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Fringe projection is related to optical triangulation using a single point of light and light sectioning where a single line is projected onto an object and viewed in a different direction to determine the surface contour (Case et al, 1987) These techniques are usually used with diffuse objects; however, alternative methods have been developed to measure specular surfaces by looking at the fringe re ection (Ritter and Hahn, 1983; Hang et al, 2000) Moire and fringe projection interferometry complement conventional holographic interferometry, especially for testing optics to be used at long wavelengths Although two-wavelength holography (TWH) can be used to contour surfaces at any longerthan-visible wavelength, visible interferometric environmental conditions are required Moire and fringe projection interferometry can contour surfaces at any wavelength longer than 10 100 mm with reduced environmental requirements and no intermediate photographic recording setup.

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Moire is also a useful technique for aiding in the understanding of interferometry This chapter explains what moire is and how it relates to interferometry Con touring techniques utilizing fringe projection, projection and shadow moire, and twoangle holography are all described and compared All of these techniques provide the same result and can be described by a single theory The relationship between these techniques and the holographic and conventional interferometry will be shown Errors caused by divergent geometries are described, and applications of these techniques combined with phase-measurement techniques are presented Further information on these techniques can be found in the following books and book chapters: Varner (1974), Vest (1979), Hariharan (1984), Gasvik (2002), Chiang (1983) Patorski and Kujawinska (1993), Post et al (1997), Amridror (2000), and Walker (2004) 1612 What is Moire Moire patterns are extremely useful to help understand basic interferometry and interferometric test results.

Figure 161 shows the moire pattern (or beat pattern) produced by two identical straight line gratings rotated by a small angle relative to each other A dark fringe is produced where the dark lines are out of step one-half period, and a bright fringe is produced where the dark lines for one grating fall on top of the corresponding dark lines for the second grating If the angle between the two gratings is increased, the separation between the bright and dark.

Fast base station switching (FBSS) and macro diversity handovers (MDHO) require a close synchronization between base stations As the basic IP protocol does not ensure constant latency and bandwidth for a connection, IP QoS mechanisms have to be used over the R8 reference point The reference points/interfaces inside the ASN (R6 and R8) have not been specified in the first version of the WiMAX network infrastructure standard and thus such solutions are proprietary Due to the use of IP on all interfaces, WiMAX network components can be directly connected with each For longer distances, standard IP routers can be used to forward both user data and signaling traffic between the components No special WiMAX software is required in the IP routers This enables operators to use cheaply available IP hardware In addition, operators can lease IP bandwidth from other companies, for example to connect base stations to the ASN-GW.

Unless you re sure you can put things back exactly the way you found them, you might want to label your cables as you remove them. Pay attention to how and where they hook up, so you can replace them correctly. Most drive cable connectors use slots or guides so that connections seat properly only when inserted with the right orientation. But you must pay attention and be gentle when removing or reinserting cable connectors: excess force can damage the connectors on a drive, a controller, or your motherboard. Take our word for it: although it s easy and cheap to replace a cable, you don t want to replace any of those other items (none of them costs less than $25 or $30; some can cost hundreds of dollars).

9. Ronchi Test A. Cornejo-Rodriguez 9.1. 9.2. Introduction 9.1.1. Historical Introduction Geometrical Theory 9.2.1. Ronchi Patterns for Primary Aberrations 9.2.2. Ronchi Patterns for Aspherical Surfaces 9.2.3. Null Ronchi Rulings Wavefront Shape Determination 9.3.1. General Case 9.3.2. Surfaces with Rotational Symmetry Physical Theory 9.4.1. Mathematical Treatment 9.4.2. Fringe Contrast and Sharpness 9.4.3. Physical versus Geometrical Theory Practical Aspects of the Ronchi Test Some Related Tests 9.6.1. Concentric Circular Grid 9.6.2. Phase Shifting Ronchi Test 9.6.3. Sideband Ronchi Test 9.6.4. Lower Test 9.6.5. Ronchi Hartmann and Null Hartmann Tests

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