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Estimation infrared absorption spectrum

For a reasonable set of the parameters the calculated far-infrared absorption frequency dependence presents a two-humped curve. The absorption peaks due to the librators and the rotators are situated at higher and lower frequencies with respect to each other. The absorption dependences obtained rigorously and in the above-mentioned approximations agree reasonably. An important result concerns the low-frequency (Debye) relaxation spectrum. The hat-flat model gives, unlike the protomodel, a reasonable estimation of the Debye relaxation time td. The negative result for xD obtained in the protomodel is explained as follows. The subensemble of the rotators vanishes, if u —> oo. [Pg.78]

A variety of infrared methods have been available for the simple problems of verifying the purity of the initial resin components and mixtures of those components. The simplest possible test of the purity of a reactant is to compare its spectrum with a known standard. Subtractive methods may be employed to emphasize the most significant intensity changes 19). Composition analysis of the blended resins and hardeners becomes more difficult. In some cases, one may simply select characteristic isolated absorption bands for each component and estimate the composition by comparison to standard spectra of known composition 20,21). [Pg.86]

Infrared Spectroscopy. The following bands are seen in the ir spectrum of PPG 2970, 2940, 2880 cm-1 (C—H stretch, m) 1460,1375 cm-1 (C—H bend, m) 1100,1015 cm-1 (C—O stretch, m) of which the 2940 and 1015 band are specific. The latter are also present in copolymers of EO and PO. Absorptions due to unsaturated end groups are found at 1650 cm-1 (allyl ether) and 1672 cm-1 (1-propenyl ether). The O—H stretching band at 3470 cm-1 shows the greatest variation for different hydroxyl number polyols and has been used to estimate the hydroxyl number (169). [Pg.354]

The structure and electronic levels of the molecule have been established by Merer and Travis (1 ) from an analysis of the rotational structure of the visible absorption bands. The estimated triplet state is based on the electronic levels of CP and CHg as given in these tables. The vibrational levels are from Merer and Trvls (j ) and Jacox and Milligan (2), the latter investigated the Infrared spectrum of matrix-isolated HCP and also estimated the missing frequency. [Pg.582]

The discovery of methane in the atmosphere is due to Migeotte (1948). He observed the characteristic absorption features of CH4 in the infrared spectrum of the sun and estimated a mixing ratio of 1.5 ppmv. The majority of all recent measurements since the late 1960s have employed gas chromato-... [Pg.146]


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