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You know for certain that you took every precaution in the design of your network. It should be reliable and fast . . . very fast. As a matter of fact, you made sure to put in a top-of-the-line network management station with all the bells and whistles. So what could possibly go wrong The answer to that question is, almost anything. And that is what is so challenging to the network professional. Exactly why is the network having issues Following is a list of possible issues that you might come across when troubleshooting a problem in your LAN:6 Damaged cables Dirty ber Excessive signal attenuation Insuf cient bandwidth
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splitter, while the other beam is just transmitted once. Thus, the intensities of the two interfering beams will be quite different. However, this is partially compensated because the weaker beam is the one with a smaller diameter. Shukla et al. (1992) has also described several other radial shear interferometers based on the same working principle. A very simple holographic radial shear interferometer, shown in Figure 5.21 was devised by Fouere and Malacara (1974) and Fouere (1974). The rst step in making
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Figure 12.2 Fourier series solution to the vibrating string problem. A mesh plot of u(x, t) 1 as given by Eq. (12.37) for the parameters L = 1, c/L = 1 , and H = 10 . The plot employed 8 the rst 100 terms of the series expansion.
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X = 6065.67 Y = 3450.58 Z = 0.00
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some work has been reported on the generation of long pulses. Long-pulse oscillators emitting near-rectangular pulses have been demonstrated by suppressing the relaxation oscillation behavior (temporal spiking) typical of solid-state lasers. This has been accomplished by actively varying the intracavity loss during the laser pulse either with closed-loop feedback on the output power [42] or with a preprogrammed temporal shape [43]. In both cases, pulse widths of up to 600 ns were achieved. However, the sensitivity and temporal bandwidth required for these control schemes are often dif cult to achieve even in a carefully controlled laboratory environment. Long pulses have also been generated with passive control using an intracavity saturable absorber. In this manner, pulse widths of up to 500 ns were demonstrated but with a peaked temporal pro le, large shot-to-shot pulse width variations (100-ns RMS), and a pulse energy of only 0.2 mJ [44]. The pulse energy requirements of a long-range illuminator (.10 J) make a master-oscillator power ampli er (MOPA) the most practical laser architecture. The design goal for the laser ampli er output that is presented here was 30 J/pulse at 1 mm. The large amount of ampli cation required to reach this energy from a lowenergy injected oscillator pulse leads to severe temporal distortion of the input pulse shape due to ampli er gain saturation during ef cient optical extraction. For this reason, the near-rectangular output of previously reported that long-pulse oscillators would not be suitable as an injection source. It has been recognized, however, that the smooth temporal pro le of a relaxation oscillation pulse emitted by a freerunning solid-state laser suffers much less pulse-width distortion when ampli ed [45]. Applying this concept, 1.1 J in a 110-ns pulse was demonstrated from a single ampli er aperture that was then frequency-doubled to 520 mJ at 532 nm [46]. The temporal pro le remained, however, near Gaussian in shape. For this laser system, we adopted a scheme that also relies on the ampli cation of the output of a free-running master oscillator [32]. However, only the leading edge of the pulse is used and it will be shown that the measured width of the injected pulse does not directly determine the width of the ampli ed output pulse. The ampli cation of the leading edge of the input pulse gives rise to a quasi-constant output power, the magnitude of which is dependent on the exponential time constant of this rising edge. A simple analytical theory allows the power, and hence pulse duration, to be tailored to a desired level by adjusting the optical buildup time in the oscillator. 5.4.2 Optical architecture of the 500-ns system
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For many years the only alternative to the method of using the knife-edge test during the manufacture of a paraboloidal mirror was to test the mirror by autocollimation with the aid of an optical at, which had to be as large and as accurately gured as the mirror being manufactured. 12.7.1. Couder, Burch, and Ross Compensators Couder (1927) pointed out that departure from stigmatism of the image of a point source at the center of curvature of a paraboloidal mirror can be removed by interposing a small compensating lens between the image and the mirror. He used a two-element compensator in the arrangement shown in Figure 12.26. Two elements were necessary because he required a null corrector of zero total power to conveniently carry out the manufacturing process desired in his paper. To manufacture a 30-cm f/5 paraboloidal mirror, he used a null corrector whose aperture (scaled from his drawing) was about 4 cm. The use of a spherical mirror beyond the center of curvature of a paraboloid to compensate for the aberrations of a paraboloid used with source and knife edge near its center of curvature was described by Burch (1936). He derived the fth-order aberration of the null systems of this type and showed that with the two-mirror arrangement of Figure 12.27, the residual aberration of the paraboloid is less than one-fortieth of a wave for paraboloids as fast as f=5 and with apertures up to 80 cm,
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