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UV wavelength

Nonoxide NLO ceramics include Si and compound semiconductors (qv) having the silicon stmcture, eg, GaAs, InP, and InSb, as weU as ferroelectrics such as SbSI. These materials tend to be more highly nonlinear than oxide ceramics, although lack of transparency at visible and uv wavelengths prevents them from competing with the oxides for the same appHcations. [Pg.338]

Acetone is a moderately polar molecule that can hydrogen-bond with water. Which electronic state of acetone would be stabilized more by moving the molecule from hexane to water Will this shift the n Tt transition to longer or shorter UV wavelengths Explain. [Pg.260]

The use of UV adsorption enhancers as reagents that introduce a UV chromaphore into a molecule that is transparent in the UV wavelength range has already been briefly discussed. The two most common reagents are the phenyl and methyl isothiocyanates. These reagents react with amino acids to form thiodantoins. [Pg.241]

The backside passivation processes are most critical for the blue and UV wavelengths. For 0.5-0.7 pm light, high QE is more easily attained - the absorption depth is a few microns, and photons penetrate beyond the backside... [Pg.140]

Since the early 1990s an increasing number of papers has been devoted to the application of CE for the analysis of both inorganic cations [906-915] and low-molecular-mass anions [915-922]. Standard CE methods have been developed and validated for determining inorganic anions (e.g. chloride, sulfate and nitrate), small carboxylic acids and metal ions that all have limited or no UV absorbance. In those situations, short UV wavelengths (190 nm) or indirect UV detection should be used. Such methods might be extended to metallic... [Pg.277]

RF, r.f. rms Radiofrequency Root mean square UV-C UV wavelength range 200-280 nm... [Pg.770]

Consider continuous radiation with specific intensity I incident normally on a uniform slab with a source function 5 = Bv(Tex) unit volume per unit solid angle to the volume absorption coefficient Kp and is equal to the Planck function Bv of an excitation temperature Tcx obtained by force-fitting the ratio of upper to lower state atomic level populations to the Boltzmann formula, Eq. (3.4). For the interstellar medium at optical and UV wavelengths, effectively S = 0. [Pg.58]

Others have described modifications of these methods for various purposes. Hiscox (82) suggested the direct spec-trophotometric assay of CTC in either acid or alkaline solution at various UV wavelengths. The possible contamination of CTC with other tetracycline drugs was addressed by Chicearelli et... [Pg.130]

There are two types of detectors under UV/IR classifications. Both of the types respond to frequencies in the UV wavelength and IR in the CO2 wavelength. In both types simultaneous presence of the UV and IR signals must be available for alarm conditions. In the simple voting device an alarm is generated once both conditions are met. In the ratio device, satisfaction of the ratio between the level of UV signal received and IR signal received must also be achieved before an alarm condition is confirmed. [Pg.182]

High-sensitivity detection of non-chromophoric organic ions can be achieved by combining the power of suppressed conductivity detection with these columns. Suppressed conductivity is usually a superior approach to using refractive index or low UV wavelength detection. [Pg.44]

Although AS and AES can be detected at a low UV wavelength, sensitivity is lacking and a more suitable detection was achieved using indirect photometric detection, post-column colour formation reactions, or a pre-column derivatisation, suppressed conductivity detection and refractive index detection [1,42,43]. A comparison of detection limits for the determination of these anionic surfactants shows that photometric and conductivity detectors are better (picomole or nanogram range) than refractive index or fluorometry detectors by about a factor of 1000 [40],... [Pg.124]

There does not seem to be one definitive collection of measured data for various locations world wide, although quite a lot have been collected by Wypych [6]. Figures for total irradiation cannot be sensibly used because it is necessary to work with the irradiation at the more important UV wavelengths to make comparison with the artificial light sources. [Pg.46]

The short (UV) wavelength limit of the optical range is imposed by instrumental considerations (spectrophotometers do not usually work at wavelengths shorter than about 200 nm) and by the validity of the macroscopic Maxwell equations. These equations assume a continuous medium in other words, that there is a large number of ions within a volume of. The long (IR) wavelength limit of the optical range is basically imposed by experimental considerations (spectrophotometers work up to about 3000 nm). [Pg.4]

Photolytic. Ethion in hexane did not exhibit absorption at UV wavelengths >260 nm (Gore et al, 1971). [Pg.1581]


See other pages where UV wavelength is mentioned: [Pg.117]    [Pg.511]    [Pg.512]    [Pg.128]    [Pg.134]    [Pg.311]    [Pg.171]    [Pg.172]    [Pg.221]    [Pg.72]    [Pg.189]    [Pg.191]    [Pg.311]    [Pg.174]    [Pg.182]    [Pg.166]    [Pg.1338]    [Pg.562]    [Pg.770]    [Pg.770]    [Pg.295]    [Pg.296]    [Pg.277]    [Pg.304]    [Pg.531]    [Pg.480]    [Pg.138]    [Pg.248]    [Pg.207]    [Pg.390]    [Pg.21]    [Pg.165]    [Pg.616]   


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Fixed wavelength UV detectors

Multi-wavelength UV detectors

The Fixed Wavelength UV Detector

The Variable Wavelength UV Detector

UV radiations wavelengths

UV wavelength region

Variable wavelength UV detector

Wavelength-modulated UV-visible Reflectance Spectroscopy

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