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Wavelengths mercury

In contrast to spectrophotometry, hght-scattering experiments are generally conducted at constant wavelength. Mercury vapor lamps are the most widely used light sources, since the strong lines at 436 and 546 nm are readily isolated by filters to allow monochromatic illumination. Polarizing filters are also included for both the incident and scattered beams so that depolarization can... [Pg.690]

Pressure. Standard atmospheric pressure is defined to be the force exerted by a column of mercury 760-mm high at 0°C. This corresponds to 0.101325 MPa (14.695 psi). Reference or fixed points for pressure caUbration exist and are analogous to the temperature standards cited (23). These points are based on phase changes or resistance jumps in selected materials. For the highest pressures, the most rehable technique is the correlation of the wavelength shift, /SX with pressure of the mby, R, fluorescence line and is determined by simultaneous specific volume measurements on cubic metals... [Pg.20]

Chlorine free radicals used for the substitutioa reactioa are obtaiaed by either thermal, photochemical, or chemical means. The thermal method requites temperatures of at least 250°C to iaitiate decomposition of the diatomic chlorine molecules iato chlorine radicals. The large reaction exotherm demands close temperature control by cooling or dilution, although adiabatic reactors with an appropriate diluent are commonly used ia iadustrial processes. Thermal chlorination is iaexpeasive and less sensitive to inhibition than the photochemical process. Mercury arc lamps are the usual source of ultraviolet light for photochemical processes furnishing wavelengths from 300—500 nm. [Pg.507]

However, the optical train illustrated in Figure 22B allows the determination of fluorescence quenching. The interfering effect described above now becomes the major effect and determines the result obtained. For this purpose the deuterium lamp is replaced by a mercury vapor lamp, whose short-wavelength emission line (2 = 254 nm) excites the luminescence indicator in the layer. Since the radiation intensity is now much greater than was the case for the deuterium lamp, the fluorescence emitted by the indicator is also much more intense and is, thus, readily measured. [Pg.33]

Sensitized by Acetophenone. A -butanol solution of (114) (2.10 M) and acetophenone (0.8 M) is irradiated for 6 hr at 30° under nitrogen with a Hanau Q 81 high-pressure mercury lamp through a Pyrex-acetone filter (path length 1 cm, cut-off of wavelengths below 3270 A). Better than 98 % of the incident light is absorbed by the acetophenone. A 70% conversion of (114) to the same products as listed above is observed. The ratio (118) (120) is again -2 1. [Pg.322]

Before each wavelength scan, the grating locates itself by finding the 365 nm triplet of a built-in mercury light source, and then moves sequentially to the wavelengths for the elements to be determined. As an option the instrument... [Pg.777]

As mentioned previously (11), the wavelength position and stability of spectral lines from xenon or mercury excitation sources of spectrofluorometers may be variable with time-, and such sources are difficult to use with certainty for the calibration of monochromators. ... [Pg.100]


See other pages where Wavelengths mercury is mentioned: [Pg.248]    [Pg.147]    [Pg.291]    [Pg.248]    [Pg.147]    [Pg.291]    [Pg.311]    [Pg.344]    [Pg.1178]    [Pg.2962]    [Pg.428]    [Pg.776]    [Pg.115]    [Pg.122]    [Pg.123]    [Pg.203]    [Pg.15]    [Pg.191]    [Pg.194]    [Pg.424]    [Pg.432]    [Pg.433]    [Pg.23]    [Pg.9]    [Pg.397]    [Pg.214]    [Pg.420]    [Pg.381]    [Pg.64]    [Pg.257]    [Pg.743]    [Pg.15]    [Pg.253]    [Pg.288]    [Pg.329]    [Pg.339]    [Pg.174]    [Pg.35]    [Pg.676]    [Pg.735]    [Pg.736]    [Pg.322]    [Pg.163]    [Pg.174]    [Pg.168]    [Pg.128]    [Pg.136]   
See also in sourсe #XX -- [ Pg.620 ]




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Mercury, atomic wavelength

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