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Radiation, angular distribution polarization

The characterization of a system from the hght it scatters is an inverse problem, i.e., a procednre to obtain information of the scattering system from the electromagnetic properties of the scattered radiation intensity, angular distribution, polarization, etc. [Pg.176]

The discovery of confinement resonances in the photoelectron angular distribution parameters from encaged atoms may shed light [36] on the origin of anomalously high values of the nondipole asymmetry parameters observed in diatomic molecules [62]. Following [36], consider photoionization of an inner subshell of the atom A in a diatomic molecule AB in the gas phase, i.e., with random orientation of the molecular axis relative to the polarization vector of the radiation. The atom B remains neutral in this process and is arbitrarily located on the sphere with its center at the nucleus of the atom A with radius equal to the interatomic distance in this molecule. To the lowest order, the effect of the atom B on the photoionization parameters can be approximated by the introduction of a spherically symmetric potential that represents the atom B smeared over... [Pg.37]

The angular distribution of the X-ray radiation, integrated between 70 and 200 eV and measured in the plane of the laser polarization, is displayed in Fig. 11.5. It is found to be much broader than the theoretical width (10°) expected if the electron is considered to be initially at rest. It is also centered on the laser axis (9 = 0) instead of 23° for a0 = 5.6. Similar results were obtained at all the X-ray spectral bandwidths. However, as we have already discussed, the properties of the radiation produced depend on the parameters of the electrons [34]. The angular distribution is significantly modified,... [Pg.220]

We now consider the radiative decay of the excited ensemble of atoms. The angular distribution and polarisation of the emitted photons can be conveniently described in terms of the Stokes parameters I, t]i, t]2, and (Born and Wolf, 1970). The emitted photons can be observed in the direction n making polar angles 6 and azimuthal angles with respect to the collision frame (fig. 8.1). It is convenient to choose the coordinate system in which the direction of observation n of the radiation is chosen as the z axis. The polarisation vector of the photons is restricted to the plane perpendicular to n by the two unit vectors i = (0 + 90°, 0) and 2 = (0,light emitted in the direction n and I y) the intensity transmitted by a linear polariser oriented at an angle y with respect to the i-axis, then the Stokes parameters are defined by... [Pg.209]

Fluorescence polarization cannot attain the +1 theoretical limits for maximum beam polarization owing to the nature of the absorption and emission processes, which usually correspond to electric dipole transitions. Although the excitation with linearly polarized radiation favours certain transition dipole orientations (hence certain fluorophore orientations, and the so-called photoselection process occurs), a fairly broad angular distribution is still obtained, the same happening afterwards with the angular distribution of the radiation of an electric dipole. The result being that, in the absence of fluorophore rotation and other depolarization processes, the polarization obeys the Lev shin-Perrin equation,... [Pg.246]

Since synchrotron radiation is polarized, an anisotropic orientational distribution of molecules can be produced by core electron excitation. This distribution is determined by the orientation of the transition dipole moment with respect to the electric vector of the radiation. Information about this alignment and subsequent time evolution is eontained in the angular distributions of fragmentation products resulting from the excitation. Details have been worked out and described in several references for the case of valence electron excitation and ionization (Zare 1972 Yang and Bersohn... [Pg.23]

CP) Qjj-Quiaj-iy polarized radiation. The intensity difference means that a Circular Dichroism in the Angular Distribution of photoelectrons (CDAD) effect is present. [Pg.77]

The level of quality that has been achieved in OLEDs can be seen also from their radiation characteristics Fig. 11.13 shows the angular distribution of the emitted intensity in a polar diagram for the multilayer OLED (Figs. 11.9 and 11.10). Its... [Pg.379]

The dependence of the radiation pattern from dipoles uniformly distributed within a spherical particle of relative refractive index m = n /n2 = 2.0 upon the particle size is illustrated in Fig.4.9 where the angular distribution in the scattered intensity is plotted in arbitrary units for different values of the size parameter. The exciting radiation incident upon the particle is assumed to be horizontally polarized. There is a sharp increase in the differential scattering... [Pg.105]

The MO measurements provide information about the angular distribution of molecules in the x, y, and z film coordinates. To extract MO data from IR spectra, the general selection rule equation (1.27) is invoked, which states that the absorption of linearly polarized radiation depends upon the orientation of the TDM of the given mode relative to the local electric field vector. If the TDM vector is distributed anisotropically in the sample, the macroscopic result is selective absorption of linearly polarized radiation propagating in different directions, as described by an anisotropic permittivity tensor e. Thus, it is the anisotropic optical constants of the ultrathin film (or their ratios) that are measured and then correlated with the MO parameters. Unlike for thick samples, this problem is complicated by optical effects in the IR spectra of ultrathin films, so that optical theory (Sections 1.5-1.7) must be considered, in addition to the statistical formulas that establish the connection between the principal values of the permittivity tensor s and the MO parameters. In fact, a thorough study of the MO in ultrathin films requires judicious selection not only of the theoretical model for extracting MO data from the IR spectra (this section) but also of the optimum experimental technique and conditions [angle(s) of incidence] for these measurements (Section 3.11.5). [Pg.266]

The different values of AM correspond to different angular distributions of the radiation and to different polarization conditions. For AM = 0 only the z component of p = -er contributes and the radiation can be compared to that of a classical dipole oscillating along the direction of the field (quantization axis). The radiation then has an intensity which is proportional to sin, e being the angle between the field and the direction of... [Pg.49]


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See also in sourсe #XX -- [ Pg.271 ]




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