{"title":"利用Sun Fits影像计算库法地区农村地面气溶胶光学深度(AOD)和Ångström浊度参数","authors":"H. Jawad, A. S. Baron","doi":"10.31257/2018/JKP/2020/120203","DOIUrl":null,"url":null,"abstract":"Since there are no previous studies conducted for calculating Kufa turbidity parameters considering that the urban pollutions is less than that of the Kufa city. For this The prior location of the Faculty of science telescope was chosen to make such observation using a 60 mm solar telescope Coronado of Hα filter equipped with CCD DSI III pro connected to laptop computer . Sun Fits images were captured under a clear sky as well as dusty conditions. Two types of images were classified, one in the clear sky and the other in dusty weather. Matlab code was used to estimate sun intensities in order to calculate aerosol optical depth and Ångström turbidity parameters from sun images. These values are expressing the normality behavior with nearer places in territorial region.","PeriodicalId":16215,"journal":{"name":"Journal of Kufa - Physics","volume":"13 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2020-12-10","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Using Sun Fits images for calculation of terrestrial aerosol optical depth (AOD) and Ångström turbidity parameters in countryside of Kufa district\",\"authors\":\"H. Jawad, A. S. Baron\",\"doi\":\"10.31257/2018/JKP/2020/120203\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Since there are no previous studies conducted for calculating Kufa turbidity parameters considering that the urban pollutions is less than that of the Kufa city. For this The prior location of the Faculty of science telescope was chosen to make such observation using a 60 mm solar telescope Coronado of Hα filter equipped with CCD DSI III pro connected to laptop computer . Sun Fits images were captured under a clear sky as well as dusty conditions. Two types of images were classified, one in the clear sky and the other in dusty weather. Matlab code was used to estimate sun intensities in order to calculate aerosol optical depth and Ångström turbidity parameters from sun images. These values are expressing the normality behavior with nearer places in territorial region.\",\"PeriodicalId\":16215,\"journal\":{\"name\":\"Journal of Kufa - Physics\",\"volume\":\"13 1\",\"pages\":\"\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2020-12-10\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Journal of Kufa - Physics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.31257/2018/JKP/2020/120203\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Kufa - Physics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.31257/2018/JKP/2020/120203","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
摘要
由于考虑到库法市的城市污染比库法市小,目前还没有对库法浊度参数的计算进行研究。为此,选择科学学院望远镜的优先位置,使用60毫米太阳望远镜科罗纳多Hα滤光片,配备CCD DSI III pro连接笔记本电脑进行观测。Sun Fits的照片是在晴朗的天空和多尘的条件下拍摄的。两种类型的图像被分类,一种在晴朗的天空中,另一种在尘土飞扬的天气中。利用Matlab代码估计太阳强度,从太阳图像中计算气溶胶光学深度和Ångström浊度参数。这些数值表达的是在领土区域内距离较近的正常行为。
Using Sun Fits images for calculation of terrestrial aerosol optical depth (AOD) and Ångström turbidity parameters in countryside of Kufa district
Since there are no previous studies conducted for calculating Kufa turbidity parameters considering that the urban pollutions is less than that of the Kufa city. For this The prior location of the Faculty of science telescope was chosen to make such observation using a 60 mm solar telescope Coronado of Hα filter equipped with CCD DSI III pro connected to laptop computer . Sun Fits images were captured under a clear sky as well as dusty conditions. Two types of images were classified, one in the clear sky and the other in dusty weather. Matlab code was used to estimate sun intensities in order to calculate aerosol optical depth and Ångström turbidity parameters from sun images. These values are expressing the normality behavior with nearer places in territorial region.