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Scattering residual elastic

Thus, the corrections to the velocities Cpb (r) and Csb (r) on the first iteration can be obtained by correlating the back-propagated scattered elastic field with the derivatives of the incident field U (r,t). This transformation is similar to wavefield migration described previously. Thus we see that elastic field inversion can be constructed by iterative migration of the residual elastic data. [Pg.526]

Figure 9.12. FT-Raman spectrum of solid sulfur, obtained with a Bruker 66 FTIR and Raman attachment. Filter rejection band blocks Raman shifts from -f-55 to —130 cm. Small feature at zero shift is the residual elastic scatter transmitted by the rejection filter. Figure 9.12. FT-Raman spectrum of solid sulfur, obtained with a Bruker 66 FTIR and Raman attachment. Filter rejection band blocks Raman shifts from -f-55 to —130 cm. Small feature at zero shift is the residual elastic scatter transmitted by the rejection filter.
Lovesey (1). We are interested in elastic scattering from spin-only systems where, for discussing magnetic scattering at low x at least, residual orbital effects introduced via spin-orbit coupling may be accounted for by a factor g/2 associated with the form factor, where the g-factor may be determined by magnetic resonance measurements. [Pg.27]

In discussing the alternative theoretical approaches let us limit ourselves to those which have been applied directly to processes in which we are interested in this article, but first of all let us stress once more the importance of the work of Delos and Thorson (1972). They formulated a unified treatment of the two-state atomic potential curve crossing problem, reducing the two second-order coupled equations to a set of three first-order equations. Their formalism is valid in the diabatic as well as the adiabatic representation and also at distances of closest approach near Rc. Moreover the problem of the residual phase x(l) is solved implicitly. They were able to show that a solution of the three first-order classical trajectory equations is not sensitive to all details of the potentials and the coupling term, but to only one function which therefore can be used readily for modelling assumptions. The resulting equations should be solved numerically. Their method has been applied now to the problem of the elastic scattering of He+ + Ne (Bobbio et at., 1973) but unfortunately not yet to any ionization problem. [Pg.480]

The lifetime of the beam is influenced by many factors. The dominant beam loss mechanism results from collisions of the electrons with residual gas molecules in the machine vacuum. Both inelastic and elastic scattering can take place off the nuclei and orbital electrons of the gas molecules. The beam lifetime is inversely proportional to the vacuum pressure that can be achieved. After the start-up of a new storage ring, or one for which the vacuum has been let up to atmosphere and then the ring pumped down and baked, the lifetime will be poor. However, it will improve with operation. This is because the gas molecules adsorbed to the vacuum vessel surfaces are desorbed by the SR itself. [Pg.109]

The advent of undulators (see section 4.10) requires the pole pieces of these insertion devices to be brought close together for short wavelength emission. There is a limit to how small the gap can be made because small apertures limit the lifetime primarily due to elastic Coulomb scattering of electrons off the residual gas molecules. [Pg.109]

There are no reports of the elastic or inelastic scattering of protons in N . Strong resonances are however found in the (p a) and (p y) reactions. In the former reaction there are, in analogy with the same process in other nuclei of mass (4n —1), strong transitions to both the ground and first excited state (2 ) of the residual even-even nucleus (C ). Resonance information for some of the levels is given in Table 6. [Pg.84]

For obvious reasons there are no measurements of y-Ce at low temperatures. It is, however, believed that the residual quasi-elastic line width would only be a few meV and an inelastic crystal field transition would be observable. This can be inferred from the results of inelastic neutron scattering experiments on Ceo.g-xLa Thg.i (for x = 0.14, 0.20, 0,40) by Grier et al. (1980, 1981). The addition of La suppresses the y->a transition of Ceo.gThg j. The spectra below IlOK were... [Pg.49]


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See also in sourсe #XX -- [ Pg.445 , Pg.447 , Pg.457 ]




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Elastic scattering

Scatter elastically

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