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There s nothing to stop you creating a loop inside another loop. In fact, this can be quite a useful technique. When you nest one loop inside another, the inner loop runs through all its iterations first. Then the outer loop iterates, causing the inner loop to run through all its iterations again, and so on. Here s a simple example of nested looping:

and the minimum measurable height difference is determined by the total tuning range as 15:32 hmin p= kmax kmin However, other factors in uence these values; for example, the depth of eld of the objective may limit the maximum measurable depth of the object (see Section 1541) 1573 Signal Analysis As explained in the previous section, information about the relative distance between the object and reference plane can be retrieved by nding the fringe frequency or phase change rate at a given point At rst, the fringe frequency was determined by counting the number of zero-crossings of the signal at each pixel Later, a method based on the Fourier transform calculation was developed (Takeda and Yamamoto, 1994; Barnes et al, 1996; Yamaguchi et al, 1998) Figure 1542 shows three interferograms for three different objects at one wavelength during a wavelength scan.

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In Proceedings of International Parallel and Distributed Processing Symposium, 2004 24 M Smith and T Williams Phylospaces: reconstructing evolutionary trees in tuple spaces In Proceedings of International Parallel and Distributed Processing Symposium, 2006..

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Also shown is the signal as recorded by a pixel during a wavelength scan and the Fourier transform of the signal with the peak position determining the height of the object To further improve the resolution of the Fourier transform technique, the rate of phase change (spectral phase slope) along the spectral interference can be calculated (Kinoshita et al, 1999; Mehta et al, 2003a; Mehta et al, 2003b) Wavelength scanning interferometry requires tens or hundreds of registered interferograms during the wavelength scanning of the source The measurement time in wavelength scanning interferometry is the same for shallow and deep surfaces because the number of required frames does not depend on sample s depth like in white light interferometry In the Michelson interferometer object height can be, in relative terms, on both sides of the reference mirror.

After opening the editor you are ready to add, delete, or modify the flow definition using the tools provided by the toolbar or by using the property dialogs. Opening a file in the Graphical Web Flow Editor does not prevent your opening the same file in another Eclipse Editor. You can use the Open with context menu item to open a Web Flow Config in the XML editor and start to work with the graphical and source editors.

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Because the methods described here solve only for the magnitude of the object s distance from the reference, not its direction, a height ambiguity problem exists Figure 1543 shows the height ambiguity that can be created In these cases, a special phase unwrapping procedure must be applied (Paulson et al, 2000), or a phase unwrapping procedure known as temporal phase unwrapping (Huntley and Saldner, 1993, 1997; Saldner and Huntley, 1997a, 1997b, Huntley and Coggrave, 1998) must be applied to wavelength scanning interferometry If the object were shifted above or below the focus plane, no unwrapping procedure would be necessary because the object would be clearly on one side of focus or the other Shifting the object away from focus increases the frequency of fringes at each point as shown in Figure 1544.

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