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The Infra‐Red Prism Spectrograph as a Precision Instrument
dc.contributor.authorOetjen, R. A.en_US
dc.contributor.authorKao, Chao‐lanen_US
dc.contributor.authorRandall, H. M.en_US
dc.date.accessioned2010-05-06T23:21:05Z
dc.date.available2010-05-06T23:21:05Z
dc.date.issued1942-12en_US
dc.identifier.citationOetjen, R. A.; Kao, Chao‐Lan; Randall, H. M. (1942). "The Infra‐Red Prism Spectrograph as a Precision Instrument." Review of Scientific Instruments 13(12): 515-523. <http://hdl.handle.net/2027.42/71192>en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/71192
dc.description.abstractAn investigation of the working conditions of an infra‐red spectrometer of the recording type has resulted in techniques of operation which have increased the precision of the measurements attainable and has permitted an appraisal of the magnitudes of the variations in the resulting data which may still be expected. Included in this study is the remeasurement of the fine structure of certain of the absorption bands of CO2, NH3, and H2O. Measured with a grating instrument whose resolution was made to equal that of the prism instrument in each case, these data give 150 sharp absorption lines between 5μ and 15μ suitable for an empirical calibration of great accuracy.en_US
dc.format.extent3102 bytes
dc.format.extent1548655 bytes
dc.format.mimetypetext/plain
dc.format.mimetypeapplication/pdf
dc.publisherThe American Institute of Physicsen_US
dc.rights© The American Institute of Physicsen_US
dc.titleThe Infra‐Red Prism Spectrograph as a Precision Instrumenten_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelPhysicsen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumUniversity of Michigan, Ann Arbor, Michiganen_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/71192/2/RSINAK-13-12-515-1.pdf
dc.identifier.doi10.1063/1.1769960en_US
dc.identifier.sourceReview of Scientific Instrumentsen_US
dc.identifier.citedreferenceN. Wright, Ind. Eng. Chem. Anal. Ed. 13, 1 (1941); E. D. McAlister, G. L. Matheson, and W. J. Sweeney, Rev. Sci. Inst. 12, 314 (1941); W. H. Avery, J. Opt. Soc. Am. 31, 633 (1941).en_US
dc.identifier.citedreferenceH. M. Randall and John Strong, Rev. Sci. Inst. 2, 585 (1931).en_US
dc.identifier.citedreferenceJohn Strong, Procedures in Experimental Physics (Prentice‐Hall, 1938), p. 305.en_US
dc.identifier.citedreferenceF. A. Firestone, Rev. Sci. Inst. 3, 163 (1932).en_US
dc.identifier.citedreferenceP. C. Cross, Rev. Sci. Inst. 4, 197 (1933).en_US
dc.identifier.citedreferenceC. Schaefer and F. Matossi, Das Ultrarote Spektrum (Springer, 1930), p. 47.en_US
dc.identifier.citedreferenceP. E. Martin and E. F. Barker, Phys. Rev. 41, 291 (1932).en_US
dc.identifier.citedreferenceH. Y. Sheng, E. F. Barker, and D. M. Dennison, Phys. Rev. 60, 786 (1941).en_US
dc.identifier.citedreferenceE. F. Barker, Phys. Rev. 33, 684 (1929).en_US
dc.identifier.citedreferenceW. W. Sleator, Astrophys. J. 48, 125 (1918); W. W. Sleator and E. R. Phelps, Astrophys. J. 62, 28 (1925); H. H. Nielsen, Phys. Rev. 59, 565 (1941).en_US
dc.identifier.citedreferenceR. G. Owens and E. F. Barker, J. Chem. Phys. 10, 146 (1942).en_US
dc.owningcollnamePhysics, Department of


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