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The Global ETD Search service is a free service for researchers
to find electronic theses and dissertations. This service is
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Networked Digital Library of Theses and Dissertations.
Our metadata is collected from universities around the world. If you manage a university/consortium/country archive and want to be added, details can be found on the NDLTD website.
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Showing 81 to 90 of 232 (0.059 seconds)Spelling suggestions: "subject:"absorption spectra"" "subject:"asbsorption spectra""
| 81 |
Effects of foreign gases on the total absorption of entire bands in the infrared /Singleton, Edgar Bryson January 1958 (has links)
No description available.
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| 82 |
A sample modulation technique for the study of infrared absorption spectra /Gilfert, James Clare. January 1957 (has links)
No description available.
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| 83 |
Infrared absorption laws for some minor atmospheric constituents /Burch, D. E. January 1959 (has links)
No description available.
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| 84 |
Whole band analysis of absorption bands of carbon dioxide near 3.8 [mu]m.Hoke, Michael Lee January 1981 (has links)
No description available.
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| 85 |
Structural analysis of the purple membrane using absorption and circular dichroism spectra /Draheim, James Edward January 1984 (has links)
No description available.
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| 86 |
Absorption spectrum of VCl₄ /Pennella, Filippo January 1964 (has links)
No description available.
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| 87 |
Infrared spectra of ¹⁵N₂¹⁸O and ¹⁵N¹⁸O /Griggs, James Lee January 1967 (has links)
No description available.
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| 88 |
High resolution absorption spectra of the isotopic modifications of nitrogen dioxide and other small molecules /Hurlock, Stephen Craig January 1970 (has links)
No description available.
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| 89 |
X-ray K absorption spectra of solid argon and krypton /Soules, Jack Arbuthnott January 1954 (has links)
No description available.
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| 90 |
Interstellar C2, CH, and CN in Translucent Molecular Cloudsvan Dishoeck, E. F. 12 1900 (has links)
Optical absorption line techniques have been applied to the study of a number of translucent
molecular clouds in which the total column densities are large enough that substantial
molecular abundances can be maintained. Results are presented for a survey of absorption
lines of interstellar C2, CH, and CN. Detections of CN through the A2II -X2E+ (1,0) and
(2,0) bands of the red system are reported, and are compared with observations of the
blue system for one line of sight. The population distributions in C2 provide diagnostic
information on temperature and density. The measured column densities of the three
species can be used to test details of the theory of molecule formation in clouds where
photo -processes still play a significant role. The C2 and CH column densities are strongly
correlated with each other and probably also with the H2 column density. In contrast, the
CN column densities are found to vary greatly from cloud to cloud. The observations are
discussed with reference to detailed theoretical models.
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