莫斯科城市热岛时空变化的机器学习逼近

IF 0.4 4区 物理与天体物理 Q4 PHYSICS, MULTIDISCIPLINARY
M. I. Varentsov, M. A. Krinitskiy, V. M. Stepanenko
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引用次数: 0

摘要

本研究以莫斯科特大城市为例,致力于应用机器学习(ML)方法对城市温度异常(称为城市热岛(UHI))及其时空动态进行统计近似。这项任务被认为是一个更普遍的问题的一部分,即根据城市条件统计降低气象场的尺度。因此,我们的目标是基于表征低分辨率气象数据和高分辨率地表特性的预测因子来近似一个高分辨率的城市温度异常场。我们使用COSMO区域大气模式和TERRA_URB城市冠层参数化对莫斯科地区气象状况进行的高分辨率水动力模拟结果作为训练ML模型的输入数据。对于机器学习模型,我们使用了由GPU支持的CatBoost算法实现的梯度增强方法。为了解释UHI和表面性质之间的非局部依赖关系,我们使用原始的准局部方法来定义特征向量。该方法包括使用定位于单个点(COSMO模型计算网格的节点)的数据作为特征描述,并使用不同类型的卷积过滤器基于相邻点的预测器值生成附加特征。作为这样的滤波器,我们使用具有不同半径的圆形核的移动平均线和更先进的自调整方向滤波器,这些滤波器是通过考虑大规模的风速和风向数据而形成的。研究表明,这些非局地特征对于正确再现城市热岛空间结构的关键格局非常重要,特别是与地表特征相比,季节平均温度异常的结构更平滑,以及在不同风向的特定情况下温度异常向城市背风侧的转移。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Approximation of Spatial and Temporal Variability of the Urban Heat Island in Moscow Using Machine Learning

Approximation of Spatial and Temporal Variability of the Urban Heat Island in Moscow Using Machine Learning

This study is devoted to the application of machine learning (ML) methods for statistical approximation of the urban-induced temperature anomaly, known as the urban heat island (UHI), and its spatiotemporal dynamics, using the example of the Moscow megacity. This task is considered as part of a more general problem of statistical downscaling of meteorological fields for urban conditions. Therefore, we aim to approximate a high-resolution field of urban temperature anomalies based on predictors characterizing low-resolution meteorological data and high-resolution surface properties. As the input data for training ML models, we use the results of high-resolution hydrodynamic simulations of the meteorological regime in the Moscow region conducted with the COSMO regional atmospheric model coupled with the TERRA_URB urban canopy parameterization. For the ML model, we use the gradient boosting method implemented by the CatBoost algorithm with GPU support. To account for nonlocal dependences between UHI and surface properties, we use an original quasi-local approach to define the feature vectors. This approach consists of using data localized at individual points (nodes of the computational mesh of the COSMO model) as feature descriptions and generating additional features based on the predictors’ values for neighboring points using different types of convolution filters. As such filters, we use a moving average with a circular kernel of different radii and more advanced self-adjusting directional filters formed by taking into account large-scale data on wind speed and direction. We show that such nonlocal features are important for correctly reproducing the key patterns of the UHI spatial structure, in particular the smoother structure of seasonally-averaged temperature anomalies in comparison to surface properties, and the shift of temperature anomalies to the leeward side of the city for specific cases with different wind directions.

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来源期刊
Moscow University Physics Bulletin
Moscow University Physics Bulletin PHYSICS, MULTIDISCIPLINARY-
CiteScore
0.70
自引率
0.00%
发文量
129
审稿时长
6-12 weeks
期刊介绍: Moscow University Physics Bulletin publishes original papers (reviews, articles, and brief communications) in the following fields of experimental and theoretical physics: theoretical and mathematical physics; physics of nuclei and elementary particles; radiophysics, electronics, acoustics; optics and spectroscopy; laser physics; condensed matter physics; chemical physics, physical kinetics, and plasma physics; biophysics and medical physics; astronomy, astrophysics, and cosmology; physics of the Earth’s, atmosphere, and hydrosphere.
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