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Digital Image Transfers . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 236 Personal Video Recorders . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 237 Video Files and Formats . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 242
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10.2 SELF-PUMPED PHASE CONJUGATION BY JOINT STIMULATED SCATTERING 10.2.1 Geometrical features of joint stimulated scattering The principle of joint stimulated scattering can be explained by simultaneous formation of the same scattering gratings dn13 dn24 by two pairs of optical waves: strong (pumping) waves E1,2 and scattering waves E3,4: dn13 * E1 E3 , dn24 * E2 E4 (Fig. 10.1). To have a single grating, coupling all four optical beams, it is required that the wave vector synchronism be ful lled (or almost ful lled): ~ ~ ~ ~ ~ k3 k1 q k4 k2 (1)
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Internationalization and Localization . . . . . Preparing Applications for Multiple Languages An NLS example . . . . . . . . . . . . . . What it all means . . . . . . . . . . . . . . Formatting Locale-Specific Output . . . . . . . Changing the locale . . . . . . . . . . . . Locale-specific formatting . . . . . . . . . Properties of locales . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
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Estimation of straight-line parameters from Poisson distributed observations. Let the estimation problem be that of Example 5.2. In that example, the observations have a Poisson distribution, which is a linear exponential family of distributions. The expectation model is the straight line. Therefore, the expectations of the observations are described by (5.281) E ~ =, X T e = el(,, + ez where 2 = (En l)T the nth measurement point. The observations are independent and, , is since they are Poisson distributed, their variance is equal to their expectation. Therefore,
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Absorption: An atom or molecule has many di erent energy levels. When the atom or molecule absorbs a photon, its energy is increased by an amount equal to the energy of the photon. The atom or molecule then enters an excited state. Hence, absorption is the process by which the energy of a photon is taken up by another entity, for example, by an atom that makes a transition between two electronic energy levels; the photon is destroyed in the process. Spontaneous emission: This is the process by which matter may lose energy, resulting in the creation of a photon. Stimulated emission: This is the process by which, when perturbed by a photon, matter may lose energy, resulting in the creation of another photon. The perturbing photon is not destroyed in the process and the second photon is created with the same frequency and phase as the original. Stimulated emission is a quantum mechanical phenomenon. The process can be conceived as optical ampli cation, and it forms the basis of the laser (these mechanisms are used, for example, in EDFAs). In a linear material the amount of charge displacement is proportional to the instantaneous magnitude of the electric eld. The charges oscillate at the same frequency as the frequency of the incident light. Either the oscillating charges radiate light at that frequency or the energy is transferred into nonradiative modes that result in material heating (or other energy transfer mechanisms). Generally, the radiated light travels in the same direction as the incident light beam: The light is e ectively bound to the material; the light excites charges that reradiate light that excites charges; and so on. As a result, the light travels through the material at a lower speed than it does in vacuum. If the motion of some of the charges within the material decays without giving o light, some of the light intensity is lost from the incident beam by scattering and absorbance. The absorbance is de ned as the ratio of light exiting a material to the light incident into the material divided by the material thickness. Both the absorbance and refractive index (ratio of speed of light in vacuum to the speed of light in the material) are linear optical properties of a material for low-intensity incident light [377]. In a nonlinear optical material, the displacement of charge from its equilibrium value is a nonlinear function of the electric eld (e.g., see Fig. 5.9). All materials when exposed to a high enough light intensity show a nonlinear response. Nonlinearity in optics occurs when the electromagnetic wave is large enough such that the medium responds not only at the fundamental driving frequency but also at higher harmonics. For small forces, the displacement of the charge is small and is approximated by a harmonic potential. When the displacement away from equilibrium is large, the harmonic approximation breaks down and the force is no longer a linear function of the displacement. When the charges in a molecule are bound by a harmonic potential, the induced dipole moment is linear in the applied eld. The response of a molecule is nonlinear if the charges are bound to the molecule by a nonharmonic potential. In this case, the dipole moment of the molecule is a nonlinear function of applied electric eld. More generally, if a nonlinear molecule is exposed to light, the time-dependent induced dipole moment is a nonlinear function of the time-dependent electric eld [377].
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A combination of efforts from different sectors of lm producers, farmers, and municipalities will be needed to resolve this problem [60, 61]. The various solutions to curtail the problems of plastic lm waste disposal include: 1. Waste reduction of plastic lms by farmers. 2. Means to make recycling viable and economical for the farmers need to be determined. 3. Finding cost-effective ways to collect, clean, and store the material and nding end markets for the recycled products.
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Evaluate Application Requirements Evaluate Hardware Infrastructure Evaluate Storage Requirements Evaluate Networking Requirements Evaluate Operations Requirements Evaluate Risk
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T h e t i m e correlation f u n c t i o n : p h ( A t ) = R h ( 0 , At) quantifies the time varying nature of the channel. Its Fourier transform is the Doppler power spectrum @ ~ ( z I= F { p h ( A t ) } . The nominal width of @ h ( U ) , termed the ) Doppler spread B D ,is defined as the range of frequencies over which the Doppler spectrum is essentially non-zero. The inverse of the Doppler spread,
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Open Web Page tool. Clicking the tool opens a dialog box where a URL can be supplied for converting Web pages to PDF files. Save tool. The tool exists for both Reader and Acrobat. In Acrobat, files changed can be saved while Reader is capable of only saving a copy of the PDF. E-mail tool. The open PDF file is automatically attached to an e-mail message. Clicking the tool launches your e-mail application and attaches the file.
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On the CD-ROM The drawing used in the following exercise on matching properties, ab11-f.dwg, is in the Drawings folder on the CD-ROM.
When Convert to Adobe PDF is accessed via the tool in the toolbar or the menu option in the Acrobat menu, a dialog box appears where the filename and destination can be determined. Supply a name and destination and the file is saved as a PDF. The PDF can be viewed immediately by choosing Acrobat View Results in Acrobat or by later opening it in an Acrobat viewer. When the PDF is open in Acrobat, click the Navigation pane tool to open the bookmarks. If the file has been successfully converted and the structure preserved, the display should appear, as shown in Figure 6-16.
The context stage of risk management is similar to that for any project, although the criteria and consequence scales may be more specific to environmental matters, and the elements for structuring the process may be tailored to have a particular environmental focus.
'The Early Universe', E. W. Kolb and M. S. Turner, Addison-Wesley, Redwood City. 1994 (paperback edition): A detailed study of the dynamics and thermodynamics of the Big Bang cosmology. followed by material focusing on possible physics of the very early Universe. 'Principles of Physical Cosmology', P. J. E. Peebles. Princeton University Press. 1993: An account of Big Bang cosmology. strong on historical detail. followed by highly detailed studies of the origin of structure in the Universe. 'Cosmology: the Origin and Evolution of Cosmic Structure'. P. Coles and F. Lucchin. Wiley. Chichester. 2002 (2nd ed): Again, a book primarily concerned with structure formation in the Universe. but including some material on the Big Bang cosmology itself. 'Cosmological Physics', J. A. Peacock, Cambridge University Press, 1999: An extremely lucid account of many aspects of cosmology. both the Big Bang and structure formation, mostly at postgraduate level. 'Cosmological Inflation and Large-Scale Structure', A. R. Liddle and D. H. Lyth. Cambridge University Press, 2000: I can't resist mentioning my other book, a highly-technical account of all aspects of the inflationary cosmology. However there is a significant gap in level between the end of this book and the start of that one, which one of the above books would be needed to fill.
and by (5.316) and (5.317),
* Assumes adequate echo control. ** Exact values depend on speci c codec, but assumes use of a packet loss concealment algorithm to minimise e ect of packet loss. *** Quality is very dependent on codec type and bit-rate. **** These values are to be considered as long-term target values which may not be met by current technology. PLR Packet loss ratio.
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