{"title":"High Temperature Absorption Spectrum of 4.3 Micron CO2†","authors":"M. Esplin, H. Sakai","doi":"10.1364/sam.1980.wp11","DOIUrl":"https://doi.org/10.1364/sam.1980.wp11","url":null,"abstract":"The importance of CO2 as an atmospheric molecule makes the obtaining of high precision band parameters for a great number of bands a significant contribution to both theoretical and experimental studies of our atmosphere. Very accurate parameters on the (00011-00001) band of 12C16O2 have been obtained by Pine and Guelachvili. Their measurment was accomplished by combining two spectra, a room temperature Fourier transform spectrum, and a high temperature tunable laser spectrum.1 There have been numerous measurements of other bands of CO2,2,3 but they were made either with lower resolution spectrometers, or near room temperature where fewer rotational lines were excited, resulting in a less accurate determination of band parameters. In this work a high resolution Michelson interferometer was coupled with a high temperature absorption cell4 heated to 800 K to obtain a high resolution (0.007 cm−1), high temperature spectrum of CO2 in the 4.3 micron region.","PeriodicalId":199214,"journal":{"name":"Topical Meeting on Spectroscopy in Support of Atmospheric Measurements","volume":"60 1","pages":"0"},"PeriodicalIF":0.0,"publicationDate":"1900-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"129905833","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Infrared Emission Spectroscopy of Atmospheric Atoms and Molecules*","authors":"Ron Johansson, Martti Peltola, H. Sakai","doi":"10.1364/sam.1980.wp12","DOIUrl":"https://doi.org/10.1364/sam.1980.wp12","url":null,"abstract":"In recent years many studies have been focused on the problems associated with the infrared radiation observable in the upper atmosphere. Identification of the spectral features in the observed radiation is a key to improving our understanding of the physical and chemical processes in the upper atmosphere. In our laboratory experimental program we study the infrared emission features of various atmospheric species, atomic and molecular, using the technique of Fourier spectroscopy.","PeriodicalId":199214,"journal":{"name":"Topical Meeting on Spectroscopy in Support of Atmospheric Measurements","volume":"1 1","pages":"0"},"PeriodicalIF":0.0,"publicationDate":"1900-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"128995852","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Cutoff-Free Theory of Impact Broadening and Shifting of Microwave and Infrared Molecular Spectra","authors":"R. Leavitt, D. Korff","doi":"10.1364/sam.1980.wp5","DOIUrl":"https://doi.org/10.1364/sam.1980.wp5","url":null,"abstract":"The semiclassical Anderson-Tsao-Curnutte (ATC) impact theory [1,2] of pressure broadening in molecular spectra has been successful in calculations of linewidths and shifts in the microwave and infrared regimes. However, the theory suffers from a fundamental defect in that, for small impact parameter, b, the interruption function, S(b), attains unphysically large values. In an attempt to circumvent this difficulty, Murphy and Boggs [3] developed an alternative method that used an exponential expansion of the collision matrix elements; this expansion led to finite values of the matrix elements for all impact parameters. Cattani [4] grafted the Murphy-Boggs expansion onto the ATC theory; a similar result was later derived by Salesky and Korff [5]. These latter three approaches neglect the important reorientation terms that were shown by Gordon [6] to be significant.","PeriodicalId":199214,"journal":{"name":"Topical Meeting on Spectroscopy in Support of Atmospheric Measurements","volume":"279 1","pages":"0"},"PeriodicalIF":0.0,"publicationDate":"1900-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"123183049","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Introductory Remarks","authors":"R. Toth","doi":"10.1364/sam.1980.ma1","DOIUrl":"https://doi.org/10.1364/sam.1980.ma1","url":null,"abstract":"Summary not available.","PeriodicalId":199214,"journal":{"name":"Topical Meeting on Spectroscopy in Support of Atmospheric Measurements","volume":"37 1","pages":"0"},"PeriodicalIF":0.0,"publicationDate":"1900-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"125748687","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}