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Experiment 1 Photometry

The following polyvitamin prepai ations were analyzed Kal tsid (OAO Comfort Plus , Russia), Asvitol (OAO INC Marbiofarm , Russia), Pikovit (KRKA, d.d. The New Place, Slovenia), Yeast with vitamin C (000 EKKO Plus , Russia). Chromatographic experiment has been carried out using Silufol UV-254 (Kavalier, Czech Republic) and acetone - ethyl acetate - acetic acid - ethanol (3 5 1 1) - CTAB (2T0 M) as a mobile phase mixture. The linearity calibration plot, built in coordinate S = f (IgqAC), is valid in the interval 5-25 p.g. Correctness of the determination has been checked by photometry. The obtained results for the ascorbic acid determination are presented below. [Pg.385]

SEC-MALLS and SEC-LALLS Coupled chromatography and light-scattering photometry that allows the determination of a number of important values along with chain length distribution, sedimentation equilibrium experiment Ultracentrifugation technique that allows chain length information to be determined. [Pg.80]

Other methods, such as the fasting urinary hydroxypro-line/creatinine ratio, alkaline phosphatase activity, dualabsorption photometry of the hip, and serum osteocalcin measurements, can also be used, depending on an individual clinic s equipment and experience (SEDA-17, 447). [Pg.29]

A schematic of the apparatus is shown in Figure 1. OH was produced by 248 nm (or 266 nm in some experiments) pulsed laser photolysis of H2O2 and detected by observing fluorescence excited by a pulsed tunable dye laser. Fluorescence was excited in the 0H(a2e+ - X tt) 0-1 band at 282 nm and detected in the O-O and 1-1 bands at 309+5 nm. Kinetic data was obtained by electronically varying the time delay between the photolysis laser and the probe laser. Sulfide concentrations were measured in situ in the slow flow system by UV photometry at 228.8 nm. [Pg.134]

Britton and Davidson have shocked mixtures of H2-Br2 diluted in argon to temperatures between 1000 °K and 1500 °K. Under the conditions of these experiments, steady-state concentrations of Br atoms are not achieved. By using previously measured rates for the collision induced dissociation of bromine and direct measurement of the time dependence of the Br2 concentrations by photometry, they calculated the rate coefficient for (2) and obtain values approximately one-half as large as those based on low temperature measurements. They find... [Pg.214]

Hanert, H. H. (2002). Bacterial and chemical iron oxide deposition in a shallow bay on Palaea Kameni, Santorini, Greece microscopy, electron probe microanalysis, and photometry of in situ experiments. Geomicrobiol. J. 19, 317-342. [Pg.365]

Calcination, conditioning and catalytic reaction under steady state and transient conditions were carried out in a microcatalytic tubular reactor using different feeds containing up to 30 vol % water vapour. The reaction products were determined by on line gas chromatography (MA and n-butane) and nondispersive IR photometry (C0,C02). In addition, experiments were performed with catalyst samples pretreated by mixtures of N2 with water vapour. The P V ratios in the surface and subsurface layers were determined by XPS and ISS, respectively. The influence of H2O on the solids was measured by in situ TG. [Pg.463]

The spectroscopic observation of rather concentrated solutions is of broad interest in photometry. Because of the necessary transmission of solutions, the concentrations in normal direct spectroscopy measurements in photokinetics are restricted to approximately 10 molar solutions. In many experiments - especially in the case of preparative photochemistry (whoe often... [Pg.285]

Rapid progress currently is being made in interpreting photometry and polarimetry of particulate media. This is driven by the needs in many fields of science from laboratory experiments with biological objects to terrestrial and planetary remote sensing. One classic example of particulate media (powder-like surfaces) is a planetary regolith, i.e. soil. [Pg.192]

Each experiment typically removes <0.5% of the analyte from solution - hence virtually non-destructive. Each student will have a different background knowledge but examples of non-destructive techniques are uv-visible spectrometry, infrared spectrometry examples of destructive techniques are atomic absorption spectroscopy, flame photometry. [Pg.244]

Flame atomic emission spectroscopy, also called flame photometry, is based on the measurement of the emission spectrum produced when a solution containing metals or some nonmetals such as halides, sulfur, or phosphorus is introduced into a flame. In early experiments, the detector used was the analyst s eye. Those elements that emitted visible light could be identified qualitatively, and these flame tests were used to confirm the presence of certain elements in the sample, particularly alkali metals and alkaline-earth metals. A list of visible colors emitted by elements in a flame is given in Table 7.1. [Pg.450]

The first experiments of this school were directed to the understanding of ionization interference in flame photometry. Alkemade showed that the short-fall in resonance radiation intensity from alkali metals through ionization, and the suppression of such ionization, could be reconciled with the Saha relation only if an excess of electrons over alkali ions were present in acetylene flames, in amounts which decreased with height in the flame. In developing the study Borgers used the R.F. coil technique to measure electron concentration. He at first supported this conclusion for the clean acetylene flame, but then... [Pg.223]

When using an ultraviolet photometer for recording purposes, the disturbance resulting from this absorption at 280 nm is rather small in normal experiments, wherein the average concentration of ampholytes is 1 %. However, the disturbances can be severe for low protein contents and high concentrations of ampholytes. If it is desired to evaluate column experiments quantitatively by photometry at 280 nm, it may be necessary to make corrections for this absorption. These can be made by running one control experiment without protein. [Pg.25]

Becquerel at least knew about Auer s result. Kriiss, one of the founders of photometry (Szabadvary 1966, p. 343), in a paper published together with Nilson, concluded from their absorption photometric studies that the rare earth elements known up to then include at least twenty as yet unknown elements (Kriiss and Nilson 1887). Bettendorf repeated Auer s experiments in 1890 and by subjecting all mother liquors individually to spectrometry he confirmed the existence of praseodidymium and neodidymium (Bettendorf 1890). [Pg.62]

Experience showed that the performance of Brewer-Mast sondes critically depends on the prelaunch procedure of the sondes, whereas the ECC sondes need less sophisticated control before launch. The integrated ozone amount measured by the sonde can be compared with the total ozone amount measured by sun photometry (usually performed by Dobson spectrophotometers). This requires the extrapolation of the O3 profile above the burst level of the balloons (residual ozone). This comparison can be used to check the quality of the ozone profile of the sonde. The factor obtained by the sum of the ozone measured by the sonde plus the residual ozone divided... [Pg.280]

In general many experiments are needed with both techniques to obtain a comprehensive picture of a reaction. Kinetic photometry can be used in n experiments at different wavelengths, or time-resolved spectroscopy can be repeated in n experiments at different times and the data can be analyzed to provide a complete picture. Apart of being time-consuming and often expensive in chemicals, such repeated experiments present problems of reproducibility and accuracy which have so far severely limited their use. [Pg.151]

This "space experiment data consist of broad bandpass photometry, most of it in the far-infrared (FIR). There is also limited information on source size. [Pg.129]

There is also considerable variety in the astronomical goals. Seven experiments are devoted primarily to far Infrared surveys, seven to measurements of the cosmic background radiation, four to high resolution mapping and photometry, one to measurement of diffuse emission in the near Infrared, five to solar brightness, polarization, and spectra, and one to planetary spectra,... [Pg.156]


See other pages where Experiment 1 Photometry is mentioned: [Pg.17]    [Pg.19]    [Pg.21]    [Pg.23]    [Pg.411]    [Pg.208]    [Pg.187]    [Pg.20]    [Pg.244]    [Pg.123]    [Pg.209]    [Pg.112]    [Pg.17]    [Pg.19]    [Pg.21]    [Pg.23]    [Pg.411]    [Pg.267]    [Pg.498]    [Pg.2049]    [Pg.32]    [Pg.295]    [Pg.443]    [Pg.1091]    [Pg.60]    [Pg.23]    [Pg.94]    [Pg.382]    [Pg.642]    [Pg.433]    [Pg.1069]    [Pg.159]    [Pg.356]    [Pg.78]    [Pg.575]   


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Photometry

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