{"title":"测量平流层对3.05 - 3.70微米太阳辐射的吸收","authors":"M. Ackerman, D. Frimout","doi":"10.18758/A_066","DOIUrl":null,"url":null,"abstract":"Solar spectra have been recorded from 3.05 to 3.70µm by means of a balloon borne monochromator at an altitude of 35 km and for solar zenith distances from 75° to 95°. Absorptions due to CH4 and H2O are identified as well as 03 bands observed for the first time in the atmosphere. \n Upper limits for the stratospheric mixing ratios of NO2 and HCHO are deduced.","PeriodicalId":296277,"journal":{"name":"Bulletin de la Classe des sciences","volume":"82 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2018-01-22","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"2","resultStr":"{\"title\":\"Mesure de l'absorption stratosphérique du rayonnement solaire de 3,05 à 3,70 microns\",\"authors\":\"M. Ackerman, D. Frimout\",\"doi\":\"10.18758/A_066\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Solar spectra have been recorded from 3.05 to 3.70µm by means of a balloon borne monochromator at an altitude of 35 km and for solar zenith distances from 75° to 95°. Absorptions due to CH4 and H2O are identified as well as 03 bands observed for the first time in the atmosphere. \\n Upper limits for the stratospheric mixing ratios of NO2 and HCHO are deduced.\",\"PeriodicalId\":296277,\"journal\":{\"name\":\"Bulletin de la Classe des sciences\",\"volume\":\"82 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2018-01-22\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"2\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Bulletin de la Classe des sciences\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.18758/A_066\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Bulletin de la Classe des sciences","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.18758/A_066","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Mesure de l'absorption stratosphérique du rayonnement solaire de 3,05 à 3,70 microns
Solar spectra have been recorded from 3.05 to 3.70µm by means of a balloon borne monochromator at an altitude of 35 km and for solar zenith distances from 75° to 95°. Absorptions due to CH4 and H2O are identified as well as 03 bands observed for the first time in the atmosphere.
Upper limits for the stratospheric mixing ratios of NO2 and HCHO are deduced.
求助内容：
应助结果提醒方式：
京公网安备 11010802042870号
