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Titlebook: Machine Learning of Natural Language; David M. W. Powers,Christopher C. R. Turk Book 1989 Springer-Verlag London Limited 1989 artificial i

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Computer Science and Artificial Intelligence,terministic rules which largely eliminate the search component and reduce the generality of the systems. But the addition of a general Problem Solving or Machine Learning component returns such systems to the fold of heuristic search. Such systems differ in the way they are read, taught and criticiz
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Book 1989ained in literature. He moved into linguistics, and then into computational linguistics. In 1983 he took a sabbatical in Roger Shank‘s AI project in the Computer Science Department at Yale University. Like an earlier visitor to the project, John Searle from California, Christopher Turk was increasin
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nd hence elusive, radiative equilibrium. It is elusive partly because Earth’s overwhelming external boundary condition, solar irradiance, is never constant thanks to continuous variations in both orbit about the Sun and solar output. As such, the best Earth, and any other planet, can do is achieve a
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David M. W. Powers ThC(Hons), PhD, MACS, MIEEE,Christopher C. R. Turk MA (Cantab), DPhil (Sussex)s. Using polarization, investigators may, firstly, upgrade information capacity of signals and, secondly, develop polarization-based methods to discriminate a useful signal. The very first calculations to find information content of visible radiation polarization scattered by a cloud were performed
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David M. W. Powers ThC(Hons), PhD, MACS, MIEEE,Christopher C. R. Turk MA (Cantab), DPhil (Sussex)ce in Newton’s law of gravity or in Coulomb’s law yields a simple, radially symmetric force field ∼ 1/r.. The isotropy of space in such a force field entails a dynamic symmetry, namely conservation of angular momentum. The point-source concept constitutes a drastic simplification compared to the sou
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David M. W. Powers ThC(Hons), PhD, MACS, MIEEE,Christopher C. R. Turk MA (Cantab), DPhil (Sussex) scanners for wafer inspection [.]. More recent applications include laser cleaning [.], scanning near-field optical microscopy (SNOM) [.] and plasmon resonances effects in surface-enhanced Raman spectroscopy (SERS) [.]. Several studies have addressed this scattering problem using different methods.
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David M. W. Powers ThC(Hons), PhD, MACS, MIEEE,Christopher C. R. Turk MA (Cantab), DPhil (Sussex)haracterize the scattering properties is to consider how the brightness and polarization of scattering depend on the wavelength λ of incident light and the geometry of observations. The geometry is often characterized by the phase angle α which is defined as the source-object-detector angle. Instead
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David M. W. Powers ThC(Hons), PhD, MACS, MIEEE,Christopher C. R. Turk MA (Cantab), DPhil (Sussex)har in the 1940s (.;.). Using a formulation in terms of the Stokes vector for polarized light, Chandrasekhar was able to solve completely the polarization problem for an atmosphere with Rayleigh scattering, and benchmark calculations from the 1950s are still appropriate today (.). The scalar (intens
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