在Poly-ZWD经验模式中使用集合卡尔曼滤波同化美国天顶湿延迟观测

IF 1.9 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS
Masoud Dehvari , Saeed Farzaneh , Ehsan Forootan
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引用次数: 0

摘要

模拟低层大气中水汽的时空变化对气象和大地测量应用至关重要,因为它直接影响天气预报和卫星定位。然而,传统的经验模型往往难以捕捉水汽的快速波动,限制了它们的准确性和实用性。这些模型通常也是基于网格的,并且涉及许多参数,使得针对当前观测的实时校准具有挑战性。为了解决这些局限性,本研究采用了基于集成卡尔曼滤波(Ensemble Kalman Filter, EnKF)的集成校准和数据同化(C/DA)方法,该方法根据观测数据顺序调整模型参数,从而提高了短期预测精度。具体来说,我们通过开发一个区域经验模型Poly-ZWD来增强对天顶湿延迟(ZWD)的估计。该模型采用三阶多项式来表示水平变化,因为它们可以用更少的系数灵活地捕捉空间趋势,而b样条函数用于时间变化,因为它们具有紧凑的支持和强大的局部控制,从而实现平滑和高效的时间相关建模。该模型采用2016 - 2020年ERA5再分析数据构建。Poly-ZWD横跨美国(27°-49°N, 94°-68°W),包含680个参数,这些参数共同捕获了整个区域ZWD的时空行为。这些参数使用来自美国460个站点的gnss衍生的ZWD观测数据进行了重新校准,与原始PCA-ZWD衍生系数相比,改善了与真实大气条件的一致性,提高了模型的性能。重新校准的模型被称为C/DA Poly-ZWD,与来自15个独立GNSS测试站和7个无线电探空站点的ZWD估计进行了评估。结果表明,该模型的均方根误差(RMSE)约为1.1 cm,优于ERA5和GTrop模型。虽然在24小时预测范围内RMSE从1.1 cm逐渐增加到约6 cm,但与考虑的经验模型相比,校准模型始终保持更高的精度。值得注意的是,C/DA方法在3小时的预测窗口内提供了比ERA5更准确的短期ZWD预测。这些发现强调了基于集成的C/DA技术在增强实时ZWD建模能力方面的有效性,并有望提高基于gnss的定位精度和短期天气预报。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Assimilation of Zenith Wet Delay observations using the ensemble Kalman Filter in a Poly-ZWD empirical model over the USA
Modeling the spatial and temporal variability of water vapor in the lower atmosphere is crucial for meteorological and geodetic applications, as it directly influences weather prediction and satellite-based positioning. However, traditional empirical models often struggle to capture rapid water vapor fluctuations, limiting their accuracy and practical utility. These models are also typically grid-based and involve numerous parameters, making real-time calibration against current observations challenging. To address these limitations, this study applies an ensemble-based Calibration and Data Assimilation (C/DA) approach using the Ensemble Kalman Filter (EnKF), which sequentially adjusts model parameters based on observational data, thereby improving short-term prediction accuracy. Specifically, we enhance the estimation of Zenith Wet Delay (ZWD) through the development of a regional empirical model, Poly-ZWD. This model employs third-order polynomials for horizontal variations due to their flexibility in capturing spatial trends with fewer coefficients, and B-spline functions for temporal variations because of their compact support and strong local control, which enable smooth and efficient time-dependent modeling. The model was built using ERA5 reanalysis data from 2016 to 2020. Poly-ZWD spans the contiguous United States (27°–49°N, 94°–68°W) and incorporates 680 parameters, which collectively capture the spatial and temporal behavior of ZWD across the domain. These parameters were recalibrated using GNSS-derived ZWD observations from 460 stations across the U.S. for the year 2021, improving alignment with real-world atmospheric conditions and enhancing model performance compared to the original PCA-ZWD derived coefficients. The recalibrated model, referred to as C/DA Poly-ZWD, was evaluated against ZWD estimates from 15 independent GNSS test stations and 7 radiosonde sites. Results show that the proposed model achieves a root mean square error (RMSE) of approximately 1.1 cm, outperforming both ERA5 and GTrop models. While RMSE increases gradually from 1.1 cm to around 6 cm over a 24-h forecast horizon, the calibrated model consistently maintains superior accuracy compared to the considered empirical models. Notably, the C/DA approach provides more accurate short-term ZWD predictions than ERA5 within a 3-h forecast window. These findings highlight the effectiveness of ensemble-based C/DA techniques in enhancing real-time ZWD modeling capabilities, with promising implications for improving GNSS-based positioning accuracy and short-term weather forecasting.
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来源期刊
Journal of Atmospheric and Solar-Terrestrial Physics
Journal of Atmospheric and Solar-Terrestrial Physics 地学-地球化学与地球物理
CiteScore
4.10
自引率
5.30%
发文量
95
审稿时长
6 months
期刊介绍: The Journal of Atmospheric and Solar-Terrestrial Physics (JASTP) is an international journal concerned with the inter-disciplinary science of the Earth''s atmospheric and space environment, especially the highly varied and highly variable physical phenomena that occur in this natural laboratory and the processes that couple them. The journal covers the physical processes operating in the troposphere, stratosphere, mesosphere, thermosphere, ionosphere, magnetosphere, the Sun, interplanetary medium, and heliosphere. Phenomena occurring in other "spheres", solar influences on climate, and supporting laboratory measurements are also considered. The journal deals especially with the coupling between the different regions. Solar flares, coronal mass ejections, and other energetic events on the Sun create interesting and important perturbations in the near-Earth space environment. The physics of such "space weather" is central to the Journal of Atmospheric and Solar-Terrestrial Physics and the journal welcomes papers that lead in the direction of a predictive understanding of the coupled system. Regarding the upper atmosphere, the subjects of aeronomy, geomagnetism and geoelectricity, auroral phenomena, radio wave propagation, and plasma instabilities, are examples within the broad field of solar-terrestrial physics which emphasise the energy exchange between the solar wind, the magnetospheric and ionospheric plasmas, and the neutral gas. In the lower atmosphere, topics covered range from mesoscale to global scale dynamics, to atmospheric electricity, lightning and its effects, and to anthropogenic changes.
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