首页> 外文期刊>Radio Science >Meteor radar wind over Chung-Li (24.9°N, 121°E), Taiwan, for the period 10-25 November 2012 which includes Leonid meteor shower: Comparison with empirical model and satellite measurements
【24h】

Meteor radar wind over Chung-Li (24.9°N, 121°E), Taiwan, for the period 10-25 November 2012 which includes Leonid meteor shower: Comparison with empirical model and satellite measurements

机译:2012年11月10日至25日,台湾中-(24.9°N,121°E)上的流星雷达风,包括狮子座流星雨:与经验模型和卫星测量值的比较

获取原文
获取原文并翻译 | 示例
           

摘要

The neutral winds in the mesosphere and lower thermosphere (MLT) region are measured by a newly installed meteor trail detection system (or meteor radar) at Chung-Li, Taiwan, for the period 10-25 November 2012, which includes the Leonid meteor shower period. In this study, we use the 3 m field-aligned plasma irregularities in the sporadic E (E_s) region in combination with the International Geomagnetic Reference Field model to calibrate the system phase biases such that the true positions of the meteor trails can be correctly determined with interferometry technique. The horizontal wind velocities estimated from the radial velocities of the meteor trails and their locations by using a least squares method show that the diurnal tide dominates the variation of the MLT neutral wind with time over Chung-Li, which is in good agreement with the horizontal wind model (HWM07) prediction. However, harmonic analysis reveals that the amplitudes of the mean wind, diurnal, and semidiurnal tides of the radar-measured winds in height range 82-100 km are systematically larger than those of the model-predicted winds by up to a factor of 3. A comparison shows that the overall pattern of the height-local time distribution of the composite radar-measured meteor wind is, in general, consistent with that of the TIMED Doppler Interferometer-observed wind, which is dominated by a diurnal oscillation with downward phase progression at a rate of about 1.3 km/h. The occurrences of the E_s layers retrieved from fluctuations of the amplitude and excess phase of the GPS signal received by the FORMOSAT-3/COSMIC satellites during the GPS radio occultation (RO) process are compared with the shear zones of the radar-measured meteor wind and HWM07 wind. The result shows that almost all of the RO-retrieved E_s layers occur within the wind shear zones that favor the E_s layer formation based on the wind shear theory, suggesting that the primary physical process responsible for the E_s layer events retrieved from the scintillations of the GPS RO signal is very likely the plasma convergence effect of the neutral wind shear.
机译:用新安装的位于台湾中-的流星迹探测系统(或流星雷达)测量了中层和低层热层(MLT)区域的中性风,时间为2012年11月10日至25日,其中包括狮子座流星雨期。在这项研究中,我们结合零星E(E_s)区域中3 m的场对准等离子体不规则性,并结合国际地磁参考场模型来校准系统相位偏差,以便可以正确确定流星踪迹的真实位置与干涉技术。利用最小二乘法从流星径的径向速度及其位置估计的水平风速表明,在t里地区,日潮主导了MLT中性风随时间的变化,这与水平方向吻合得很好。风模型(HWM07)预测。但是,谐波分析显示,雷达测量的风在82-100 km高度范围内的平均风,日潮和半日潮的振幅比模型预测的风有系统地大3倍。比较表明,复合雷达测量的流星风的高度-局部时间分布的总体模式通常与TIMED多普勒干涉仪观测到的风一致,该模式主要由具有向下相位递进的昼夜振荡主导时速约为1.3公里/小时。将在GPS无线电掩星(RO)过程中从FORMOSAT-3 / COSMIC卫星接收到的GPS信号的幅度和过量相位的波动中获得的E_s层的出现与雷达测量的流星风的剪切带进行了比较和HWM07风。结果表明,基于风切变理论,几乎所有的RO剥蚀E_s层都在有利于E_s层形成的风切变区内发生,这表明从E.s闪烁产生的E_s层事件的主要物理过程。 GPS RO信号很可能是中性风切变的等离子收敛效应。

著录项

相似文献

  • 外文文献
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号