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unit zI+1+j have a weight of 1 Hence, the activation value yj is simply copied to zI+1+j It is, however, possible to have weights not equal to 1, in which case the in uence of previous states is weighted Determining such weights adds additional complexity to the training step Each output unit s activation is then calculated as ok,p = fok

The combination gives rise to disturbances which are described as E x D E1x 0 cos (2 t C 1x ) C E2x 0 cos (2 t C 2x ) , E y D E1y 0 cos 2 t C 1y C E2y 0 cos 2 t C 2y These latter two equations can be contracted to E x D E x 0 cos 2 t C x , E y D E y 0 cos 2 t C y , where, (E x 0 )2 D fE1x 0 cos 1x C E2x 0 cos 2x g2 C fE1x 0 sin 1x C E2x 0 sin 2x g2 , 2 2 (E y 0 )2 D E1y 0 cos 1y C E2y 0 cos 2y C E1y 0 sin 1y C E2y 0 sin 2y , tan x D fE1x 0 sin 1x C E2x 0 sin 2x g / fE1x 0 cos 1x C E2x 0 cos 2x g , tan y D E1y 0 sin 1y C E2y 0 sin 2y / E1y 0 cos 1y C E2y 0 cos 2y Thus, as can be seen from (323) and (324), combinations of orthogonally resolved classical coherent waves, with particular polarization forms, lead to a pair of classical waves with a new resultant polarization form (323) (324) (321) (322)

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vji zi,p ) (317)

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wkj fyj (

It is impossible here to provide all the material required to appreciate fully the physics and mathematics associated with scattering within astrophysical situations There are several texts available which comprehensively cover these matters However, it is important that scattering mechanisms are understood to some degree in respect of their polarigenic potential As it turns out, some of the algebra used to formulate scattering processes has overtones with the Jones calculus When radiation encounters assemblies of small particles such as dust within circumstellar envelopes, electron clouds in extended dissociated stellar atmospheres, or dust in the interstellar medium, the interaction causes it to be scattered Generally the scattering is not isotropic with the amplitudes of the waves being dependent on the angle of emergence with respect to the original direction of incidence In addition, the scattering is also sensitive to polarization By de ning some plane associated with any incoming radiation, the waves may be resolved in directions perpendicular ( ) and parallel (k) to this plane Thus, the orthogonal vibrations may be written as E D E o cos (2 t C ) , Ek D Ek o cos 2 t C k (325) (326)

where (zI+2,p , , zI+1+J,p ) = (y1,p (t 1), , yJ,p (t 1))

Figure 34 Jordan Simple Recurrent Neural Network Jordan SRNNs [428], on the other hand, make a copy of the output layer instead of the hidden layer The copy of the output layer, referred to as the state layer, extends the input layer to z = (z1 , , zI+1 , zI+2 , , zI+1+K ) (318)

Fig 32 Radiation travelling along the z-axis hits an assembly of scattering particles positioned in the x y-plane and is scattered in a direction given by ,

www.appforge.com Borland Borland offers C++BuilderX Mobile Edition and JBuilder Mobile Edition as well as the more recent Borland Mobile Studio for developers that want to develop rapidly on Symbian OS using C++, Java or both. These multi-platform IDEs offer on-target debugging, GUI RAD and a unifying IDE for Symbian OS SDKs and compilers. www.borland.com Forum Nokia In addition to a wide range of SDKs, Forum Nokia also offers various development tools to download, including the Nokia Developer Suite for J2ME, which plugs in to Borland s JBuilder MobileSet or Sun s Sun One Studio integrated development environment. www.forum.nokia.com Metrowerks Metrowerks offers the following products supporting Symbian OS development:

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