS大气密度扰动和平均RMS水平风扰动分别为5.1%和25 m / s。春季和秋季的密度扰动生长长度小于夏季和冬季的密度扰动的生长长度,年均值为38 km。年平均密度剪切方差约为15(%/ km)2,最大值出现在春分点附近。理查森平均数约为1.0。 RMS垂直风扰动的平均值为0.85 m / s,最大值出现在年底。 m个谱图显示了幂律形状,其变化范围在2.06到3.81之间,年平均值为2.93。 ω谱还显示出幂律形状,其变化范围在1.06和2.32之间,年平均为1.64。密度摄动谱的平均振幅Fa(m)(m =2π/ 4 km)和水平风起伏的Fu(m)(m =2π/ 4 km)的平均振幅分别为1.35(m / cycles)和3 ×105(m2 s2 / 2 /(周期/ m))。秋分前后的平均λz *值为14.8 km,比春分前后的平均16.8 km低。 T *的年平均为23.5小时。联合(m,ω)光谱不可分离的事实,以及在m个光谱斜率中发现的较大变异性,与线性不稳定性理论不兼容,但与多普勒扩散理论和扩散滤波理论兼容。

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