...
首页> 外文期刊>Geoscientific Model Development Discussions >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
【24h】

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实验(CAPTEX)观测的弱约束反向建模 - 包括模型不确定性在源期估算中的效果

获取原文
           

摘要

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:使用从六个中收集的跨阿巴拉契亚示踪实验(CAPTEX)数据评估基于变分数据同化和拉格朗日色散传递系数矩阵(TCM)的混合单粒子拉格朗日集成轨迹版本4(HYSPLIT-4)逆系统控制版本。为简单起见,初始测试应用于第2版,Hysplit具有最佳性能。在引入模型的不确定条件之前,将随着源估计变为源估计,使用浓度差异的测试在成本函数中导致严重低估,而使用对数浓度差异的人会导致释放速率的高估。添加模型不确定性术语可提高成本函数中度量变量的两种选择的结果。稍后引入了成​​本函数规范化方案以避免使用对数浓度差异时的杂散最小源术语解决方案。该方案有效地消除了杂散的解决方案,并且还有助于改善度量变量选择的释放估计。该测试还表明,计算对数浓度差异通常比计算浓度差异更好地产生,并且对于合理的模型不确定参数来说,估计更加坚固。通过九个集合Hysplit进行进一步证实,其中产生气象场,其具有不同的行星边界层(PBL)方案。另外,发现使用组合的TCM通过采用九个TCMS的平均值的发射估计与使用每个TCMS单独使用的九个估计的中值类似。然后将逆系统应用于具有固定的观察和模型不确定性参数的其他CAPTEX释放,并且六个释放中的最大相对误差为53.3%。最后,测试系统的能力以找到单个源位置以及其源极度。在这些测试中,产生预测和观察到的浓度之间最佳匹配的位置和强度被认为是逆建模结果。估计的释放速率主要不如已知确切释放位置的情况一样好,但它们全部在3倍的范围内为所有六个释放。然而,估计的位置可能具有大的错误。

著录项

获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号