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Wave-optics uncertainty propagation and regression-based bias model in GNSS radio occultation bending angle retrievals

机译:GNSS无线电掩星弯曲角检索中基于波光学不确定性传播和基于回归的偏差模型

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摘要

A new reference occultation processing system (rOPS) will include a GlobalNavigation Satellite System (GNSS) radio occultation (RO) retrieval chainwith integrated uncertainty propagation. In this paper, we focus onwave-optics bending angle (BA) retrieval in the lower troposphere and introduce(1) an empirically estimated boundary layer bias (BLB) model then employed toreduce the systematic uncertainty of excess phases and bending angles in about thelowest 2 km of the troposphere and (2) the estimation of(residual) systematic uncertainties and their propagation together withrandom uncertainties from excess phase to bending angle profiles. Our BLBmodel describes the estimated bias of the excess phase transferred from theestimated bias of the bending angle, for which the model is built, informedby analyzing refractivity fluctuation statistics shown to induce such biases.The model is derived from regression analysis using a large ensemble ofConstellation Observing System for Meteorology, Ionosphere, and Climate(COSMIC) RO observations and concurrent European Centre for Medium-RangeWeather Forecasts (ECMWF) analysis fields. It is formulated interms of predictors and adaptive functions (powers and cross products of predictors),where we use six main predictors derived from observations: impact altitude,latitude, bending angle and its standard deviation, canonical transform (CT)amplitude, and its fluctuation index. Based on an ensemble of test days,independent of the days of data used for the regression analysis to establishthe BLB model, we find the model very effective for bias reduction and capableof reducing bending angle and corresponding refractivity biases by about afactor of 5. The estimated residual systematic uncertainty, after the BLBprofile subtraction, is lower bounded by the uncertainty from the (indirect) useof ECMWF analysis fields but is significantly lower than the systematicuncertainty without BLB correction. The systematic and random uncertaintiesare propagated from excess phase to bending angle profiles, using aperturbation approach and the wave-optical method recently introduced byGorbunov and Kirchengast (2015), starting with estimated excess phaseuncertainties. The results are encouraging and this uncertainty propagationapproach combined with BLB correction enables a robust reduction andquantification of the uncertainties of excess phases and bending angles inthe lower troposphere.
机译:新的参考掩星处理系统(rOPS)将包括具有集成不确定性传播的全球导航卫星系统(GNSS)无线电掩星(RO)检索链。在本文中,我们将重点放在对流层下层的波波弯曲角(BA)检索上,并介绍(1)根据经验估算的边界层偏置(BLB)模型,然后采用该模型来减小大约2的最小相位和弯曲角的系统不确定性对流层公里数(2)(剩余)系统不确定性及其传播的估计以及从不确定相位到弯曲角度剖面的随机不确定性。我们的BLB模型描述了从弯曲角度的估计偏差转移过来的过剩相位的估计偏差,为此模型建立了模型,并通过分析表明会导致这种偏差的折射率波动统计信息进行了建模。该模型是通过使用大型星座观测的整体回归分析得出的气象,电离层和气候系统(COSMIC)RO观测,以及欧洲中距离天气预报中心(ECMWF)分析领域。它由预测变量和自适应函数(预测变量的乘方和叉积)组成,在这里我们使用从观测中得出的六个主要预测变量:撞击高度,纬度,弯曲角度及其标准偏差,规范变换(CT)幅度及其波动指数。基于测试天数的集合,与用于建立BLB模型的回归分析的数据天数无关,我们发现该模型对于减小偏差非常有效,并且能够将弯曲角度和相应的折射率偏差减小大约5倍。在减去BLB轮廓后,残留的系统不确定性受到(间接)使用ECMWF分析字段的不确定性的下限限制,但比未进行BLB校正的系统不确定性要低得多。系统的和随机的不确定性从超相位传播到弯曲角轮廓,使用扰动方法和最近由Gorbunov和Kirchengast(2015)引入的波动光学方法,从估计的超相位不确定性开始。结果令人鼓舞,并且这种不确定性传播方法与BLB校正相结合,可以有效地降低和量化对流层下部多余相位和弯曲角度的不确定性。

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