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Polarisability wavelength dependence

Simple systems such as that shown in Fig. 5.11 yield an excellent optical efficiency, and are almost free of pulse dispersion and wavelength-dependent pulse shift. Another benefit is that the detection path is almost free of polarisation effects compared to monochromator-based systems. The high numerical aperture of the light eollection system further reduces the influence of the rotational relaxation see Fig. 5.9. With aspheric lenses an NA of around 1 can be achieved, and at an NA this high the polariser in the detection path can often be omitted. In the setup in the left graphic of Fig. 5.11, residual depolarisation effects can be removed by slightly tilting the polarisation direetion of the laser. [Pg.73]

Moreover, the fraction of the light diffracted into the first order depends on the wavelength. If a grating monochromator or polychromator is used to record a spectrum, the wavelength dependence of the efficiency needs to be calibrated. The diffraction efficiency of a grating also depends on the polarisation of the light. [Pg.281]

Fig. 7.4 - Wavelength dependence of (l// )(d/ /d0) for strongly and weakly adsorbed hydrogen p-polarised light with 45° angle of incidence. Fig. 7.4 - Wavelength dependence of (l// )(d/ /d0) for strongly and weakly adsorbed hydrogen p-polarised light with 45° angle of incidence.
Before going further, it may be noted that the flipping ratio does not depend either on the Lorentz factor or on absorption in the sample. Certain instrumental parameters such as the polarisation of the neutron beam for the two spin states, the half wavelength contamination of the neutron beam and the dead-time detector can readily be taken into account when analysing the data. On the other hand, the extinction which may occur in the scattering process is not so easy to assess, but must also be included [14]. Sometimes, it is even possible to determine the magnetisation density of twinned crystals [15]. [Pg.247]

An integral part of a fibre optic sensor is the light source. Its primary task is to deliver an appropriate light, which possesses such features as an optical power suitable to interact with an analyte or an indicator from the optrode, a wavelength matched to the spectral properties of the sensors in order to obtain the highest sensitivity, and, in dependence on the construction of the sensor, polarisation, short pulse etc. There are many various light sources utilised in the fibre optic chemical sensors. They differ in spectral properties, generated optical power and coherence. [Pg.51]

When the electric field strength of the incident light is ED, the induced dipole will be m, = aE0 where a is the optical polarisability. The electric field strength of radiation scattered by the induced dipole Es, depends on second derivative of m1 with respect to time. The useful experimental quantities are intensities of scattered light (Is) and incident important light (is). These are respectively proportional to Es2 and E02, averaged over a vibrational period, i.e., from time t = 0 to 10/C, where 1 is wavelength of... [Pg.112]

In order to derive these we will consider an adiabatic evacuated enclosure, like that shown in Fig. 5.19, with walls of any material. In this enclosure a state of thermodynamic equilibrium will be reached The walls assume the same temperature T overall and the enclosure is filled with radiation, which is known as hollow enclosure radiation. In the sense of quantum mechanics this can also be interpreted as a photon gas in equilibrium. This equilibrium radiation is fully homogeneous, isotropic and non-polarised. It is of equal strength at every point in the hollow enclosure and is independent of direction it is determined purely by the temperature T of the walls. Due to its isotropic nature, the spectral intensity L x of the hollow enclosure radiation does not depend on / and universal function of wavelength and temperature L x = L x X,T), which is also called Kirchhoff s function. As the enclosure is filled with the same diffuse radiation, the incident spectral intensity Kx for every element of any area that is oriented in any position, will, according... [Pg.524]

Another useful method, especially when only a single wavelength is available, is the different dependence of Y and surface electric field on the polarisation and angle of incidence.72 From the Fresnel equations and the known optical constants of metals the electric field experienced by the adsorbate and the absorbance of the substrate can be calculated. 72.73 por substrate excitation Y should follow (1-R). For adsorbate excitation some knowledge (or model) of the symmetry of the adsorbate layer (orientation of transition dipole) is required to relate the electric field to the excitation probability. The angle of incidence dependence of Y for different input polarisations have been calculated for some typical cases.72.74 Cavanagh s group have... [Pg.501]

The principle shown in Fig. 5.100 ean be extended to more than two start detectors. The photons can be separated depending on their wavelength or polarisation. The photons of different channels ean be used as start ehannels and be correlated with the photons in a common stop channel. The TCSPC system uses a router to combine the events in the start ehannels into a eommon timing pulse line, see Fig. 5.104. [Pg.173]


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See also in sourсe #XX -- [ Pg.320 ]




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Polarisability

Polarisable

Polarisation

Polariser

Wavelength dependence

Wavelength-dependent

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