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Empirical analysis and modeling of errors of atmospheric profiles from GPS radio occultation

机译:GPS无线电掩星对大气廓线误差的实证分析与建模

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The utilization of radio occultation (RO) data in atmospheric studiesrequires precise knowledge of error characteristics. We present results ofan empirical error analysis of GPS RO bending angle, refractivity, drypressure, dry geopotential height, and dry temperature. We find very goodagreement between data characteristics of different missions (CHAMP,GRACE-A, and Formosat-3/COSMIC (F3C)).In the global mean, observational errors (standard deviation from "true"profiles at mean tangent point location) agree within 0.3% in bendingangle, 0.1% in refractivity, and 0.2 K in dry temperature at allaltitude levels between 4 km and 35 km.Above 35 km the increase of the CHAMP raw bending angle observationalerror is more pronounced than that of GRACE-A and F3C leading to alarger observational error of about 1% at 42 km. Above ≈20 km,the observational errors show a strong seasonal dependence at highlatitudes. Larger errors occur in hemispheric wintertime and are associatedmainly with background data used in the retrieval process particularlyunder conditions when ionospheric residual is large. The comparison betweenUCAR and WEGC results (both data centers have independent inversionprocessing chains) reveals different magnitudes of observational errors inatmospheric parameters, which are attributable to different backgroundfields used. Based on the empirical error estimates, we provide a simpleanalytical error model for GPS RO atmospheric parameters for the altituderange of 4 km to 35 km and up to 50 km for UCAR raw bending angle andrefractivity. In the model, which accounts for vertical, latitudinal, andseasonal variations, a constant error is adopted around the tropopauseregion amounting to 0.8% for bending angle, 0.35% for refractivity,0.15% for dry pressure, 10 m for dry geopotential height, and 0.7 Kfor dry temperature. Below this region the observational error increasesfollowing an inverse height power-law and above it increasesexponentially.For bending angle and refractivity we also include formulations for errorcorrelations in order to enable modeling of full error covariance matricesfor these primary data assimilation variables.The observational error model is the same for UCAR and WEGC data but due tosomewhat different error characteristics below about 10 km and above about20 km some parameters have to be adjusted. Overall, the observationalerror model is easily applicable and adjustable to individual errorcharacteristics.
机译:在大气研究中利用无线电掩星(RO)数据需要精确了解误差特征。我们提出了GPS RO弯曲角,折射率,干压,干地势高度和干温度的经验误差分析结果。我们发现不同任务(CHAMP,GRACE-A和Formosat-3 / COSMIC(F3C))的数据特征之间有着很好的一致性。在整体平均值上,观测误差(在平均切点位置与“真实”轮廓的标准偏差)一致在4 km至35 km高度范围内,弯曲角度误差在0.3%以内,折射率在0.1%以内,干燥温度为0.2 K.在35 km以上,CHAMP原始弯曲角度观测误差的增加比GRACE-A和F3C更为明显导致42公里处的观测误差更大,约为1%。在≈20 km以上,观测误差在高纬度地区表现出强烈的季节依赖性。较大的误差发生在半球冬季,主要与检索过程中使用的背景数据有关,特别是在电离层残留较大的情况下。 UCAR和WEGC结果(两个数据中心都有独立的反演处理链)之间的比较显示,大气参数的观测误差幅度不同,这可归因于所使用的不同背景场。基于经验误差估计,我们为GPS RO大气参数提供了一个简单的分析误差模型,该模型在4 km至35 km的海拔范围内以及对于UCAR原始弯曲角和折射率的最大50 km范围内。在考虑垂直,纬度和季节变化的模型中,对流层顶区域周围采用恒定误差,折角为0.8%,折射率为0.35%,干压为0.15%,干地势高度为10 m,0.7干燥温度。在该区域以下,观察误差遵循反高度幂律而增加,在其上方则呈指数增加。对于弯曲角度和折射率,我们还包括误差相关公式,以便能够为这些主要数据同化变量建立完整的误差协方差矩阵。对于UCAR和WEGC数据相同,但是由于在大约10 km以下和大约20 km以上的误差特性有所不同,因此必须调整一些参数。总体而言,观察误差模型很容易适用于个人的误差特征,并可对其进行调整。

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