首页> 外文期刊>Journal of Geophysical Research. Biogeosciences >OBSERVING EARTHS ATMOSPHERE WITH RADIO OCCULTATION MEASUREMENTS USING THE GLOBAL POSITIONING SYSTEM
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OBSERVING EARTHS ATMOSPHERE WITH RADIO OCCULTATION MEASUREMENTS USING THE GLOBAL POSITIONING SYSTEM

机译:使用全球定位系统通过无线电测量测量来观测大气中的大气

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The implementation of the Global Positioning System (GPS) network of satellites and the development of small, high-performance instrumentation to receive GPS signals have created an opportunity for active remote sounding of the Earth's atmosphere by radio occultation at comparatively low cost. A prototype demonstration of this capability has now been provided by the GPS/MET investigation. Despite using relatively immature technology, GPS/MET has been extremely successful [Ware et al., 1996; Kursinski et al., 1996], although there is still room for improvement. The aim of this paper is to develop a theoretical estimate of the spatial coverage, resolution, and accuracy that can be expected for atmospheric profiles derived from GPS occultations. We consider observational geometry, attenuation, and diffraction in defining the vertical range of the observations and their resolution. We present the first systematic, extensive error analysis of the spacecraft radio occultation technique using a combination of analytical and simulation methods to establish a baseline accuracy for retrieved profiles of refractivity, geopotential, and temperature. Typically, the vertical resolution of the observations ranges from 0.5 km in the lower troposphere to 1.4 km in the middle atmosphere. Results indicate that useful profiles of refractivity can be derived from similar to 60 km altitude to the surface with the exception of regions less than 250 m in vertical extent associated with high vertical humidity gradients. Above the 250 K altitude level in the troposphere, where the effects of water are negligible, sub-Kelvin temperature accuracy is predicted up to similar to 40 km depending on the phase of the solar cycle. Geopotential heights of constant pressure levels are expected to be accurate to similar to 10 m or better between 10 and 20 km altitudes. Below the 250 K level, the ambiguity between water and dry atmosphere refractivity becomes significant, and temperature accuracy is degraded. Deep in the warn troposphere the contribution of water to refractivity becomes sufficiently large for the accurate retrieval of water vapor given independent temperatures from weather analyses [Kursinski et al., 1995]. The radio occultation technique possesses a unique combination of global coverage, high precision, high vertical resolution, insensitivity to atmospheric particulates, and long-term stability. We show here how these properties are well suited for several applications including numerical weather prediction and long-term monitoring of the Earth's climate. [References: 99]
机译:卫星全球定位系统(GPS)网络的实施以及接收GPS信号的小型高性能仪器的开发为通过无线电掩星以相对较低的成本主动远程探测地球大气创造了机会。 GPS / MET调查现已提供了此功能的原型演示。尽管使用了相对不成熟的技术,GPS / MET还是非常成功的[Ware et al。,1996; Kursinski et al。,1996],尽管仍有改进的空间。本文的目的是对从GPS掩星获得的大气廓线进行空间覆盖,分辨率和精度的理论估算。在定义观测值的垂直范围及其分辨率时,我们考虑了观测值的几何形状,衰减和衍射。我们介绍了航天器无线电掩星技术的第一个系统的,广泛的误差分析,它使用分析和模拟方法的组合来为检索到的折射率,地势和温度剖面建立基线精度。通常,观测值的垂直分辨率范围从对流层较低的0.5 km到中层大气的1.4 km。结果表明,有用的折射率分布可以从接近60 km的海拔高度得出,但与高垂直湿度梯度相关的垂直范围小于250 m的区域除外。在对流层的250 K海拔高度之上,水的影响可以忽略不计,根据太阳周期的相位,预测的开尔文温度精度可达40 km。在10至20 km高度之间,恒定压力水平的地势高度有望精确到10 m或更高。低于250 K时,水和干燥大气折射率之间的模糊性变得很明显,并且温度精度降低。在对流层的深处,给定来自天气分析的独立温度,水对折射率的贡献就变得足够大,可以准确地恢复水汽[Kursinski et al。,1995]。无线电掩星技术具有全球覆盖范围,高精度,高垂直分辨率,对大气微粒不敏感以及长期稳定性的独特组合。我们在这里展示这些特性如何很好地适合几种应用,包括数值天气预报和对地球气候的长期监测。 [参考:99]

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