首页 > 最新文献

Journal of Atmospheric and Solar-Terrestrial Physics最新文献

英文 中文
Comparative analysis of machine learning models for rainfall prediction 降雨预测机器学习模型的比较分析
IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-08-30 DOI: 10.1016/j.jastp.2024.106340

Predicting rainfall is essential for many applications, including agriculture, hydrology, and disaster management. In this work, we undertake a comparison examination of various machine learning models to forecast rainfall based on meteorological data. The target variable in this study is rainfall, and the dataset used includes characteristics like temperature, relative humidity, wind speed, and wind direction. The following seven machine learning models were assessed: Support Vector Regression (SVR), Multivariate adaptive regression splines (MARS), Random Forest Regression, and Deep Neural Network with Historical Data (DWFH), Haar Wavelet Function, Decision Tree and Discrete wavelet Transform (DWT). Data preprocessing, which includes standardisation and lagging to capture temporal dependencies, comes first in the analysis phase. A wavelet transformation is also used to capture complex patterns in the data. Each model is tested on a different test set after being trained on a subset of the dataset. The results are assessed using the Root Mean Squared Error (RMSE) and Mean Squared Error (MSE), focusing on the RMSE and MSE values for better comparison across models. Our findings reveal that the DWFH model achieved an RMSE of 0.0138807 mm and MSE of 0.000193 mm2, demonstrating their effectiveness in predicting rainfall. The Random Forest and SVR models also provided competitive results. This study highlights the importance of selecting an appropriate machine learning model for rainfall prediction and the significance of preprocessing techniques in improving model performance. These insights can aid decision-makers in choosing the most suitable model for their specific application, contributing to more accurate rainfall predictions and enhanced decision support systems.

预测降雨量对农业、水文和灾害管理等许多应用都至关重要。在这项工作中,我们对基于气象数据预测降雨的各种机器学习模型进行了比较研究。本研究的目标变量是降雨量,使用的数据集包括温度、相对湿度、风速和风向等特征。对以下七个机器学习模型进行了评估:支持向量回归(SVR)、多变量自适应回归样条(MARS)、随机森林回归、带历史数据的深度神经网络(DWFH)、哈小波函数、决策树和离散小波变换(DWT)。在分析阶段,首先要进行数据预处理,包括标准化和滞后处理,以捕捉时间依赖性。小波变换也用于捕捉数据中的复杂模式。每个模型在数据集的一个子集上进行训练后,在不同的测试集上进行测试。使用均方根误差(RMSE)和均方误差(MSE)对结果进行评估,重点关注 RMSE 和 MSE 值,以便更好地比较不同模型。我们的研究结果表明,DWFH 模型的 RMSE 为 0.0138807 毫米,MSE 为 0.000193 平方毫米,这表明它们在预测降雨量方面非常有效。随机森林和 SVR 模型也提供了有竞争力的结果。这项研究强调了选择合适的机器学习模型进行降雨预测的重要性,以及预处理技术对提高模型性能的重要意义。这些见解可以帮助决策者为其特定应用选择最合适的模型,从而提高降雨预测的准确性并增强决策支持系统。
{"title":"Comparative analysis of machine learning models for rainfall prediction","authors":"","doi":"10.1016/j.jastp.2024.106340","DOIUrl":"10.1016/j.jastp.2024.106340","url":null,"abstract":"<div><p>Predicting rainfall is essential for many applications, including agriculture, hydrology, and disaster management. In this work, we undertake a comparison examination of various machine learning models to forecast rainfall based on meteorological data. The target variable in this study is rainfall, and the dataset used includes characteristics like temperature, relative humidity, wind speed, and wind direction. The following seven machine learning models were assessed: Support Vector Regression (SVR), Multivariate adaptive regression splines (MARS), Random Forest Regression, and Deep Neural Network with Historical Data (DWFH), Haar Wavelet Function, Decision Tree and Discrete wavelet Transform (DWT). Data preprocessing, which includes standardisation and lagging to capture temporal dependencies, comes first in the analysis phase. A wavelet transformation is also used to capture complex patterns in the data. Each model is tested on a different test set after being trained on a subset of the dataset. The results are assessed using the Root Mean Squared Error (RMSE) and Mean Squared Error (MSE), focusing on the RMSE and MSE values for better comparison across models. Our findings reveal that the DWFH model achieved an RMSE of 0.0138807 mm and MSE of 0.000193 mm<sup>2</sup>, demonstrating their effectiveness in predicting rainfall. The Random Forest and SVR models also provided competitive results. This study highlights the importance of selecting an appropriate machine learning model for rainfall prediction and the significance of preprocessing techniques in improving model performance. These insights can aid decision-makers in choosing the most suitable model for their specific application, contributing to more accurate rainfall predictions and enhanced decision support systems.</p></div>","PeriodicalId":15096,"journal":{"name":"Journal of Atmospheric and Solar-Terrestrial Physics","volume":null,"pages":null},"PeriodicalIF":1.8,"publicationDate":"2024-08-30","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142151149","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
A statistical analysis of atmospheric parameters for cataloged astronomical observatory sites 对编目天文观测站点大气参数的统计分析
IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-08-30 DOI: 10.1016/j.jastp.2024.106334

Astronomical sites have to be selected according to many factors whereas the geographic location of the site and the quality of the atmosphere above the site play an important role in the decision process. The following factors were chosen to create layers 1907 northern and 235 southern observatories: CC (cloud coverage), PWV (precipitable water vapor), AOD (aerosol optical depth), VWV (vertical wind velocity), and HWV (horizontal wind velocity). To estimate the astronomical importance of the sites, DEM (digital elevation model) and LAT (latitude of observatory location) layers were also included. In addition to the variations or trends, a complete statistical analysis was carried out for all factors to investigate the potential correlations between the factors. There is a clear difference between the northern and southern hemispheres. The exchange of meteorological seasons between hemispheres is also compliant with factors. The geographical locations of most of the observatories were found to be “not suitable”. There seem to be no apparent long-term variations and/or patterns in all factors.

天文观测站必须根据许多因素来选择,而观测站的地理位置和观测站上空的大气质量在决策过程中起着重要作用。我们选择了以下因素来创建 1907 个北方观测站和 235 个南方观测站层:CC(云覆盖率)、PWV(可降水水汽)、AOD(气溶胶光学深度)、VWV(垂直风速)和 HWV(水平风速)。为了估算观测点的天文重要性,还加入了 DEM(数字高程模型)和 LAT(观测站位置纬度)层。除了变化或趋势之外,还对所有因素进行了完整的统计分析,以研究各因素之间的潜在相关性。南北半球之间存在明显差异。半球之间的气象季节交换也与各因素有关。大部分观测站的地理位置被认为 "不合适"。所有因素似乎都没有明显的长期变化和/或模式。
{"title":"A statistical analysis of atmospheric parameters for cataloged astronomical observatory sites","authors":"","doi":"10.1016/j.jastp.2024.106334","DOIUrl":"10.1016/j.jastp.2024.106334","url":null,"abstract":"<div><p>Astronomical sites have to be selected according to many factors whereas the geographic location of the site and the quality of the atmosphere above the site play an important role in the decision process. The following factors were chosen to create layers 1907 northern and 235 southern observatories: CC (cloud coverage), PWV (precipitable water vapor), AOD (aerosol optical depth), VWV (vertical wind velocity), and HWV (horizontal wind velocity). To estimate the astronomical importance of the sites, DEM (digital elevation model) and LAT (latitude of observatory location) layers were also included. In addition to the variations or trends, a complete statistical analysis was carried out for all factors to investigate the potential correlations between the factors. There is a clear difference between the northern and southern hemispheres. The exchange of meteorological seasons between hemispheres is also compliant with factors. The geographical locations of most of the observatories were found to be “not suitable”. There seem to be no apparent long-term variations and/or patterns in all factors.</p></div>","PeriodicalId":15096,"journal":{"name":"Journal of Atmospheric and Solar-Terrestrial Physics","volume":null,"pages":null},"PeriodicalIF":1.8,"publicationDate":"2024-08-30","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142097696","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Time series analysis of sea surface temperature change in the coastal seas of Türkiye 图尔基耶近海海面温度变化的时间序列分析
IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-08-28 DOI: 10.1016/j.jastp.2024.106339

Sea surface temperature (SST) is a crucial geophysical parameter in assessing heat exchange between the air and sea surface. Changes in SST and its accurate prediction play a pivotal role in explaining the global heat balance, determining atmospheric circulations, and constructing global climate models. This work aims to reveal a model for one-month-ahead forecasting of SST time series data along the Türkiye coasts, encompassing the Mediterranean, Aegean, Marmara, and Black Seas, and their long-term future forecast. A long short-term memory (LSTM) neural network and seasonal autoregressive integrated moving average (SARIMA) models are used for this purpose. The ECMWF ERA5 (0.5ox0.5°) monthly SST dataset spanning the years 1970–2023 is used for model development. The results obtained from the LSTM and SARIMA models show that there will be an increasing trend in SSTs along these seacoasts until 2050. The SST measurements of 23.4 °C, 20.2 °C, 17.0 °C, and 16.6 °C recorded along the Mediterranean, Aegean, Marmara, and Black Seas in 2023 are expected to rise to 25.1 °C, 21.9 °C, 18.1 °C, and 18.8 °C, respectively, by 2050. These figures indicate an increase of 7.3%, 8.4%, 6.5%, and 13.3% in the SST values across these coastal seas over the next quarter century.

海面温度(SST)是评估空气与海面之间热量交换的重要地球物理参数。SST 的变化及其准确预测在解释全球热平衡、确定大气环流和构建全球气候模型方面发挥着关键作用。本研究旨在揭示一个模型,用于提前一个月预测图尔基耶沿岸(包括地中海、爱琴海、马尔马拉海和黑海)的 SST 时间序列数据及其未来长期预测。为此使用了长短期记忆(LSTM)神经网络和季节自回归综合移动平均(SARIMA)模型。模型开发使用了 ECMWF ERA5(0.5ox0.5°)月度 SST 数据集,时间跨度为 1970-2023 年。LSTM 和 SARIMA 模型得出的结果表明,直到 2050 年,这些沿海地区的海温将呈上升趋势。2023 年地中海、爱琴海、马尔马拉海和黑海沿岸的海温测量值分别为 23.4 ℃、20.2 ℃、17.0 ℃ 和 16.6 ℃,预计到 2050 年将分别升至 25.1 ℃、21.9 ℃、18.1 ℃ 和 18.8 ℃。这些数据表明,在未来四分之一世纪里,这些沿岸海域的海温值将分别上升 7.3%、8.4%、6.5% 和 13.3%。
{"title":"Time series analysis of sea surface temperature change in the coastal seas of Türkiye","authors":"","doi":"10.1016/j.jastp.2024.106339","DOIUrl":"10.1016/j.jastp.2024.106339","url":null,"abstract":"<div><p>Sea surface temperature (SST) is a crucial geophysical parameter in assessing heat exchange between the air and sea surface. Changes in SST and its accurate prediction play a pivotal role in explaining the global heat balance, determining atmospheric circulations, and constructing global climate models. This work aims to reveal a model for one-month-ahead forecasting of SST time series data along the Türkiye coasts, encompassing the Mediterranean, Aegean, Marmara, and Black Seas, and their long-term future forecast. A long short-term memory (LSTM) neural network and seasonal autoregressive integrated moving average (SARIMA) models are used for this purpose. The ECMWF ERA5 (0.5<sup>o</sup>x0.5°) monthly SST dataset spanning the years 1970–2023 is used for model development. The results obtained from the LSTM and SARIMA models show that there will be an increasing trend in SSTs along these seacoasts until 2050. The SST measurements of 23.4 °C, 20.2 °C, 17.0 °C, and 16.6 °C recorded along the Mediterranean, Aegean, Marmara, and Black Seas in 2023 are expected to rise to 25.1 °C, 21.9 °C, 18.1 °C, and 18.8 °C, respectively, by 2050. These figures indicate an increase of 7.3%, 8.4%, 6.5%, and 13.3% in the SST values across these coastal seas over the next quarter century.</p></div>","PeriodicalId":15096,"journal":{"name":"Journal of Atmospheric and Solar-Terrestrial Physics","volume":null,"pages":null},"PeriodicalIF":1.8,"publicationDate":"2024-08-28","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142097697","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Comparative analysis of machine learning models for predicting PM2.5 concentrations using meteorological and chemical indicators 利用气象和化学指标预测 PM2.5 浓度的机器学习模型比较分析
IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-08-27 DOI: 10.1016/j.jastp.2024.106338

Air pollution significantly impacts human health, causing numerous premature deaths, particularly with the rise in PM2.5 concentrations. Therefore, comparing different machine learning (ML) models for predicting PM2.5 concentration is crucial. This research focuses on six ML models: Linear Regression (LR), Regression Tree (RT), Support Vector Machine (SVM), Ensemble Regression (ERT), Gaussian Process Regression (GPR), and Artificial Neural Networks (ANN). Trained on six years of data (July 2015–December 2021) with optimized hyperparameters, the models consider eight meteorological and chemical indicators as PM2.5 predictors, including temperature, relative humidity, air pressure, O3, SO2, NO2, dew point, and wind speed. Model efficiency is assessed using Mean Squared Error (MSE), Root Mean Squared Error (RMSE), Correlation Coefficient (R), and Coefficient of Determination (R2) values. The models achieve R2 and RMSE values as follows: LR (0.72, 13.52), RT (0.8, 12.156), SVM (0.82, 10.28), ERT (0.81, 11.87), GPR (0.94, 7.65), and ANN (0.99, 2.36). These metrics indicate the superior performance of ANN, with its R2 value approaching 1 and the lowest RMSE compared to other models. The results highlight the effectiveness of ANN, particularly the model with three hidden layers, in predicting PM2.5 concentration. Utilizing ML models for this purpose is crucial for understanding and mitigating the impacts on human health and the environment, with ANN emerging as a promising tool for various investigations.

空气污染严重影响人类健康,导致许多人过早死亡,尤其是随着 PM2.5 浓度的上升。因此,比较不同的机器学习(ML)模型来预测 PM2.5 浓度至关重要。本研究主要关注六种 ML 模型:线性回归(LR)、回归树(RT)、支持向量机(SVM)、集合回归(ERT)、高斯过程回归(GPR)和人工神经网络(ANN)。这些模型以六年(2015 年 7 月至 2021 年 12 月)的数据为基础,采用优化的超参数进行训练,将温度、相对湿度、气压、O3、SO2、NO2、露点和风速等八个气象和化学指标作为 PM2.5 的预测因子。使用平均平方误差 (MSE)、均方根误差 (RMSE)、相关系数 (R) 和判定系数 (R2) 值评估模型效率。模型的 R2 和 RMSE 值如下:LR(0.72,13.52)、RT(0.8,12.156)、SVM(0.82,10.28)、ERT(0.81,11.87)、GPR(0.94,7.65)和 ANN(0.99,2.36)。这些指标表明 ANN 性能优越,其 R2 值接近 1,与其他模型相比 RMSE 最低。这些结果凸显了 ANN,尤其是具有三个隐藏层的模型在预测 PM2.5 浓度方面的有效性。为此目的利用 ML 模型对于了解和减轻对人类健康和环境的影响至关重要,而 ANN 正在成为各种调查的一种有前途的工具。
{"title":"Comparative analysis of machine learning models for predicting PM2.5 concentrations using meteorological and chemical indicators","authors":"","doi":"10.1016/j.jastp.2024.106338","DOIUrl":"10.1016/j.jastp.2024.106338","url":null,"abstract":"<div><p>Air pollution significantly impacts human health, causing numerous premature deaths, particularly with the rise in PM<sub>2.5</sub> concentrations. Therefore, comparing different machine learning (ML) models for predicting PM<sub>2.5</sub> concentration is crucial. This research focuses on six ML models: Linear Regression (LR), Regression Tree (RT), Support Vector Machine (SVM), Ensemble Regression (ERT), Gaussian Process Regression (GPR), and Artificial Neural Networks (ANN). Trained on six years of data (July 2015–December 2021) with optimized hyperparameters, the models consider eight meteorological and chemical indicators as PM<sub>2.5</sub> predictors, including temperature, relative humidity, air pressure, O<sub>3</sub>, SO<sub>2</sub>, NO<sub>2</sub>, dew point, and wind speed. Model efficiency is assessed using Mean Squared Error (MSE), Root Mean Squared Error (RMSE), Correlation Coefficient (R), and Coefficient of Determination (R<sup>2</sup>) values. The models achieve R<sup>2</sup> and RMSE values as follows: LR (0.72, 13.52), RT (0.8, 12.156), SVM (0.82, 10.28), ERT (0.81, 11.87), GPR (0.94, 7.65), and ANN (0.99, 2.36). These metrics indicate the superior performance of ANN, with its R<sup>2</sup> value approaching 1 and the lowest RMSE compared to other models. The results highlight the effectiveness of ANN, particularly the model with three hidden layers, in predicting PM<sub>2.5</sub> concentration. Utilizing ML models for this purpose is crucial for understanding and mitigating the impacts on human health and the environment, with ANN emerging as a promising tool for various investigations.</p></div>","PeriodicalId":15096,"journal":{"name":"Journal of Atmospheric and Solar-Terrestrial Physics","volume":null,"pages":null},"PeriodicalIF":1.8,"publicationDate":"2024-08-27","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142097694","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
A mathematical modelling for solar irradiance reduction of sunshades and some near-future albedo modification approaches for mitigation of global warming 降低遮阳板太阳辐照度的数学模型和一些近未来减缓全球变暖的反照率修正方法
IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-08-24 DOI: 10.1016/j.jastp.2024.106337

To address the global warming problem, one of the space-based geoengineering solutions suggests the construction of an occluding disc that can work as a solar curtain to mitigate solar irradiation penetration to the earth atmosphere. A widely discussed concept needs the construction of a large-scale sunshade system near the Sun–Earth L1 equilibrium point in order to control the average global temperature. However, to improve the accuracy of theoretical estimations, more consistent modeling of the Sun-Curtain-Earth system and solar irradiance reduction rate are required. This study revisits the mathematical modeling of the solar irradiance reduction system and considers the fundamentals of shading physics. Simplified mathematical modeling of solar irradiance reduction rate is derived based on the solar flux density. For the climate control, controllability of the reduction rate by using some physical parameters (e.g., flux reflection rate and angle of the curtain) is discussed. Based on the results of this model, the technical challenges and feasibility of constructing a sunshade system at L1 Lagrange point are evaluated. Some technologically feasible, near-future options for the warming problem are discussed briefly.

为解决全球变暖问题,天基地球工程解决方案之一建议建造一个遮挡圆盘,作为太阳幕布,减少太阳辐射对地球大气层的穿透。一个被广泛讨论的概念是需要在太阳-地球 L1 平衡点附近建造一个大型遮阳系统,以控制全球平均温度。然而,为了提高理论估算的准确性,需要对 "太阳幕-地球 "系统和太阳辐照减少率进行更一致的建模。本研究重新审视了太阳辐照减少系统的数学模型,并考虑了遮阳物理学的基本原理。根据太阳通量密度推导出太阳辐照度降低率的简化数学模型。在气候控制方面,讨论了通过使用一些物理参数(如通量反射率和幕布角度)来控制辐照度降低率的可控性。根据该模型的结果,评估了在 L1 拉格朗日点建造遮阳系统的技术挑战和可行性。此外,还简要讨论了一些技术上可行的、在不远的将来解决气候变暖问题的方案。
{"title":"A mathematical modelling for solar irradiance reduction of sunshades and some near-future albedo modification approaches for mitigation of global warming","authors":"","doi":"10.1016/j.jastp.2024.106337","DOIUrl":"10.1016/j.jastp.2024.106337","url":null,"abstract":"<div><p>To address the global warming problem, one of the space-based geoengineering solutions suggests the construction of an occluding disc that can work as a solar curtain to mitigate solar irradiation penetration to the earth atmosphere. A widely discussed concept needs the construction of a large-scale sunshade system near the Sun–Earth L<sub>1</sub> equilibrium point in order to control the average global temperature. However, to improve the accuracy of theoretical estimations, more consistent modeling of the Sun-Curtain-Earth system and solar irradiance reduction rate are required. This study revisits the mathematical modeling of the solar irradiance reduction system and considers the fundamentals of shading physics. Simplified mathematical modeling of solar irradiance reduction rate is derived based on the solar flux density. For the climate control, controllability of the reduction rate by using some physical parameters (e.g., flux reflection rate and angle of the curtain) is discussed. Based on the results of this model, the technical challenges and feasibility of constructing a sunshade system at L<sub>1</sub> Lagrange point are evaluated. Some technologically feasible, near-future options for the warming problem are discussed briefly.</p></div>","PeriodicalId":15096,"journal":{"name":"Journal of Atmospheric and Solar-Terrestrial Physics","volume":null,"pages":null},"PeriodicalIF":1.8,"publicationDate":"2024-08-24","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142097695","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Novel particulate matter (PM2.5) forecasting method based on deep learning with suitable spatiotemporal correlation analysis 基于深度学习和适当时空相关性分析的新型颗粒物(PM2.5)预报方法
IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-08-23 DOI: 10.1016/j.jastp.2024.106336

Since air pollution caused by PM 2.5 (particulate matter with an aerodynamic diameter of ≤2.5 μm) is a serious threat to human health, the accurate forecasting of PM 2.5 concentration in metropolitan areas is one of the prior conditions to reduce and eliminate the harmful impacts on human beings produced by PM2.5. In this study, we analyzed the spatiotemporal correlations between target and observation parameters relevant to air pollution forecasting and proposed a convolutional neural network (CNN) and long short-term memory (LSTM) model (also called PM predictor) for next day's daily average PM 2.5 concentration forecasting in Beijing. The proposed spatiotemporal correlations were analyzed for efficient estimation of mutual information, not only if the degrees of variations between the two spaces under consideration are similar, but also if the degrees of variations are significantly different, thereby generating a spatiotemporal feature vector. CNN provided an efficient extraction of inherent features for latent air quality and meteorological input data relevant to PM 2.5, and LSTM delivered the historical information in the time series data, thus a novel PM predictor with remarkably improved performance was constructed, compared with multi-layer perceptron (MLP) and LSTM model in overall forecasting. The air quality and meteorological data from the monitoring stations in Beijing and four surrounding cities from January 1, 2015 to December 31, 2017 were adopted as dataset. The forecasting results suggest that the proposed PM predictor is superior to other models in overall forecasting, while LSTM is better than PM predictor with slight difference in seasonal forecasting.

由于 PM2.5(空气动力学直径≤2.5 μm的颗粒物)造成的空气污染严重威胁人类健康,准确预报城市地区 PM2.5 浓度是减少和消除 PM2.5 对人类造成危害的先决条件之一。在本研究中,我们分析了与空气污染预报相关的目标参数和观测参数之间的时空相关性,并提出了一种卷积神经网络(CNN)和长短期记忆(LSTM)模型(又称 PM 预测器),用于北京地区次日 PM2.5 日均浓度的预报。对所提出的时空相关性进行了分析,以有效估计互信息,不仅考虑两个空间之间的变化程度是否相似,还考虑变化程度是否存在显著差异,从而生成时空特征向量。CNN 有效提取了与 PM 2.5 相关的潜在空气质量和气象输入数据的固有特征,而 LSTM 则提供了时间序列数据中的历史信息,因此,与多层感知器(MLP)和 LSTM 模型相比,构建的新型 PM 预测器在整体预测方面的性能有了显著提高。数据集采用了北京及周边四个城市监测站 2015 年 1 月 1 日至 2017 年 12 月 31 日的空气质量和气象数据。预报结果表明,所提出的 PM 预测模型在总体预报中优于其他模型,而 LSTM 在季节预报中优于 PM 预测模型,但略有差异。
{"title":"Novel particulate matter (PM2.5) forecasting method based on deep learning with suitable spatiotemporal correlation analysis","authors":"","doi":"10.1016/j.jastp.2024.106336","DOIUrl":"10.1016/j.jastp.2024.106336","url":null,"abstract":"<div><p>Since air pollution caused by PM 2.5 (particulate matter with an aerodynamic diameter of ≤2.5 μm) is a serious threat to human health, the accurate forecasting of PM 2.5 concentration in metropolitan areas is one of the prior conditions to reduce and eliminate the harmful impacts on human beings produced by PM2.5. In this study, we analyzed the spatiotemporal correlations between target and observation parameters relevant to air pollution forecasting and proposed a convolutional neural network (CNN) and long short-term memory (LSTM) model (also called PM predictor) for next day's daily average PM 2.5 concentration forecasting in Beijing. The proposed spatiotemporal correlations were analyzed for efficient estimation of mutual information, not only if the degrees of variations between the two spaces under consideration are similar, but also if the degrees of variations are significantly different, thereby generating a spatiotemporal feature vector. CNN provided an efficient extraction of inherent features for latent air quality and meteorological input data relevant to PM 2.5, and LSTM delivered the historical information in the time series data, thus a novel PM predictor with remarkably improved performance was constructed, compared with multi-layer perceptron (MLP) and LSTM model in overall forecasting. The air quality and meteorological data from the monitoring stations in Beijing and four surrounding cities from January 1, 2015 to December 31, 2017 were adopted as dataset. The forecasting results suggest that the proposed PM predictor is superior to other models in overall forecasting, while LSTM is better than PM predictor with slight difference in seasonal forecasting.</p></div>","PeriodicalId":15096,"journal":{"name":"Journal of Atmospheric and Solar-Terrestrial Physics","volume":null,"pages":null},"PeriodicalIF":1.8,"publicationDate":"2024-08-23","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142151150","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Polarization lidar observations of diurnal and seasonal variations in the atmospheric mixing layer above a tropical rural place gadanki, India 极化激光雷达对印度加丹吉热带农村地区上空大气混合层昼夜和季节变化的观测
IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-08-23 DOI: 10.1016/j.jastp.2024.106335

This study presents the daily and seasonal variation of the atmospheric mixing layer height (MLH) over Gadanki, India (13.45°N, 79.18°E), a tropical rural location based on polarization lidar observations. The observations spanned the years 2009–2014, encompassing 303 instances, and coinciding with radiosonde and surface weather station measurements. The MLH was determined through the analysis of aerosol profiles and confirmed with the MLH values derived from radiosonde data. The lidar depolarization ratio was employed to characterize aerosol shape. This study aims to establish a connection between aerosol backscatter and its shape through lidar observations, considering diurnal and seasonal variations, while also identifying the influencing factors. This study illustrates four distinct case studies conducted during different seasons to depict aerosol behavior in both convectively active and non-active periods. These case studies unveil the influence of aerosol shape on water intake and subsequent residual layer and cloud formation. The observed fluctuations in MLH and aerosol shape suggest a dynamic relationship between local meteorology and long-range aerosol transport.

本研究基于偏振激光雷达观测数据,介绍了印度加丹吉(北纬 13.45°,东经 79.18°)上空大气混合层高度(MLH)的日变化和季节变化。观测时间跨度为 2009-2014 年,共 303 次,与无线电探空仪和地面气象站的测量结果相吻合。通过分析气溶胶剖面确定了 MLH,并与从辐射计数据得出的 MLH 值进行了确认。利用激光雷达去极化比来描述气溶胶的形状。本研究旨在通过激光雷达观测建立气溶胶后向散射与其形状之间的联系,同时考虑昼夜和季节变化,并确定影响因素。本研究阐述了在不同季节进行的四个不同案例研究,以描述对流活跃期和非活跃期的气溶胶行为。这些案例研究揭示了气溶胶形状对吸水和随后的残留层及云形成的影响。观察到的 MLH 和气溶胶形状的波动表明,当地气象与长程气溶胶传输之间存在动态关系。
{"title":"Polarization lidar observations of diurnal and seasonal variations in the atmospheric mixing layer above a tropical rural place gadanki, India","authors":"","doi":"10.1016/j.jastp.2024.106335","DOIUrl":"10.1016/j.jastp.2024.106335","url":null,"abstract":"<div><p>This study presents the daily and seasonal variation of the atmospheric mixing layer height (MLH) over Gadanki, India (13.45°N, 79.18°E), a tropical rural location based on polarization lidar observations. The observations spanned the years 2009–2014, encompassing 303 instances, and coinciding with radiosonde and surface weather station measurements. The MLH was determined through the analysis of aerosol profiles and confirmed with the MLH values derived from radiosonde data. The lidar depolarization ratio was employed to characterize aerosol shape. This study aims to establish a connection between aerosol backscatter and its shape through lidar observations, considering diurnal and seasonal variations, while also identifying the influencing factors. This study illustrates four distinct case studies conducted during different seasons to depict aerosol behavior in both convectively active and non-active periods. These case studies unveil the influence of aerosol shape on water intake and subsequent residual layer and cloud formation. The observed fluctuations in MLH and aerosol shape suggest a dynamic relationship between local meteorology and long-range aerosol transport.</p></div>","PeriodicalId":15096,"journal":{"name":"Journal of Atmospheric and Solar-Terrestrial Physics","volume":null,"pages":null},"PeriodicalIF":1.8,"publicationDate":"2024-08-23","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142097699","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Inter-seasonal variation of rainfall microphysics as observed over New Delhi, India 在印度新德里上空观测到的降雨微物理的季节间变化
IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-08-22 DOI: 10.1016/j.jastp.2024.106333

This study analyzes the raindrop size distribution (RSD) characteristics over New Delhi by dividing the year into three seasons: PreM (March–May), monsoon (June–September), and PostM (October–February). Data from a Joss-Waldvogel Disdrometer, installed at IITM New Delhi, Rajendra Nagar, was used for three years (2021–2023). The observed raindrop spectra were fitted with three-parameter Gamma functions to obtain the RSD. ERA-5 and satellite data were also employed to establish atmospheric and cloud properties for the three seasons. The RSD for the monsoon season shows the highest concentration of midsize (1–3 mm diameter) drops and the highest mean rain rate. PostM has the least concentration of midsize and large (diameter >3 mm) drops. General statistics of rain integral parameters reveal high variability in rain rate (R) and mass-weighted mean diameter (Dm) values during the monsoon season. The mu-lambda scatter plots show considerable differences among the three seasons, indicating slightly distinct rainfall mechanisms in the three seasons. Z-R relations of the form Z = aRb were derived, with the highest coefficient (a) values observed for the PreM precipitation. The exponent (b) is found to be greater than unity in all three seasons. Rainfall was stratified based on rain rate. RSD gets broader with increasing R. Large drops are not found appreciably in the spectrum for R < 20 mm/h. A notable disparity between convective and stratiform RSD is evident. The values of rain integral parameters show considerable differences between the convective and stratiform regimes. A higher fraction of large drops is found for the stratiform rainfall in the PreM season compared to the other two seasons. CAPE, water vapor, surface temperature, and surface winds were higher during PreM and monsoon months compared to PostM. The distribution of differential temperature (δT) indicates that clouds with significant depth are found in PreM and monsoon seasons but are often lacking during PostM.

本研究将一年分为三个季节,分析了新德里上空的雨滴大小分布 (RSD) 特征:季前(3 月至 5 月)、季风(6 月至 9 月)和季后(10 月至 2 月)。数据来自安装在 Rajendra Nagar 新德里国际理工学院的 Joss-Waldvogel 测距仪,时间为三年(2021-2023 年)。观测到的雨滴光谱用三参数伽马函数拟合,以获得 RSD。ERA-5和卫星数据也用于确定三个季节的大气和云层属性。季风季节的 RSD 显示中型(直径 1-3 毫米)雨滴的浓度最高,平均降雨率也最高。后季风季的中型和大型(直径 3 毫米)雨滴最少。雨量积分参数的一般统计显示,季风季节的雨量(R)和质量加权平均直径(Dm)值变化很大。亩-λ散点图显示三个季节之间存在很大差异,表明三个季节的降雨机制略有不同。得出了 Z = aRb 形式的 Z-R 关系,其中预雨季降水的系数(a)值最高。三个季节的指数(b)均大于 1。根据降雨率对降雨进行了分层。在 R < 20 mm/h 的频谱中没有发现明显的大滴。对流和分层 RSD 之间存在明显差异。雨积分参数值在对流和平流状态下显示出相当大的差异。与其他两个季节相比,PreM 季节的层状降雨中大滴的比例更高。与后季风季节相比,前季风季节和季风季节的 CAPE、水汽、地表温度和地表风都更高。温差分布(δT)表明,在气象预报季节和季风季节会出现深度较大的云层,但在气象预报季节后往往缺乏云层。
{"title":"Inter-seasonal variation of rainfall microphysics as observed over New Delhi, India","authors":"","doi":"10.1016/j.jastp.2024.106333","DOIUrl":"10.1016/j.jastp.2024.106333","url":null,"abstract":"<div><p>This study analyzes the raindrop size distribution (RSD) characteristics over New Delhi by dividing the year into three seasons: PreM (March–May), monsoon (June–September), and PostM (October–February). Data from a Joss-Waldvogel Disdrometer, installed at IITM New Delhi, Rajendra Nagar, was used for three years (2021–2023). The observed raindrop spectra were fitted with three-parameter Gamma functions to obtain the RSD. ERA-5 and satellite data were also employed to establish atmospheric and cloud properties for the three seasons. The RSD for the monsoon season shows the highest concentration of midsize (1–3 mm diameter) drops and the highest mean rain rate. PostM has the least concentration of midsize and large (diameter &gt;3 mm) drops. General statistics of rain integral parameters reveal high variability in rain rate (<em>R</em>) and mass-weighted mean diameter (<em>D</em><sub><em>m</em></sub>) values during the monsoon season. The mu-lambda scatter plots show considerable differences among the three seasons, indicating slightly distinct rainfall mechanisms in the three seasons. <em>Z</em>-<em>R</em> relations of the form <em>Z</em> = a<em>R</em><sup>b</sup> were derived, with the highest coefficient (a) values observed for the PreM precipitation. The exponent (b) is found to be greater than unity in all three seasons. Rainfall was stratified based on rain rate. RSD gets broader with increasing <em>R</em>. Large drops are not found appreciably in the spectrum for <em>R</em> &lt; 20 mm/h. A notable disparity between convective and stratiform RSD is evident. The values of rain integral parameters show considerable differences between the convective and stratiform regimes. A higher fraction of large drops is found for the stratiform rainfall in the PreM season compared to the other two seasons. CAPE, water vapor, surface temperature, and surface winds were higher during PreM and monsoon months compared to PostM. The distribution of differential temperature (<em>δT</em>) indicates that clouds with significant depth are found in PreM and monsoon seasons but are often lacking during PostM.</p></div>","PeriodicalId":15096,"journal":{"name":"Journal of Atmospheric and Solar-Terrestrial Physics","volume":null,"pages":null},"PeriodicalIF":1.8,"publicationDate":"2024-08-22","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142049725","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Influence of galactic cosmic ray flux on extreme rainfall events in Greece and Libya 银河宇宙射线通量对希腊和利比亚极端降雨事件的影响
IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-08-21 DOI: 10.1016/j.jastp.2024.106327

The Galactic Cosmic Rays (GCR) flux can contribute to the formation of condensation nuclei (CN), radionuclides, and other particles, which in turn influence the formation of rain and extreme weather events. The aim of this analysis was to investigate the possible influence of GCR flux on the extreme rainfall events that occurred in Greece and Libya in September 2023. We used time series data for GCR, rainfall estimates from ERA5, and Sea Surface Temperature (SST) for the period between September 1, 2023, and September 11, 2023. The results revealed a negative correlation between GCR and SST of −0.807 (Greece) and −0.828 (Libya), and a positive correlation between precipitation and SST of +0.972 (Greece) and +0.998 (Libya). The GCR flux and SST accounted for approximately 60.52% and 34.53% of the extreme event in Greece, and 33.71% and 65.96% in Libya, respectively. These statistical results indicate that GCR flux contributed to the formation of the extreme precipitation event that caused significant destruction in Greece and Libya in September 2023.

银河宇宙射线(GCR)通量可促成凝结核(CN)、放射性核素和其他粒子的形成,进而影响降雨和极端天气事件的形成。本分析旨在研究 GCR 通量对 2023 年 9 月在希腊和利比亚发生的极端降雨事件可能产生的影响。我们使用了 2023 年 9 月 1 日至 2023 年 9 月 11 日期间的 GCR 时间序列数据、ERA5 推算的降雨量以及海面温度(SST)。结果显示,全球降水环流与海面温度的负相关性为-0.807(希腊)和-0.828(利比亚),降水量与海面温度的正相关性为+0.972(希腊)和+0.998(利比亚)。在希腊极端事件中,全球径向温差通量和海温分别约占 60.52% 和 34.53%,在利比亚分别约占 33.71% 和 65.96%。这些统计结果表明,2023 年 9 月希腊和利比亚发生的极端降水事件造成了严重破坏,而全球降水通量对极端降水事件的形成起到了推波助澜的作用。
{"title":"Influence of galactic cosmic ray flux on extreme rainfall events in Greece and Libya","authors":"","doi":"10.1016/j.jastp.2024.106327","DOIUrl":"10.1016/j.jastp.2024.106327","url":null,"abstract":"<div><p>The Galactic Cosmic Rays (GCR) flux can contribute to the formation of condensation nuclei (CN), radionuclides, and other particles, which in turn influence the formation of rain and extreme weather events. The aim of this analysis was to investigate the possible influence of GCR flux on the extreme rainfall events that occurred in Greece and Libya in September 2023. We used time series data for GCR, rainfall estimates from ERA5, and Sea Surface Temperature (SST) for the period between September 1, 2023, and September 11, 2023. The results revealed a negative correlation between GCR and SST of −0.807 (Greece) and −0.828 (Libya), and a positive correlation between precipitation and SST of +0.972 (Greece) and +0.998 (Libya). The GCR flux and SST accounted for approximately 60.52% and 34.53% of the extreme event in Greece, and 33.71% and 65.96% in Libya, respectively. These statistical results indicate that GCR flux contributed to the formation of the extreme precipitation event that caused significant destruction in Greece and Libya in September 2023.</p></div>","PeriodicalId":15096,"journal":{"name":"Journal of Atmospheric and Solar-Terrestrial Physics","volume":null,"pages":null},"PeriodicalIF":1.8,"publicationDate":"2024-08-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142088341","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Formation of ions under the action of cosmic rays in humid air 潮湿空气中宇宙射线作用下离子的形成
IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-08-14 DOI: 10.1016/j.jastp.2024.106332

The processes of ion formation in humid tropospheric air under the action of cosmic rays are considered. In this case, positive and negative cluster ions appear. For this analysis, a kinetic model was developed that includes 55 components and 161 reactions. The calculation was carried out using the KINET software package. It is shown that the ionization of air by cosmic rays at altitudes of 5–35 km leads to the formation of plasma consisting mainly of NH4+NH3H2O, H+(H2O)4 and O2(H2O)2 ions. The maximum concentrations of ions under conditions of minimum magnetic rigidity are observed at altitudes from 10 to 18 km. These results differ sharply from the calculation results obtained for the dry air model.

研究了对流层潮湿空气在宇宙射线作用下形成离子的过程。在这种情况下,会出现正团离子和负团离子。为进行分析,开发了一个动力学模型,其中包括 55 个成分和 161 个反应。计算使用 KINET 软件包进行。结果表明,在 5-35 公里的高空,宇宙射线对空气的电离导致等离子体的形成,主要由 NH4+⋅NH3⋅H2O、H+⋅(H2O)4 和 O2-⋅(H2O)2 离子组成。在磁刚度最小的条件下,10 至 18 千米高度处的离子浓度最大。这些结果与干燥空气模型的计算结果大相径庭。
{"title":"Formation of ions under the action of cosmic rays in humid air","authors":"","doi":"10.1016/j.jastp.2024.106332","DOIUrl":"10.1016/j.jastp.2024.106332","url":null,"abstract":"<div><p>The processes of ion formation in humid tropospheric air under the action of cosmic rays are considered. In this case, positive and negative cluster ions appear. For this analysis, a kinetic model was developed that includes 55 components and 161 reactions. The calculation was carried out using the KINET software package. It is shown that the ionization of air by cosmic rays at altitudes of 5–35 km leads to the formation of plasma consisting mainly of <span><math><mrow><mi>N</mi><msubsup><mi>H</mi><mn>4</mn><mo>+</mo></msubsup><mo>⋅</mo><mi>N</mi><msub><mi>H</mi><mn>3</mn></msub><mo>⋅</mo><msub><mi>H</mi><mn>2</mn></msub><mi>O</mi></mrow></math></span>, <span><math><mrow><msup><mi>H</mi><mo>+</mo></msup><mo>⋅</mo><msub><mrow><mo>(</mo><mrow><msub><mi>H</mi><mn>2</mn></msub><mi>O</mi></mrow><mo>)</mo></mrow><mn>4</mn></msub></mrow></math></span> and <span><math><mrow><msubsup><mi>O</mi><mn>2</mn><mo>−</mo></msubsup><mo>⋅</mo><msub><mrow><mo>(</mo><mrow><msub><mi>H</mi><mn>2</mn></msub><mi>O</mi></mrow><mo>)</mo></mrow><mn>2</mn></msub></mrow></math></span> ions. The maximum concentrations of ions under conditions of minimum magnetic rigidity are observed at altitudes from 10 to 18 km. These results differ sharply from the calculation results obtained for the dry air model.</p></div>","PeriodicalId":15096,"journal":{"name":"Journal of Atmospheric and Solar-Terrestrial Physics","volume":null,"pages":null},"PeriodicalIF":1.8,"publicationDate":"2024-08-14","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"141998555","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
期刊
Journal of Atmospheric and Solar-Terrestrial Physics
全部 Acc. Chem. Res. ACS Applied Bio Materials ACS Appl. Electron. Mater. ACS Appl. Energy Mater. ACS Appl. Mater. Interfaces ACS Appl. Nano Mater. ACS Appl. Polym. Mater. ACS BIOMATER-SCI ENG ACS Catal. ACS Cent. Sci. ACS Chem. Biol. ACS Chemical Health & Safety ACS Chem. Neurosci. ACS Comb. Sci. ACS Earth Space Chem. ACS Energy Lett. ACS Infect. Dis. ACS Macro Lett. ACS Mater. Lett. ACS Med. Chem. Lett. ACS Nano ACS Omega ACS Photonics ACS Sens. ACS Sustainable Chem. Eng. ACS Synth. Biol. Anal. Chem. BIOCHEMISTRY-US Bioconjugate Chem. BIOMACROMOLECULES Chem. Res. Toxicol. Chem. Rev. Chem. Mater. CRYST GROWTH DES ENERG FUEL Environ. Sci. Technol. Environ. Sci. Technol. Lett. Eur. J. Inorg. Chem. IND ENG CHEM RES Inorg. Chem. J. Agric. Food. Chem. J. Chem. Eng. Data J. Chem. Educ. J. Chem. Inf. Model. J. Chem. Theory Comput. J. Med. Chem. J. Nat. Prod. J PROTEOME RES J. Am. Chem. Soc. LANGMUIR MACROMOLECULES Mol. Pharmaceutics Nano Lett. Org. Lett. ORG PROCESS RES DEV ORGANOMETALLICS J. Org. Chem. J. Phys. Chem. J. Phys. Chem. A J. Phys. Chem. B J. Phys. Chem. C J. Phys. Chem. Lett. Analyst Anal. Methods Biomater. Sci. Catal. Sci. Technol. Chem. Commun. Chem. Soc. Rev. CHEM EDUC RES PRACT CRYSTENGCOMM Dalton Trans. Energy Environ. Sci. ENVIRON SCI-NANO ENVIRON SCI-PROC IMP ENVIRON SCI-WAT RES Faraday Discuss. Food Funct. Green Chem. Inorg. Chem. Front. Integr. Biol. J. Anal. At. Spectrom. J. Mater. Chem. A J. Mater. Chem. B J. Mater. Chem. C Lab Chip Mater. Chem. Front. Mater. Horiz. MEDCHEMCOMM Metallomics Mol. Biosyst. Mol. Syst. Des. Eng. Nanoscale Nanoscale Horiz. Nat. Prod. Rep. New J. Chem. Org. Biomol. Chem. Org. Chem. Front. PHOTOCH PHOTOBIO SCI PCCP Polym. Chem.
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
0
微信
客服QQ
Book学术公众号 扫码关注我们
反馈
×
意见反馈
请填写您的意见或建议
请填写您的手机或邮箱
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
现在去查看 取消
×
提示
确定
Book学术官方微信
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术
文献互助 智能选刊 最新文献 互助须知 联系我们:info@booksci.cn
Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。
Copyright © 2023 Book学术 All rights reserved.
ghs 京公网安备 11010802042870号 京ICP备2023020795号-1