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Emissivity normal spectral

The spectral overlap integral J can be expressed in terms of either wavenumbers or wavelengths (Equation 2.36). The area covered by the emission spectrum of D is normalized by definition and the quantities / and lx are the normalized spectral radiant intensities of the donor D expressed in wavenumbers and wavelengths, respectively. Note that the spectral overlap integrals J defined here differ from those relevant for radiative energy transfer (Equation 2.33). Only the spectral distributions of the emission by D /,P and, are normalized, whereas the transition moment for excitation of A enters explicitly by way of the molar absorption coefficient sA. The integrals J" and Jx are equal, because the emission spectrum of D is normalized to unit area and the absorption coefficients sA are equal on both scales. [Pg.51]

Rate of Emission of Photons by the UV Lamp The rate of emission of photons by the lamp, so-called lamp characterization can be developed in the LTU, as described in Chapter III. In the LTU, a radiometer is placed at a fixed distance form the lamp s axis. A radiomenter correction factor of 1.41 (equation 3-1) is used which relates the tnie absolute reading to the lamp emission spectrum and the radiometer normalized spectral response. Thus the radiometric measurement allowed for the determination of the spatial distribution of the lamp radiative flux, qe y i. [Pg.67]

The identifier normal spectral emissivity indicates emittance normal to the surface and at a single wavelength (spectral). [Pg.321]

C. Cagran and G. Pottlacher, Physical Properties and Normal Spectral Emissivity of Iridium up to 3500 K, presented at 16 Symposium on Thermophysical Properties, Boulder, Co, USA, July 30 to August 4,2006, to be published in Int. J. Thermophys. [Pg.340]

Kobatake H, Khosroabadi H, Fukuyama H (2012) Normal spectral emissivity measurement of liquid iron and nickel using electromagnetic levitation in direct current magnetic Field. Metall Mater Trans A 43(7) 2466-2472... [Pg.98]

Emissivity is a thermophysical property related to optical energy transfer. The normal spectral emissivity is used for noncontact temperature measurement and the total hemispherical emissivity is used for estimating the energy transmitted from the melt surface by radiation. [Pg.113]

The normal spectral emissivity Sn was measured by Lange and Schenck at 650 nm for the first time [39]. Since then, over ten measurements have been reported [40-50], as shown in Fig. 4.12. Shvarev et al. [40] reported that thermal emission from molten silicon can be explained by Drude s free-electron model. Pulse lasers have been used to melt silicon. This method has advantages, in that measurement can be carried out in a very short time and a furnace is not required [42-44]. However, it is difficult to measure the sample temperature accurately as long as laser heating is employed. Recently, measurements using a cold crucible or levitator have been attempted these techniques assure measurement conditions without optical contamination, because there is no crucible wall at high temperature, which causes disturbing emission and reflection [47-50]. [Pg.113]

Kawamura et al. ]50] successfully measured the normal spectral emissivity over a wavelength range between 550 and 1600 nm using an electromagnetic levitation technique, which assures measurements for molten silicon in undercooled conditions from 1553 to 1797 K, as shown in Fig. 4.13. [Pg.113]

Fig. 4.12 Normal spectral emissivity of molten silicon at the melting point [39-50]. Fig. 4.12 Normal spectral emissivity of molten silicon at the melting point [39-50].
Fig. 4.13 Normal spectral emissivity measured at various wavelengths using levitation [50]. 4.4.2... Fig. 4.13 Normal spectral emissivity measured at various wavelengths using levitation [50]. 4.4.2...
H. Kawamura, H. Fukuyama, M. Watanabe, and Y. Hibiya, 2005, Normal Spectral Emissivity of Undercooled Liquid Silicon , Meas. Sci. Technol. 16, 386-393. [Pg.133]

The spectral emittance is defined as the ratio of the radiant power per unit area leaving the surface of a body at some given wavelength to that leaving a blackbody at the same temperature. The spectral emittance can be determined practically by comparing the observed or apparent surface temperature of a material with that of a blackbody cavity existing in the same material. The normal spectral emittance is a special case in which the viewing direction is normal to the smooth, opaque surface of the crystalline material. Emissivity is a property of the surface of real specimens. [Pg.192]

Several precautions can be taken to assure a good estimate of the tme surface temperature. As indicated in Eq. (8.5.1), the emissivity normally depends on the wavenumber. With a spectrometer or multichaimel radiometer one may search for a dispersion region of the surface material where the refractive index varies strongly with wavenumber (see Subsection 3.7.b). Near the index minimum the emissivity has a maximum. In addition to the composition the emissivity strongly depends on particle size and surface texture. A spectral search for an emissivity maximum is an improvement over the use of an arbitrarily chosen spectral interval. The maximum in the Martian brightness temperature near 1280 cm , shown in the upper spectrum of Fig. 6.2.8, may be an example of such a case. [Pg.387]

White Phosphorus Oxidation. Emission of green light from the oxidation of elemental white phosphoms in moist air is one of the oldest recorded examples of chemiluminescence. Although the chemiluminescence is normally observed from sotid phosphoms, the reaction actually occurs primarily just above the surface with gas-phase phosphoms vapor. The reaction mechanism is not known, but careful spectral analyses of the reaction with water and deuterium oxide vapors indicate that the primary emitting species in the visible spectmm are excited states of (PO)2 and HPO or DPO. Ultraviolet emission from excited PO is also detected (196). [Pg.271]

The spectral normal emissivity of Coming Code 7940 vitreous silica was computed from measurements of transmittance and reflectance at 25°C and is shown in Figure 8. The total normal emissivity of Code 7940 silica as a function of temperature from —200 to 1400°C is shown in Figure 9. [Pg.508]

FIG. 5-13 Hemispherical and normal emissivities of metals and their ratio. Dashed lines monochromatic (spectral) values versus r/X. Solid lines total values versus rT To convert ohm-centimeter-kelvins to ohm-meter-kelvins, multiply hy 10"l... [Pg.572]

In SXAPS the X-ray photons emitted by the sample are detected, normally by letting them strike a photosensitive surface from which photoelectrons are collected, but also - with the advent of X-ray detectors of increased sensitivity - by direct detection. Above the X-ray emission threshold from a particular core level the excitation probability is a function of the densities of unoccupied electronic states. Because two electrons are involved, incident and the excited, the shape of the spectral structure is proportional to the self convolution of the unoccupied state densities. [Pg.274]

Figure 10-10. (a) Semilogarillnnic plol of ihc stimulated emission transients for various excitation pulse energies measured for LPPP on glass. The excitation pulses have a duration of 150 fs and are centered at 400 nm. The probe pulse were spectrally filtered (Ao=500nin, Aa=l0nm). (b) Emission spectra recorded for the same excitation conditions. The spectra are normalized at the purely electronic emission baud (according lo Ref. [181). [Pg.173]

The emission line is centered at the mean energy Eq of the transition (Fig. 2.2). One can immediately see that I E) = 1/2 I Eq) for E = Eq E/2, which renders r the full width of the spectral line at half maximum. F is called the natural width of the nuclear excited state. The emission line is normalized so that the integral is one f l(E)dE = 1. The probability distribution for the corresponding absorption process, the absorption line, has the same shape as the emission line for reasons of time-reversal invariance. [Pg.10]

Sensitized emission (/ ), as defined in Eq. (7.8), reliably measures the relative amount of energy transfer occurring in each pixel (Fig. 7.2, lower right panel). Iss is corrected for spectral overlap (i.e., Problem 1 has been taken care of) however, unlike E, it is not a normalized measure for interaction nor is it quantitative in absolute terms. It depends on the specific biological question which of the two yields the most relevant information. [Pg.316]


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Spectral normalization

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