{"title":"PNL/KPNO大地频谱计划","authors":"G. Stokes, J. Brault, L. Testerman","doi":"10.1364/sam.1980.tup25","DOIUrl":null,"url":null,"abstract":"For more than a year we have obtained monthly spectra of the earth s atmosphere in the 1.0-2.5μm region using the Fourier Transform Spectrometer (FTS) at the McMath Solar Telescope of Kitt Peak National Observatory. At the present time the spectra are obtained over a range of airmasses ranging between 1 and 10 airmasses. The individual spectra cover the entire 1.0-2.5μm region in a single observation with a resolution of 9.5 mK. The signal-to-noise ratios are generally greater than 1000 for all but the 10 airmass spectra.","PeriodicalId":199214,"journal":{"name":"Topical Meeting on Spectroscopy in Support of Atmospheric Measurements","volume":"84 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1900-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"The PNL/KPNO Telluric Spectrum Program\",\"authors\":\"G. Stokes, J. Brault, L. Testerman\",\"doi\":\"10.1364/sam.1980.tup25\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"For more than a year we have obtained monthly spectra of the earth s atmosphere in the 1.0-2.5μm region using the Fourier Transform Spectrometer (FTS) at the McMath Solar Telescope of Kitt Peak National Observatory. At the present time the spectra are obtained over a range of airmasses ranging between 1 and 10 airmasses. The individual spectra cover the entire 1.0-2.5μm region in a single observation with a resolution of 9.5 mK. The signal-to-noise ratios are generally greater than 1000 for all but the 10 airmass spectra.\",\"PeriodicalId\":199214,\"journal\":{\"name\":\"Topical Meeting on Spectroscopy in Support of Atmospheric Measurements\",\"volume\":\"84 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.tup25\",\"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.tup25","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
For more than a year we have obtained monthly spectra of the earth s atmosphere in the 1.0-2.5μm region using the Fourier Transform Spectrometer (FTS) at the McMath Solar Telescope of Kitt Peak National Observatory. At the present time the spectra are obtained over a range of airmasses ranging between 1 and 10 airmasses. The individual spectra cover the entire 1.0-2.5μm region in a single observation with a resolution of 9.5 mK. The signal-to-noise ratios are generally greater than 1000 for all but the 10 airmass spectra.
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