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dc.contributor.authorFarmer, C.B.
dc.contributor.authorRaper, O.
dc.contributor.authorRobbins, B.D.
dc.contributor.authorToth, R.A.
dc.contributor.authorMuller, C.
dc.date1980
dc.date.accessioned2017-09-08T13:21:08Z
dc.date.available2017-09-08T13:21:08Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/6227
dc.descriptionNear-infrared solar absorption spectra have been recorded in the course of balloon flights from Palestine, Texas, (32 degree N latitude) in May 1976, and Broken Hill, Australia, (30 degree S latitude) in March 1977. The northern flight was made at a float altitude of 37 km and covered the spectral region from 1800 cm** minus **1 to 3600 cm** minus **1, which encompasses infrared transitions of O//3, CH//4, CO, CO//2, N//2O, H//2O, and HCl. The flight in the southern hemisphere, from a float altitude of 39 km, covered the spectral region from 2800 cm** minus **1 to 4500 cm** minus **1, which includes useful transitions for all of the above gases (with the exception of CO) and encompasses as well the 1-0 fundamental band for HF. Both sets of spectra were acquired at sunset by using a high-resolution (0. 13 cm** minus **1) Michelson interferometer. The simultaneous profiles of concentration derived from the spectra for the individual gases covered in each flight are presented and discussed.
dc.languageeng
dc.titleSimultaneous Spectroscopic Measurements of Stratospheric Species: O3, CH4, CO, CO2, N2O, H2O, HCL and HF at Northern and Southern Mid-Latitudes
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleJournal of Geophysical Research
dc.source.volume85
dc.source.issueC3
dc.source.page1621-1632
Orfeo.peerreviewedYes
dc.identifier.doi10.1029/JC085iC03p01621
dc.identifier.scopus2-s2.0-0018998407


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