奥里萨邦Subarnarekha盆地洪水易感性的比较机器学习

IF 1.9 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS
Pritee Krishna Das, Rajiv Lochan Sahu, Prakash Chandra Swain
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引用次数: 0

摘要

洪水对生态平衡、基础设施和社会经济稳定构成重大威胁,强调了准确的洪水易感性模型对有效备灾和减灾的必要性。本研究评估了五种机器学习(ML)算法——逻辑回归(LR)、k近邻(KNN)、AdaBoost、XGBoost和人工神经网络(ANN)——在奥里萨邦Subarnarekha河流域洪水易感性预测中的性能。使用包含季风季节气象和水文变量的30年数据集,使用既定指标(如接收者工作特征曲线下面积(AUC-ROC))评估模式性能。结果表明,人工神经网络的AUC-ROC最高(0.87),具有较强的分类能力,而Logistic回归(0.86)和XGBoost(0.85)也表现出较强的预测能力。研究结果强调了选择合适的ML模型进行洪水风险评估的重要性,并表明整合其他环境因素和优化超参数可以进一步提高预测精度。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Comparative machine learning for flood susceptibility in Subarnarekha Basin, Odisha
Floods present significant threats to ecological balance, infrastructure, and socioeconomic stability, underscoring the necessity of accurate flood susceptibility modeling for effective disaster preparedness and mitigation. This study evaluates the performance of five machine learning (ML) algorithms—Logistic Regression (LR), K-Nearest Neighbours (KNN), AdaBoost, XGBoost, and Artificial Neural Networks (ANN)—for flood susceptibility prediction in the Subarnarekha River Basin, Odisha. Using a 30-year dataset comprising meteorological and hydrological variables from the monsoon season, model performance was assessed using established metrics such as Area Under the Receiver Operating Characteristic Curve (AUC-ROC). The results indicate that ANN achieved the highest AUC-ROC (0.87), demonstrating superior classification capability, while Logistic Regression (0.86) and XGBoost (0.85) also exhibited strong predictive performance. The findings highlight the importance of selecting appropriate ML models for flood risk assessment and suggest that integrating additional environmental factors and optimizing hyperparameters could further enhance prediction accuracy.
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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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