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Weak-constraint inverse modeling using HYSPLIT-4 Lagrangian dispersion model and Cross-Appalachian Tracer Experiment (CAPTEX) observations – effect of including model uncertainties on source term estimation

机译:使用HYSPLIT-4拉格朗日色散模型和跨阿巴拉契亚示踪剂实验(CAPTEX)观测值的弱约束逆建模–包括模型不确定性对源项估计的影响

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A Hybrid Single-Particle Lagrangian Integrated Trajectory version 4 (HYSPLIT-4) inverse system that is based on variational data assimilation and a Lagrangian dispersion transfer coefficient matrix (TCM) is evaluated using the Cross-Appalachian Tracer Experiment (CAPTEX) data collected from six controlled releases. For simplicity, the initial tests are applied to release 2, for which the HYSPLIT has the best performance. Before introducing model uncertainty terms that will change with source estimates, the tests using concentration differences in the cost function result in severe underestimation, while those using logarithm concentration differences result in overestimation of the release rate. Adding model uncertainty terms improves results for both choices of the metric variables in the cost function. A cost function normalization scheme is later introduced to avoid spurious minimal source term solutions when using logarithm concentration differences. The scheme is effective in eliminating the spurious solutions and it also helps to improve the release estimates for both choices of the metric variables. The tests also show that calculating logarithm concentration differences generally yields better results than calculating concentration differences, and the estimates are more robust for a reasonable range of model uncertainty parameters. This is further confirmed with nine ensemble HYSPLIT runs in which meteorological fields were generated with varying planetary boundary layer (PBL) schemes. In addition, it is found that the emission estimate using a combined TCM by taking the average or median values of the nine TCMs is similar to the median of the nine estimates using each of the TCMs individually. The inverse system is then applied to the other CAPTEX releases with a fixed set of observational and model uncertainty parameters, and the largest relative error among the six releases is 53.3?%. At last, the system is tested for its capability to find a single source location as well as its source strength. In these tests, the location and strength that yield the best match between the predicted and the observed concentrations are considered as the inverse modeling results. The estimated release rates are mostly not as good as the cases in which the exact release locations are assumed known, but they are all within a factor of 3 for all six releases. However, the estimated location may have large errors.
机译:混合单粒子拉格朗日综合轨迹版本4(HYSPLIT-4)逆系统基于变分数据同化和拉格朗日色散传递系数矩阵(TCM),使用从六个地点收集的跨阿巴拉契亚示踪实验(CAPTEX)数据进行评估受控释放。为简单起见,初始测试适用于HYSPLIT具有最佳性能的版本2。在引入将随源估计而变化的模型不确定性术语之前,使用成本函数中浓度差异的测试会导致严重低估,而使用对数浓度差异的测试则会导致释放率高估。添加模型不确定性项可以改善成本函数中两个度量变量的选择结果。稍后引入成本函数归一化方案,以避免在使用对数浓度差时出现虚假的最小源项解决方案。该方案可有效消除杂散解,并且还有助于改进度量变量的两个选择的释放估计。测试还表明,计算对数浓度差通常会比计算浓度差产生更好的结果,并且对于合理范围的模型不确定性参数,估计值更可靠。九个合奏的HYSPLIT运行进一步证实了这一点,其中使用不同的行星边界层(PBL)方案生成了气象场。另外,发现通过采用九个TCM的平均值或中值使用组合TCM的排放估计类似于单独使用每个TCM的九个估计的中值。然后将反系统应用于具有固定观测值和模型不确定性参数集的其他CAPTEX版本,六个版本中最大的相对误差为53.3%。最后,测试该系统查找单个源位置的能力以及源强度。在这些测试中,在预测浓度和观察浓度之间产生最佳匹配的位置和强度被视为逆建模结果。估计的释放率大多不如假定确切的释放位置已知的情况好,但是对于所有六个释放,它们的均在三分之一以内。但是,估计的位置可能会有很大的误差。

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