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Response of GPS occultation signals to atmospheric gravity waves and retrieval of gravity wave parameters

机译:GPS掩星信号对大气重力波的响应及重力波参数的获取

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We show that the amplitude of the Global Positioning System (GPS) signals in the radio occultation (RO) experiments is an indicator of the activity of the gravity waves (GW) in the atmosphere. The amplitude of the GPS RO signals is more sensitive to the atmospheric wave structures than is the phase. Early investigations used only the phase of the GPS occultation signals for statistical investigation of the GW activity in the height interval 10–40 km on a global scale. In this study, we use the polarization equations and Hilbert transform to find the 1-D GW radio image in the atmosphere by analyzing the amplitude of the RO signal. The radio image, also called the GW portrait, consists of the phase and amplitude of the GW as functions of height. We demonstrate the potential of this method using the amplitude data from GPS/Meteorology (GPS/MET) and satellite mission Challenge Mini-satellite Payload (CHAMP) RO events. The GW activity is nonuniformly distributed with the main contribution associated with the tropopause and the secondary maximums related to the GW breaking regions. Using our method we find the vertical profiles of the horizontal wind perturbations and its vertical gradient associated with the GW influence. The estimated values of the horizontal wind perturbations are in fairly good agreement with radiosonde data. The horizontal wind perturbations v(h) are ±1 to ±5 m s with vertical gradients dv/dh ±0.5 to ±15 m s km at height 10–40 km. The height dependence of the GW vertical wavelength was inferred through the differentiation of the GW phase. Analysis of this dependence using the dispersion relationship for the GW gives the estimation of the projection of the horizontal background wind velocity on the direction of the GW propagation. For the event considered, the magnitude of this projection changes between 1.5 and 10 m s at heights of 10–40 km. We conclude that the amplitude of the GPS occultation signals contain important information about the wave processes in the atmosphere on a global scale.
机译:我们显示,在无线电掩星(RO)实验中,全球定位系统(GPS)信号的幅度是大气中重力波(GW)活动的指标。 GPS RO信号的幅度比相位对大气波结构更敏感。早期调查仅将GPS掩星信号的相位用于全球规模10-40 km高度区间的GW活动的统计调查。在这项研究中,我们使用极化方程和希尔伯特变换,通过分析RO信号的幅度来找到大气中的一维GW无线电图像。无线电图像,也称为GW肖像,由GW的相位和幅度作为高度的函数组成。我们使用来自GPS /气象(GPS / MET)和卫星任务挑战小型卫星有效载荷(CHAMP)RO事件的振幅数据证明了该方法的潜力。 GW活动是不均匀分布的,其主要贡献与对流层顶相关,而次要最大值与GW破裂区域有关。使用我们的方法,我们发现了水平风扰动的垂直剖面及其与GW影响相关的垂直梯度。水平风扰动的估计值与无线电探空仪数据相当吻合。在高度10–40 km处,水平风扰动v(h)为±1至±5 m s,垂直梯度dv / dh为±0.5至±15 m s km。 GW垂直波长的高度依赖性是通过GW相的微分来推断的。使用GW的色散关系对此依赖性进行分析,可以估算出水平背景风速在GW传播方向上的投影。对于所考虑的事件,在10–40 km的高度,该投影的大小在1.5至10 m s之间变化。我们得出的结论是,GPS掩星信号的幅度包含有关全球范围内大气中波过程的重要信息。

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