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Light scattering optical thickness

It should be noted that scattering of light by particles can be measured using remote sensing techniques on satellites, from which such parameters as total aerosol optical thickness i.e., the exponent (bcxlL) in... [Pg.367]

The human red blood cell (erythrocyte) has a shape of biconcave disc with minimal (D ) and maximal (D ) thickness and radius R (Fig. 10.1a). The optical scheme of a reflected microscope with deposited red blood cells is shown in Fig. 10. lb. The light scattering process takes place at the interface of three media air-erythrocyte-substrate with refractive index n, n and n respectively. Since the erythrocyte thickness is of the same order of magnitude as the wavelength of incidental light, the interference phenomena take place on these blood cells. The reflective capacity of an interface between two media with refractive indices n, and n is described by Eq. 10.1 [10] ... [Pg.101]

In vivo RRS spectroscopy of the macula can take advantage of favorable anatomical features of the tissue structures encountered in the excitation and light scattering pathways. The major site of macular carotenoid deposition is the Henle fiber layer, which has a thickness of only about 100 pm, and to a lesser extent the plexiform layer (Fig. 12.8). Considering that the optical density of MP in the peak of the absorption band is typically quite a bit smaller than 1, as determined from direct absorption measurements of MP in excised... [Pg.302]

From a theoretical point-of view, significantly higher current densities are feasible, but require further improved front TCO films and perfect mirrors as back reflectors. This is illustrated by the dotted curve in Fig. 8.28, which shows simulations of quantum efficiency for a 1 pm thick pc-Si H solar cell. These simulations reveal a current potential of 29.2 mA cm-2 by improved optical components like reduced parasitic absorption in the front TCO, ideal Lambertian light scattering, dielectric back reflectors, and antireflection coatings on the front side [147]. However, this still has to be achieved experimentally. [Pg.402]

Intermediate. Most of the scattered light in intermediate systems has been scattered many times, but some unscattered fight emerges from the sample [6]. A typical application would be a plastics operation that works with pigments and general-purpose polystyrene. Most systems that are typically assumed to fall into the optically thin and optically thick areas are actually intermediate media. Classically, offset... [Pg.52]

Optically Thick. All the light has been multiples scattered [6]. A paint manufacturer preparing opaque coatings, where titanium dioxide is blended with other scattering pigments to create a color, would be considered an optically thick system. [Pg.53]

The optical effects of aerosols are spectacular. Clouds, haze, and smoke all appear as they do because of the optical properties of the individual particles and the effects of these particles on each other. Few people are not affected by the drama of light scattering and absorption brilliant sunsets inspire, myriad cloud colors excite, and dense, thick fogs disorient. [Pg.341]

Figure 1.5 Left panel the young, accreting star-disk system HH30 seen edge-on at visible wavelengths. The optically thick disk occults the star and the scattered light image shows the flaring disk surface. The system also drives a powerful jet (NASA/Space Telescope Science Institute, Burrows et al. 1996). Right panel debris disk around the 12 Myr-old low-mass star AU Mic. The disk is geometrically flat, optically thin and depleted in gas (NASA/ESA/STScI). Figure 1.5 Left panel the young, accreting star-disk system HH30 seen edge-on at visible wavelengths. The optically thick disk occults the star and the scattered light image shows the flaring disk surface. The system also drives a powerful jet (NASA/Space Telescope Science Institute, Burrows et al. 1996). Right panel debris disk around the 12 Myr-old low-mass star AU Mic. The disk is geometrically flat, optically thin and depleted in gas (NASA/ESA/STScI).
Satellite photometry Inversion of scattered light to infer optical thickness -h... [Pg.2019]

Following the grinding or CMP process, the oxide thickness was measured by the conventional measurement tool using optical interference and the planarity was characterized by the profilometer. For the defect analysis, the defect inspection tool based on light scattering and AFM was used. [Pg.20]


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See also in sourсe #XX -- [ Pg.136 , Pg.137 ]




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Optical light scattering

Optical scatter

Optical thickness

Scattering optical

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