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run. Whilst this approach provides a general insight to the performance of a particular location technique, the location of the xed nodes can have a substantial impact on the location performance. Therefore, the performance of one selected xed node con guration is also examined. This is the con guration from the 1000 random xed node con gurations which produces the best results in terms of RMSE. The TOA estimation errors are produced using the synchronization technique described earlier. Throughout the rest of the chapter, the results corresponding to the time instants of the integrators as shown in Figure 17.11 are employed. Figures 17.15 and 17.16 show the accuracy and failure rate of the direct method and the spherical interpolation algorithm [7]. The TOA-based approach (results denoted DM3 ) is seen to be sensitive to the accuracy of transmit time. DM3(inacc t0) presents results with a transmit time error of 4 ns. When the transmit time error is in the order of tens of nanoseconds, the TOA-based method performs very poorly. Only when nearly error-free transmit time information is available (compared with the time reference at xed nodes) is the approach described by Equations (17.10) (17.12) suitable. Also shown are results for the spherical-interpolation method with ve, six and eight xed nodes (denoted SI5, SI6, and SI8 ). The technique does not work well in the case of four xed nodes, as indicated in [7], so the corresponding results are not presented. At relatively high SNR, the spherical-interpolation method performs well when at least ve xed nodes are employed.

You can add a revision to the table by right-clicking the table and selecting Revisions Add Revision. This includes control over whether the revision uses numerical or alphabetical revision levels, but does not provide for more complex revisioning schemes. Immediately after you have created the revision, if the option is enabled, you are prompted to place a balloon that contains the revision level to identify what has been changed. To finish placing symbols, you can press Esc. When you are finished placing the balloons, you can fill in the description of the revision by double-clicking in the Description cell where you want to add text. Figure 24.16 shows a Revision Table with balloon symbols placed on the drawing. Revision Tables work by creating a Revision custom property in the drawing document, and by incrementing this revision each time a revision is added to the table. Additional columns linked to custom properties can be added to Revision Tables and Revision Table templates.

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so a tunable laser is needed and in some cases rapid frequency changes are necessary [6]. Since some arrangements require more than six laser beams at different frequencies, diode lasers represent cost- and space-effective sources for cooling experiments. After twenty years development, laser cooling is now able to reduce the temperatures of atomic ensembles down to below the K range. By cooling in three dimensions, atoms can be confined by light to a particular region in space for large periods of time [124] producing trapped atoms [125] or regions of optical molasses [126]. This has led to the observation of some startling low temperature phenomena such as Bose-Einstein condensation in a cloud of rubidium atoms [96, 127]. Cooling has also been successfully applied in high accuracy caesium and rubidium clocks to reduce the motion of the atoms and lower the frequency uncertainty by a factor of 5 or more. Now some clocks can realize the second to an uncertainty that is less than 2 10 15 seconds [128]. Laser cooling is also used to reduce the transverse velocity distribution of a beam of atoms. Manipulating atom velocities in this way can be used to collimate atomic beams, making them somewhat similar to beams of laser light, leading to the prospect of atom lasers [127].

With high- eld NMR spectrometers that spread the proton chemical shift range over thousands of Hertz, these plots do lose some detail, but this information can be captured in subsequent blowup plots (small portions of the spectrum printed at a larger size) of speci c regions of interest When examining NMR spectra of crude reaction mixtures, extraneous peaks may frequently appear owing to solvents remaining from the reaction or the puri cation, or from contaminants.

(2.24), that is, U U F, or alternatively, V V F, where F is a diagonal matrix with zl s along the main diagonal. However, the Vandermonde structure of U and V allows for a more general version of Equation (2.24), speci cally, U U d Fd

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