{"title":"与木星和土星的旅行者任务有关的氨红外吸收再研究","authors":"N. Husson, A. Chédin, N. Scott","doi":"10.1364/sam.1980.tup9","DOIUrl":null,"url":null,"abstract":"The scientific objectives of the IRIS experiment of the Voyager 1 and 2 missions[1] (encounters with Jupiter in March and July 1979) are the study of the atmospheres of Jupiter, Saturn and possibly Uranus, from radiometric measurements in the infrared by means of a Michelson interferometer. For the first time, more than 50000 spectra of Jupiter were recorded with a spectral resolution of 4.3 cm-1.","PeriodicalId":199214,"journal":{"name":"Topical Meeting on Spectroscopy in Support of Atmospheric Measurements","volume":"1 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1900-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"The Ammonia Infrared Absorption Reinvestigated in Connection with the Voyager Mission to Jupiter and Saturn\",\"authors\":\"N. Husson, A. Chédin, N. Scott\",\"doi\":\"10.1364/sam.1980.tup9\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The scientific objectives of the IRIS experiment of the Voyager 1 and 2 missions[1] (encounters with Jupiter in March and July 1979) are the study of the atmospheres of Jupiter, Saturn and possibly Uranus, from radiometric measurements in the infrared by means of a Michelson interferometer. For the first time, more than 50000 spectra of Jupiter were recorded with a spectral resolution of 4.3 cm-1.\",\"PeriodicalId\":199214,\"journal\":{\"name\":\"Topical Meeting on Spectroscopy in Support of Atmospheric Measurements\",\"volume\":\"1 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.tup9\",\"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.tup9","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
The Ammonia Infrared Absorption Reinvestigated in Connection with the Voyager Mission to Jupiter and Saturn
The scientific objectives of the IRIS experiment of the Voyager 1 and 2 missions[1] (encounters with Jupiter in March and July 1979) are the study of the atmospheres of Jupiter, Saturn and possibly Uranus, from radiometric measurements in the infrared by means of a Michelson interferometer. For the first time, more than 50000 spectra of Jupiter were recorded with a spectral resolution of 4.3 cm-1.
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