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Adaptive linear element

Between 1959 and 1960, Bernard Wildrow and Marcian Hoff of Stanford University, in the United States developed the ADALINE (ADAptive LINear Elements) and MADELINE (Multiple ADAptive LINear Elements) models. These were the first neural networks that could be applied to real problems. The ADALAINE model is used as a filter to remove echoes from telephone lines. The capabilities of these models were again proven limited by Minsky and Papert (1969). The period between 1969 and 1981 resulted in much attention toward neural networks. The capabilities of artificial neural networks were completely blown out of proportion by writers and producers of books and movies. People believed that such neural networks could do anything, resulting in disappointment when people realized that this was not so. [Pg.913]

Because the present nonlinear method is an outgrowth of the linear ones, it is not surprising that such useful techniques as the reblurring discussed in Chapter 3 may be adapted. Other elements of Chapter 3 may be borrowed as well, including memory-conserving methods of programming (Section... [Pg.108]

W.R. Bowen and A.O. Sharif, Adaptive finite element solution of the non-linear Poisson-Boltzmann equation—a charged spherical particle at various distances from a charged cylindrical pore in a charged planar surface, J. Colloid Interface Sci. 187 (1997)... [Pg.541]

Various methods (described in Chapter 4) can be used to determine the symmetry of atomic orbitals in the point group of a molecule, i. e., to determine the irreducible representation of the molecular point group to which the atomic orbitals belong. There are two possibilities depending on the position of the atoms in the molecule. For a central atom (like O in H20 or N in NH3), the coordinate system can always be chosen in such a way that the central atom lies at the intersection of all symmetry elements of the group. Consequently, each atomic orbital of this central atom will transform as one or another irreducible representation of the symmetry group. These atomic orbitals will have the same symmetry properties as those basis functions in the third and fourth areas of the character table which are indicated in their subscripts. For all other atoms, so-called group orbitals or symmetry-adapted linear combinations (SALCs) must be formed from like orbitals. Several examples below will illustrate how this is done. [Pg.258]

Nanocrystalline TiOi has been used as prototypical elemental TM oxide with a distorted rutile phase. Most important are the spectra in Fig. 7 (XAS), Fig. 8 (VUV SE), and Fig. 10 (SXPS), and the comparisons of 3d-state splittings in Figs. 9(a) and (b) These assignments for Ti 3d, 4s and 4p atomic features in these specta have been compared with the Symmetry Adapted Linear Combinations (SALC s) atomic states approach of FA. Cotton in [13], and the modification of this to include covalency effects, in. [14 and 17]. [Pg.803]

Now to the problem in hand the use of symmetry-adapted linear combinations of the basis functions in the SCF procedure. The method is now obvious, it is simply one more additional step in the chain of transformations from the raw basis to the actual working basis. Deferring the actual technique of calculation of the elements of the transformation between the raw basis and the symmetry-adapted basis until later in this chapter, we assume that the matrix U effects this transformation. The matrix is actually unitary or, more commonly in the real case, orthogonal so that, unlike the monomial/harmonic transformation above, it does not disturb the orthogonality properties of the basis and it is, of course, square. [Pg.629]

Use the different sets of AOs on the ligands as basis sets to generate reducible representations known as symmetry-adapted linear combinations (SALCs). Any basis function that is unchanged by a given symmetry operation will contribute I to the character, any basis function that transforms into the opposite of itself will contribute — I, and any basis function that is transformed into a basis function on a different li d will be an off-diagonal element and contribute 0 to the character. [Pg.292]

Fig. 12. The relationship between the mean oceanic residence time, T, yr, and the seawater—cmstal rock partition ratio,, of the elements adapted from Ref. 29. , Pretransition metals I, transition metals , B-metals , nonmetals. Open symbols indicate T-values estimated from sedimentation rates. The sohd line indicates the linear regression fit, and the dashed curves show the Working-Hotelling confidence band at the 0.1% significance level. The horizontal broken line indicates the time required for one stirring revolution of the ocean, T. ... Fig. 12. The relationship between the mean oceanic residence time, T, yr, and the seawater—cmstal rock partition ratio,, of the elements adapted from Ref. 29. , Pretransition metals I, transition metals , B-metals , nonmetals. Open symbols indicate T-values estimated from sedimentation rates. The sohd line indicates the linear regression fit, and the dashed curves show the Working-Hotelling confidence band at the 0.1% significance level. The horizontal broken line indicates the time required for one stirring revolution of the ocean, T. ...
Fig. 11.13. Left panel projected heavy-element abundance Zp along lines of sight as a function of galactocentric distance, for differing values of the mass fraction in the form of stars at the onset of a terminal galactic wind. Right panel (mass-weighted) mean abundance as a function of final total stellar mass, for two different assumptions as to the dependence of the amount of gas lost on the initial mass. The assumed bulk yield is 0.02 and the trend along the linear part of the curves is approximately Z a M3/8. Adapted from Larson (1974b). Fig. 11.13. Left panel projected heavy-element abundance Zp along lines of sight as a function of galactocentric distance, for differing values of the mass fraction in the form of stars at the onset of a terminal galactic wind. Right panel (mass-weighted) mean abundance as a function of final total stellar mass, for two different assumptions as to the dependence of the amount of gas lost on the initial mass. The assumed bulk yield is 0.02 and the trend along the linear part of the curves is approximately Z a M3/8. Adapted from Larson (1974b).
Therefore, for large optimal control problems, the efficient exploitation of the structure (to obtain 0(NE) algorithms) still remains an unsolved problem. As seen above, the structure of the problem can be complicated greatly by general inequality constraints. Moreover, the number of these constraints will also grow linearly with the number of elements. One can, in fact, formulate an infinite number of constraints for these problems to keep the profiles bounded. Of course, only a small number will be active at the optimal solution thus, adaptive constraint addition algorithms can be constructed for selecting active constraints. [Pg.249]


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