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Figure 2.22. Re ectivity of a step index ber as a function of the average input power using a Yb:YAG laser with a wavelength of 1030 nm and a pulse duration of 220 ns.

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Designing and implementing the interface of a class The importance of encapsulation Analyzing the quality of an interface Programming by contract: preconditions, postconditions, and invariants

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+ Clearly, the coef cients of the expansion are functions of the bias point. The values of the coef cients are found by intermodulation measurements with low-frequency (in the 100-MHz range) two-tone test voltages: one sinusoidal voltage at the rst test frequency is applied to the gate (or base) of the transistor, and a second sinusoidal signal at a second, very close test frequency is applied to the drain (or collector), as in Figure 3.58. The amplitudes of the test signals are small enough for a Volterra series representation of the intermodulation phenomena to be valid. By selectively shorting some harmonic and intermodulation frequencies at the ports of the device and by expressing the spectral powers for the extraction as functions of the Taylor series expansion, it is possible to use the power of the intermodulation signals coming out of the device at intermodulation frequencies for the selective and successive identi cation of all the coef cients of the Taylor series expansions. This is obtained by inversion of the Volterra series expressions for the intermodulation terms that include the coef cients; the technique is similar to the nonlinear current method (see Section 1.3.1). Since the measurements are absolute values (powers), some care is required for the identi cation of the sign of the coef cients. The instrumentation required for the measurements is very limited: the characterisation frequency (in the 100-MHz range) is high enough to avoid low-frequency dispersion, but

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sensor Nyquist frequency is increased; (3) Use of a longer wavelength (such as 106 mm from a CO2 laser) to rescale the wavefront departure to the longer wavelength; or (4) Testing sub-apertures of the wavefront with a small enough segmentation to suf ciently resolve the individual subapertures None of these approaches is entirely satisfactory as each may involve trade-offs which often place long lead times on the design of the test, requires additional fabrication, increases the dif culty of using and calibrating the instrument, decreases its precision, or greatly increases the instrument cost In order to test aspheric surfaces without resorting to one of these four approaches, a PSI system must be capable of handling fringe densities above the Nyquist frequency, ie, those that are aliased.

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