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Spectral absorbance

It is usually difficult, if not impossible, to quantify all of the components in our samples. This is expecially true when we consider the meaning of the word "components" in the broadest sense. Even if we have accurate values for all of the constituents in our samples, how do we quantify the contribution to the spectral absorbance due to instrument drift, operator effect, instrument aging, sample cell alignment, etc. The simple answer is that, generally, we can t. To the extent that we do not provide CLS with the concentration of all of the components in our samples, we might expect CLS to have problems. In the case of our simulated data, we have samples that contain 4 components, but we only have concentration values for 3 of the components. Each sample also contains a random baseline for which "concentration values are not available. Let s see how CLS handles these data. [Pg.54]

Unlike CLS, ILS does not require that we provide concentration values for all of the components present. In equation [47], we are not trying to account for all of the absorbances in the spectra. Instead, the formulation allows us to pick up only that portion of the spectral absorbance that correlates well to the concentrations. If ILS is able to do so well with degraded spectra, imagine how much better we might do if we can find a more optimum way of reducing the dimensionality of the spectra than simply summing them into bins. That is precisely what PCR and PLS will do for us. [Pg.78]

Artifact removal and/or linearization. A common form of artifact removal is baseline correction of a spectrum or chromatogram. Common linearizations are the conversion of spectral transmittance into spectral absorbance and the multiplicative scatter correction for diffuse reflectance spectra. We must be very careful when attempting to remove artifacts. If we do not remove them correctly, we can actually introduce other artifacts that are worse than the ones we are trying to remove. But, for every artifact that we can correctly remove from the data, we make available additional degrees-of-freedom that the model can use to fit the relationship between the concentrations and the absorbances. This translates into greater precision and robustness of the calibration. Thus, if we can do it properly, it is always better to remove an artifact than to rely on the calibration to fit it. Similar reasoning applies to data linearization. [Pg.99]

Electrodes are now available for the selective determination of the concentrations of a large number of cations and anions. Halide-sensitive electrodes have been used to monitor reactions, but their relatively slow response has restricted their use. They may have particular utility in the study of reactions with low spectral absorbance changes and also in an ancillary role to the kinetics determination. [Pg.173]

Figure 24.7 Comparison of the measured (1) and calculated (2, using the HITRAN 92 database) spectral absorbance of the R-branch of the CO Zv band. The data were obtained at 296 K, 338 Torr, Aco = 9.91%, Xkv = 9.79% in air, over an absorption pathlength of 3227 cm. Spectral absorbance is defined by k L = ln(/o//)... Figure 24.7 Comparison of the measured (1) and calculated (2, using the HITRAN 92 database) spectral absorbance of the R-branch of the CO Zv band. The data were obtained at 296 K, 338 Torr, Aco = 9.91%, Xkv = 9.79% in air, over an absorption pathlength of 3227 cm. Spectral absorbance is defined by k L = ln(/o//)...
TNT Determination. Dilute the TNT filtrate obtd in 4.4.3.2.1 to 50ml with ethylene chloride. Compare its spectral absorbance at 20° with that of a soln, 0.400g of TNT in 50ml ethylene chloride at 367 millimicrons. Det TNT by reference to a graph prepd in advance from known soln. The prepn of the solns and the graph is described in 4.4.3.5.1. A Beckman DK-2 or equivalent spectrophotometer may be used to det the spectral absorbance... [Pg.27]

Determine the spectral absorbance of the hot melt standard solns at 430mu as described in 4.4.3.4.14... [Pg.32]

Spectral absorbance (absorbance spectrum) Absorbance described as function of wavelength. [Pg.259]

Step 4 Nevertheless, so far we only extracted information from the X- and Y-blocks. Now a regression step is needed to obtain a predictive model. This is achieved by establishing an inner relationship between u (the scores representing the concentrations of the analytes we want to predict) and t (the scores representing the spectral absorbances) that we just calculated for the X- and Y-blocks. The simplest one is an ordinary regression (note that the regression coefficient is just a scalar because we are relating two vectors) ... [Pg.188]

In order to express the absorbances obtained by this method in terms of moles of carbonyl, the spectral absorbances of DNPH derivatives of several purified carbonyl compounds were measured. At 430 nm, molar extinction coefficients of 16,000 and 21,350 were determined for the saturated and unsaturated carbonyl compounds, respectively, whereas at 460 nm, the values were 12,450 and 28,100, respectively. Based on the present methodology and use of 1-cm cuvettes, the above equations were derived (Henick et al., 1954). [Pg.554]

Here, A is the reaction s measured IR spectral absorbance, Nt is the number of measurements at different times, N0 is the number of wavelengths, C is the concentration matrix with the concentration-time profiles of each absorbing component in the columns, Nc is the number of chemical components and E is the pure spectra matrix with the spectral absorption at each wave number of each pure absorbing component in the rows. If a chemical component does not absorb, the corresponding spectrum of the pure chemical will be a vector of zeros. [Pg.209]

It should be noted that, by measuring reaction spectra for the purpose of estimating reaction-model parameters (such as rate constants or activation energies), a new set of unknown parameters is introduced, i.e. the spectral absorbances of the pure chemical components involved in the reaction (matrix ). [Pg.210]

A fundamental problem of reaction simulation is the choice of an appropriate reaction model. No standard procedure for this problem can be found in the literature. It is essential, therefore, that model-based measurements of reaction data support the task of model selection. Generally, the residuals in the comparison of the data from the modelled reaction with the experimental measurements are taken as an indication of the quality of the reaction model. However, the robustness of the model fit generally decreases with increasing number of reaction parameters (such as rate constants, activation energies, reaction enthalpies or spectral absorbances) that have to be determined. In this example, we demonstrate how different reaction models can be postulated and then tested on the basis of calorimetric and IR-ATR measurements. [Pg.216]

This experiment was carried out four times at 17°C and three times at each of 24, 30 and 36°C. The spectral absorbances of all experiments were then concatenated into a single AData matrix Similarly, the calorimetric data were concatenated into a single qData vector. [Pg.217]

Figure 5.3 The spectral absorbance of macular pigment plotted with the blue light hazard function. (From Hammond, B.R. et al., Optom. Vis. Sci., 82(5), 387-404, 2005.) This function described the potential for photochemical damage to the retina resulting from exposure to light from about 400 to 500 nm as defined by the IESNA Photobiology Committee for ANSI (ANSI/ IESNA RP-27.1-05). Figure 5.3 The spectral absorbance of macular pigment plotted with the blue light hazard function. (From Hammond, B.R. et al., Optom. Vis. Sci., 82(5), 387-404, 2005.) This function described the potential for photochemical damage to the retina resulting from exposure to light from about 400 to 500 nm as defined by the IESNA Photobiology Committee for ANSI (ANSI/ IESNA RP-27.1-05).
Wooten, B.R., and Hammond, B.R. Spectral absorbance and spatial distribution of macular pigment using heterochromatic flicker photometry, Optom. Vis. Sci., 82(5), 378-386, 2005. [Pg.102]

Although many elements of measurement in chemistry are by nature physical, such as those involving mass, volume, time, temperature and spectral absorbance, the calibration hierarchy in chemistry is seldom described as a series of comparisons between measurement standards. Rather, a measurement procedure points to a measuring system performing a measurement which assigns a quantity value and measurement uncertainty to a calibrator itself a type of measurement standard which serves to calibrate the next measuring system, operated according to a second measurement procedure, and so on. [Pg.32]

The experiment is run first at 118°C to remove water from the initial hydrated CuCl2, 2H20 commercial product. After around one hour, water vapour is generated at a temperature close to 390°C The formation of HC1 is monitored by conductimetry. No chlorine is observed. At a time T, a temperature jump is made to reach 530°C, the formation of molecular chlorine is then identified by its spectral absorbance. The amount of chlorine increases and then decreases when 530°C is reached. [Pg.246]

The spectral (absorbance and fluorescence) characteristics of the solute (pesticide). [Pg.123]

Principal components are primarily abstract mathematical entities and further details are described in Chapter 4. In multivariate calibration the aim is to convert these to compound concentrations. PCR uses regression (sometimes also called transformation or rotation) to convert PC scores to concentrations. This process is often loosely called factor analysis, although terminology differs according to author and discipline. Note that although the chosen example in this chapter involves calibrating concentrations to spectral absorbances, it is equally possible, for example, to calibrate the property of a material to its structural features, or the activity of a drug to molecular parameters. [Pg.292]


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See also in sourсe #XX -- [ Pg.207 ]




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