{"title":"高分辨率低噪声大气光谱学","authors":"L. Delbouille","doi":"10.1364/hrfts.1992.sab1","DOIUrl":null,"url":null,"abstract":"High resolution absorption infrared spectroscopy is a largely used way to gather information on the chemical composition of the Earth atmosphere.\n The early pioneers (A. Adel, M. Migeotte,…), using large grating instruments, were able to recognize the vibration-rotation signatures of molecules like CH4, CO, NO, N2O … They showed how the Sun can be used as the necessary bright and stable light source.","PeriodicalId":159025,"journal":{"name":"High Resolution Fourier Transform Spectroscopy","volume":"77 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1900-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"High Resolution Low Noise Atmospheric Spectroscopy\",\"authors\":\"L. Delbouille\",\"doi\":\"10.1364/hrfts.1992.sab1\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"High resolution absorption infrared spectroscopy is a largely used way to gather information on the chemical composition of the Earth atmosphere.\\n The early pioneers (A. Adel, M. Migeotte,…), using large grating instruments, were able to recognize the vibration-rotation signatures of molecules like CH4, CO, NO, N2O … They showed how the Sun can be used as the necessary bright and stable light source.\",\"PeriodicalId\":159025,\"journal\":{\"name\":\"High Resolution Fourier Transform Spectroscopy\",\"volume\":\"77 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"1900-01-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"High Resolution Fourier Transform Spectroscopy\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1364/hrfts.1992.sab1\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"High Resolution Fourier Transform Spectroscopy","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1364/hrfts.1992.sab1","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
高分辨率吸收红外光谱是收集地球大气化学成分信息的一种广泛使用的方法。早期的先驱(A. Adel, M. Migeotte,…)使用大型光栅仪器,能够识别像CH4, CO, NO, N2O这样的分子的振动旋转特征…他们展示了如何将太阳用作必要的明亮和稳定的光源。
High Resolution Low Noise Atmospheric Spectroscopy
High resolution absorption infrared spectroscopy is a largely used way to gather information on the chemical composition of the Earth atmosphere.
The early pioneers (A. Adel, M. Migeotte,…), using large grating instruments, were able to recognize the vibration-rotation signatures of molecules like CH4, CO, NO, N2O … They showed how the Sun can be used as the necessary bright and stable light source.