{"title":"光谱资料在平流层光谱解释中的应用","authors":"W. Mankin, M. Coffey, A. Goldman","doi":"10.1364/sam.1980.tup19","DOIUrl":null,"url":null,"abstract":"Infrared spectroscopy is one of the most powerful diagnostic methods for the study of atmospheric composition. One of its useful attributes is the ability to remotely sense portions of the atmosphere far from the instrument. This attribute is particularly useful when measuring strato-stratospheric trace gases as a function of latitude, since at many atitudes, especially in the tropics, there are no convenient balloon launch locations for in situ measurements.","PeriodicalId":199214,"journal":{"name":"Topical Meeting on Spectroscopy in Support of Atmospheric Measurements","volume":"21 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1900-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Application of Spectroscopic Data To The Interpretation of Stratospheric Spectra\",\"authors\":\"W. Mankin, M. Coffey, A. Goldman\",\"doi\":\"10.1364/sam.1980.tup19\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Infrared spectroscopy is one of the most powerful diagnostic methods for the study of atmospheric composition. One of its useful attributes is the ability to remotely sense portions of the atmosphere far from the instrument. This attribute is particularly useful when measuring strato-stratospheric trace gases as a function of latitude, since at many atitudes, especially in the tropics, there are no convenient balloon launch locations for in situ measurements.\",\"PeriodicalId\":199214,\"journal\":{\"name\":\"Topical Meeting on Spectroscopy in Support of Atmospheric Measurements\",\"volume\":\"21 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\":\"Topical Meeting on Spectroscopy in Support of Atmospheric Measurements\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1364/sam.1980.tup19\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Topical Meeting on Spectroscopy in Support of Atmospheric Measurements","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1364/sam.1980.tup19","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Application of Spectroscopic Data To The Interpretation of Stratospheric Spectra
Infrared spectroscopy is one of the most powerful diagnostic methods for the study of atmospheric composition. One of its useful attributes is the ability to remotely sense portions of the atmosphere far from the instrument. This attribute is particularly useful when measuring strato-stratospheric trace gases as a function of latitude, since at many atitudes, especially in the tropics, there are no convenient balloon launch locations for in situ measurements.
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