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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 studies requires precise knowledge of error characteristics. We present results of an empirical error analysis of GPS RO bending angle, refractivity, dry pressure, dry geopotential height, and dry temperature. We find very good agreement 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 0.3percent in bending angle, 0.1percent in refractivity, and 0.2 K in dry temperature at all altitude levels between 4 km and 35 km. Above 35 km the increase of the CHAMP raw bending angle observational error is more pronounced than that of GRACE-A and F3C leading to a larger observational error of about 1percent at 42 km. Above approx=20 km, the observational errors show a strong seasonal dependence at high latitudes. Larger errors occur in hemispheric wintertime and are associated mainly with background data used in the retrieval process particularly under conditions when ionospheric residual is large. The comparison between UCAR and WEGC results (both data centers have independent inversion processing chains) reveals different magnitudes of observational errors in atmospheric parameters, which are attributable to different background fields used. Based on the empirical error estimates, we provide a simple analytical error model for GPS RO atmospheric parameters for the altitude range of 4 km to 35 km and up to 50 km for UCAR raw bending angle and refractivity. In the model, which accounts for vertical, latitudinal, and seasonal variations, a constant error is adopted around the tropopause region amounting to 0.8percent for bending angle, 0.35percent for refractivity, 0.15percent for dry pressure, 10 m for dry geopotential height, and 0.7 K for dry temperature. Below this region the observational error increases following an inverse height power-law and above it increases exponentially. For bending angle and refractivity we also include formulations for error correlations in order to enable modeling of full error covariance matrices for these primary data assimilation variables. The observational error model is the same for UCAR and WEGC data but due to somewhat different error characteristics below about 10 km and above about 20 km some parameters have to be adjusted. Overall, the observational error model is easily applicable and adjustable to individual error characteristics.
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弯曲角度,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))的数据特征之间有很好的一致性。在全球平均值中,在4 km至35 km之间的所有海拔高度上,观测误差(与平均切点位置处“真实”轮廓的标准偏差)一致,弯曲角度在0.3%以内,折射率在0.1%以内,干燥温度在0.2 K以内。在35 km以上,CHAMP原始弯曲角观测误差的增加比GRACE-A和F3C更为明显,导致42 km处的观测误差更大,约为1%。在大约= 20 km以上,观测误差显示出在高纬度地区强烈的季节依赖性。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,尤其是在电离层残留量较大的情况下。 UCAR和WEGC结果(两个数据中心都有独立的反演处理链)之间的比较表明,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,该模型的海拔范围为4 km至35 km,UCAR原始弯曲角和折射率最高为50 km。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,弯曲角度为0.8%,折射率为0.35%,干压为0.15%,干地势高度为10 m,干燥温度为0.7K。在该区域以下,观测误差遵循反高度幂律,并且在其之上呈指数增长。对于弯曲角和折射率,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模完整误差协方差矩阵。对于UCAR和WEGC数据,观测误差模型是相同的,但是由于误差特性在大约10 km以下和大约20 km以上有些不同,因此必须调整一些参数。总体而言,观测误差模型很容易适用,并可针对单个误差特征进行调整。

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