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Beam Calculator Module

The Beam Calculator Module generates the instrument beam as a function of the FTS and interferometric input parameters selected by the user, and the telescope parameters. The first derived parameter required is the interferometric angular resolution, AOj. For an interferometer with a maximum baseline bmax, the maximum [Pg.82]

For a single dish with a diameter Dtci the angular resolution is A S 1.22XminlDTeh 4nd the field of view at a given wavelength is FOV = 2A4X/DTei- The number of pixels required per FOV is [Pg.83]

The beam profile is a function of the wavelength and the required angular resolution ABmax, which defines the spatial span for the calculation of the illumination profile in (x, y). The telescope illumination can be written as [Pg.83]

This computed beam is then multiplied by the sky map. In order to avoid the interpolation or decimation of the sky map, these parameters can be used as an input for the simulation of the sky map itself. [Pg.83]

As an example, Fig. 4.5 shows the calculated normalised beam profile (right) for a given wavenumber and for a telescope diameter Dja = 3 m illuminated uniformly (left). [Pg.83]


The first step is to generate a Sky Map to be fed to the subsequent modules in the Sky Generator Module and the corresponding photon noise, computed in the Sky Photon Noise Module. In parallel, given the parameters defined by the user for the instrument, an interferometric MV-map is created at the v-Map Generator Module from the position of the two telescopes. The FTS Drive module calculates the spectrometer scan parameters. Once a MV-map and the scan parameters are defined, the instrument beam is calculated at the Beam Generator Module. The sky map and the beam are then combined to recreate the observed sky map. [Pg.75]

The back-calculation module used to compute layers elastic modulus requires data obtained from a Benkelman beam, a Lacroix deflectograph, or a FWD. [Pg.575]

Figure 4. Calculation of the modulation depth using the analytic model described in the text, with the lasers focused on the axis of the molecular beam (zm = 0). The dashed curve was obtained by setting pa — pi, at zm — 0. The solid curve is the maximum possible modulation depth, obtained by setting pa — pt, at an optimum location. Figure 4. Calculation of the modulation depth using the analytic model described in the text, with the lasers focused on the axis of the molecular beam (zm = 0). The dashed curve was obtained by setting pa — pi, at zm — 0. The solid curve is the maximum possible modulation depth, obtained by setting pa — pt, at an optimum location.
When a grating is used to excite the modes, usually the waveguide film is periodically modulated at the film/cover or film/substrate (or at both) interface (Fig. 15.4b). The incident beam illuminates this grating and one of the diffraction orders will excite the modes. The mode s effective refractive index can be calculated from the so-called grating equation10,30. [Pg.403]

Anyway, due to the limited precision of the EDP - intensity measurement, especially for the (100) reflection, which is too close to the central beam - this argument is not very strong and cannot reject the 1/3 substitution at all. To confirm the hypotheses of the proposed 2/3 substitution HREM observation in [001] and [021] zones were performed in parallel with multislice calculations, based on the 2/3 substitution. These projections are used because the fourfold modulation due to the Mo atoms is well expressed in them. The observed images are enhanced by a Fourier filter with Bragg mask to eliminate the noise frequencies. [Pg.432]

An approximate calculation for the differences in optical retardation for the central and the extreme ray of a beam-path which is diverging as it travels through the FTIR modulator, separated by a half-angle (in radians) of a, shows that the maximum allowable value of a to achieve a required resolution Av at a wavenumber of is ... [Pg.131]

Bell (1981) (see also Bell and Bickel, 1981) measured all matrix elements for fused quartz fibers of a few micrometers in diameter with a photoelastic polarization modulator similar to that of Hunt and Huffman (1973) the HeCd (441.6 nm) laser beam was normal to the fiber axes. Advantages of fibers as single-particle scattering samples are their orientation is readily fixed and they can easily be manipulated and stored. Two of the four elements for a 0.96-jtim-radius fiber are shown in Fig. 13.16 dots represent measurements and solid lines were calculated using an earlier version of the computer program in Appendix C. Bell was able to determine the fiber radius to within a few tenths of a percent by varying the radius in calculations, assuming a refractive index of 1.446 + iO.O, until an overall best fit to the measured matrix elements was obtained. [Pg.425]

As to the practical way of producing a suitable modulation, a series of proposals have been made. In practically all cases a modulator is introducted into the light beam, whereas the polarizing prisms are kept at rest. It appears that the general shape of the lower curve in Fig. 6.5 remains unchanged. More precise calculations can be carried out with the aid of a matrix calculus, as reviewed by Walker (216). [Pg.302]

We detected the saturated fluorescence emitted by a beam of 23S metastable atoms as they cross at right angle the slave laser light. A 1015 atoms/s.sterad flux of metastable helium atoms was produced by electronic collisions in a DC discharge of a helium atomic beam, similar to that described in [15]. To improve the precision of the linecenter determination, we increased the signal-to-noise ratio S/N by means of standard frequency modulation the third harmonic demodulated lineshape is shown in Fig. 4. The function expected for a Lorentzian spectrum was fit and linecenters were calculated with an uncertainty ranging between 10 kHz and 20 kHz, that is consistent with the observed S/N, mainly limited by the stability of the reference frequency and of the metastable helium beam. The reproducibility was two or three times worse than the uncertainty,... [Pg.318]

The measurement of optical activity in Raman spectra is most often done by measuring the circular intensity difference (CID) and the circular intensity sum (CIS). Using this technique the linearly polarized la.ser beam used for excitation is modulated with a KD P electrooptical modulator resulting in an excitating beam which changes its state of polarization from left to right circularly polarized at a frequency of about 1/3 Hz. The Raman intensities are then collected separately and the dimensionless Raman CID calculated using ... [Pg.561]

The exact measurement of the optical path in cells of low thickness is made by interferometry (interference pattern method). The transmittance of the empty cell is measured for an interval between two wavenumbers rq and (in cm ). Figure 10.22 shows that the beam S2 has undergone a double reflection from the internal walls of the cell, thus for a normal incidence, there would be, if 21 = kX, addition of both light intensities (the two beams Sj and S2 are in phase). As a function of the wavelength a modulation of the main beam Sj of a few percent is observed. After calculation, if N represents the number of interference fringes counted between rq and PJ (in cm ), then ... [Pg.235]

Figure 20. The 5j 12j dispersed fluorescence of ultracold anthracene in a supersonic beam. The available vibrational energy is 1792 cm1. The parameters of the optically active modes are given in Table II. The top figure is the experimental spectrum.60 The bottom figure is the emission in the harmonic approximation (y6.6 = 0). The calculation clearly fails to reproduce the broad redistributed emission. The middle figure was calculated with IVR [Eqs. (131)]. Only one b ) state (the ground vibrational state f/> = 0 was used. yt.t/y, = 40. The relaxed emission was calculated in the fast modulation limit [Eq. (116a)], with f0 = 2f = 75 cm-1.61... Figure 20. The 5j 12j dispersed fluorescence of ultracold anthracene in a supersonic beam. The available vibrational energy is 1792 cm1. The parameters of the optically active modes are given in Table II. The top figure is the experimental spectrum.60 The bottom figure is the emission in the harmonic approximation (y6.6 = 0). The calculation clearly fails to reproduce the broad redistributed emission. The middle figure was calculated with IVR [Eqs. (131)]. Only one b ) state (the ground vibrational state f/> = 0 was used. yt.t/y, = 40. The relaxed emission was calculated in the fast modulation limit [Eq. (116a)], with f0 = 2f = 75 cm-1.61...
Fig. 9.6. (a) Calculated image with only the incident beam and the four superstructure spots of type 011 inside the objective aperture (b) a similar experimental image where disorder of the image features caused by charge modulation is present, both incommensurability and out of phase boundaries. [Pg.224]

The differential cross sections of argon and neon have been measured by using refinements of the modulated molecular-beam technique. From these measurements the intermolecular potentials were found. These potentials differ significantly from the Lennard-Jones potential. The neon and argon potentials have different shapes and are not related by any simple scaling factor. The macroscopic properties have been calculated and are in reasonable agreement with experiment. The face-centered cubic structure was found to be the most stable crystal lattice for neon. The effect of the argon potential on the critical properties and saturation pressures is also discussed. [Pg.370]

The y-ray beam between a Mossbauer source and absorber can be frequency-modulated by passage through a y-transparent medium with an optical path length which varies with time. In this way the refractive index of the medium for the y-radiation can be calculated [17]. [Pg.82]


See other pages where Beam Calculator Module is mentioned: [Pg.82]    [Pg.89]    [Pg.82]    [Pg.89]    [Pg.242]    [Pg.461]    [Pg.48]    [Pg.94]    [Pg.184]    [Pg.67]    [Pg.5]    [Pg.37]    [Pg.465]    [Pg.271]    [Pg.955]    [Pg.6570]    [Pg.401]    [Pg.457]    [Pg.57]    [Pg.103]    [Pg.294]    [Pg.183]    [Pg.93]    [Pg.97]    [Pg.565]    [Pg.224]    [Pg.225]    [Pg.381]    [Pg.279]    [Pg.6569]    [Pg.607]    [Pg.457]    [Pg.116]   


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Calculation module

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