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Tropospheric jet stream as a source of traveling ionospheric disturbances observed by GPS

机译:对流层射流是GPS观测到的电离层行进干扰源

摘要

The integrity and the reliability of real-time precise positioning applications with Global Positioning System (GPS) are affected by the ionospheric variability with time and space. As a consequence, scientific community aims at describing, explaining and forecasting the occurrence and the amplitude of ionospheric irregularities observed by GPS. The use of the geometric-free combination of GPS dual frequency signals allows to retrieve the Total Electron Content (TEC) along the satellite-to-receiver path, which is the basic trans-ionospheric observable. Based on L1/L2 GPS phase measurements collected at a given station, the TEC high-frequency variability is isolated. A climatological study performed over 10 years in Western Europe shows that TEC irregularities are mostly observed daytime during quiet geomagnetic background in autumn and winter and correspond to classical Medium-Scale Traveling Ionospheric Disturbances (MSTIDs). The latter are generally understood as the ionospheric signature of Atmospheric Gravity Waves (AGWs), either generated in situ (solar terminator) or in the lower atmosphere and propagating upward. Because of its associated strong wind shears, the tropospheric jetstream, occurring mainly during autumn and winter months, constitutes an ideal candidate for AGW generation. This paper analyzes the spatial correlation between the presence of both MSTIDs and strong jetstream over Western Europe. This correlation is positive when the ionospheric pierce point of the satellite is located above regions of interest where wind shears are very large. In practice, we have selected regions for which wind speed is larger than 50 m/s. In addition, the propagation of AGWs up to the ionospheric layer is taken into account by assuming horizontal and vertical velocities of 200 and 50 m/s respectively. It comes that the region of interest of the correlation study is computed using an isotropic slant propagation of the AGW, which is supposed to be generated at a tropospheric level.Based on 30s GPS data collected over several stations in Belgium and on European Centre for Medium-Range Weather Forecasts (ECMWF) wind velocity maps, the correlation study covers a period ranging from January 2002 to December 2011. Preliminary results based on a limited number of cases show that large amplitude MSTIDs are generally observed during periods of strong wind speeds at an altitude corresponding to a pressure level of 250hPa (about 10 km).
机译:电离层随时间和空间的变化会影响全球定位系统(GPS)实时精确定位应用程序的完整性和可靠性。因此,科学界旨在描述,解释和预测GPS观测到的电离层不规则现象的发生和幅度。 GPS双频信号的无几何组合的使用允许沿卫星到接收器的路径检索总电子含量(TEC),这是基本的跨电离层观测。根据在给定站点收集的L1 / L2 GPS相位测量值,可以隔离TEC高频变化。在西欧进行了超过10年的气候研究,结果表明,TEC的不规则性大多发生在秋季和冬季安静的地磁背景下的白天,这与经典的中等规模电离层扰动(MSTIDs)相符。后者通常被理解为原地(太阳能终结者)或在低层大气中向上传播的大气重力波(AGW)的电离层特征。由于其相关的强风切变,对流层急流主要发生在秋季和冬季,是AGW发电的理想选择。本文分析了MSTID的存在与西欧强射流之间的空间相关性。当卫星的电离层穿刺点位于风切变很大的目标区域上方时,这种相关性为正。实际上,我们选择了风速大于50 m / s的区域。另外,通过假设水平和垂直速度分别为200和50 m / s,考虑了AGW到电离层的传播。结果表明,相关研究的关注区域是使用AGW的各向同性倾斜传播来计算的,该传播应该是在对流层水平上产生的。基于比利时多个站点和欧洲中空中心收集的30年代GPS数据-Range Weather Forecasts(ECMWF)风速图,相关研究涵盖了从2002年1月到2011年12月的一段时间。基于数量有限的案例的初步结果显示,在强风速下,通常会观察到大振幅的MSTID。对应于250hPa(约10 km)压力水平的高度。

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