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border of the l=2 phase edge may be thought of as the border of the opaque knife edge, and the reversal side of the l=2 phase edge may be considered to have a transmittance equal to unity, as on its clear side. Therefore, the shadow patterns associated with the l=2 phase edge are, from the point of view of geometrical optics, considered to be identical with the shadow patterns associated with the wire test. Upon analysis the boundaries of the shadow patterns are, then, identical to those presented in Section 8.2.2. Notice the similarity between the Foucault test drawings in Figure 8.9 and the phase-edge photographs of a comatic lens (kindly provided by Landgrave, 1974) in Figure 8.28. It has been reported (Vasil ev, 1971; Landgrave, 1974) that the dark lines of the shadow pattern associated with the l=2 phase edge are better contrasted against the background irradiance intensity than the dark lines associated with both the knife-edge test and the wire test. Thus, the sensitivity of the l=2 phase-edge test is greater than the sensitivity obtained when using an opaque knife edge or the wire test. The wire test photographs in Figures 8.29(a,b) should be compared with the phase-edge photographs, Figures 8.31(c,d), respectively, taken with the same aspherical mirror. Obviously, a formal analysis of the sensitivity is, indeed, more complicated, and it is not considered here. However, it is possible to show (Ojeda-Castaneda, 1976, 1979) that for aberrations smaller than the wavelength of the incident radiation, the l=2 phase edge will produce images with higher contrast than the images produced with the opaque knife edge. The treatment is repeated here. The modulating function for the phase-edge method is M x1 ; y1 & 1; 1; x1 < r1 x1 > r1 8:81

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of the arriving signals. Each user is then allocated a channel according to their angular positions. The downlink weights are then computed before transmission. Results show an increased spectrum efficiency by a factor of four when using a seven-element ULA array in an environment with 1.6 ps of RMS angular spread. It is also shown that in order to retain this spectral efficiency in environments

"clutter". These base-stations are often deployed with a smaller array a t reduced heights compared to macro-cell installations, for coverage of network 'hot spots'. Deployment of a macro-cell BS antenna array has the most demanding implementation requirements of the three BS types and is considered here. Installation issues include:

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The measurable height of the object is determined by the smaller of these two numbers, namely the coherence length of the source and the depth of eld of the interferometric objective. Other criteria, which are dependent on the measurement method used, may further limit the measurable height range. The measurable height range for methods in which the object is scanned through focus such as with confocal or white light interference pro lers is limited by the scanning range and the working distance of the objective. Measurable Slopes. The maximum of the measurable slope of the sample also depends on the NA of the objective. If light re ected from a sample with a high slope is not gathered by the objective, the slope can not be measured. A common assumption holds that slopes with a maximum 0.75NA return suf cient light to be measurable as long as fringes with suf cient contrast are created. For objects with rough surfaces higher slopes can be measured since diffuse surfaces allow some light to travel back to the objective. Table 15.2 gives the optical resolution predicted by the Sparrow criterion for 600 nm wavelength of the source along with the depth of a single image at the object plane (the coherence length or depth of eld, whichever is smaller), lateral sampling interval on the test surface, and eld of view across the test surface. In summary,

This expression contains the old and new coordinate variables. Therefore, an F , transformation is not appropriate. Let s try an F2. We want