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modelscan be divided into dependent Recall from Chap. I that the terms in mathematical variables, pararneters, fbrcing functions.For the bungeejumper and and independent variable, the variable, time (t) is the independent model,the velocity(u) is the dependent (c,,) (g) is the (rr) and dragcoefTicient areparameters, the gravitational and constant rnass the modelsby perto fbrcing function.lt is cornmonplace investigate behaviorof sr.rch This involves how thedependent variable changes ana\-sis. observing fbrmingtr sensitivitlt are as the parameters forcingtunctions varied. and In Example3.7,we developed functionfunction,f uncavg, and usedit to determine a jumper velocity fbr the casewherethe parameters wereset value of the bungee the average thatwe wantedto analyze samefunction,but with the L\t :68. I and c,,- 0.25.Suppose tn parameters. course,we could retypethc functicln with new valuesfbr each Of dif'ferent but it would be preferable tojust change parameters. the case, parameters anonymous into As we learned Sec.3.5.1,it is possible incorporate in to values, could havedonethe we For example, ratherthan "wiring" the nurneric functions. fbllowing:

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As mentioned earlier, each virtual server, regardless of type, on any machine running Exchange needs to have a unique identity. This identity usually consists of an IP address and a TCP port. Let s examine the identity of the default IMAP4 virtual server we worked with in the previous walkthrough. Right-click on the Default IMAP4 Virtual Server node under the IMAP4 container and select Properties. This opens the Default IMAP4 Virtual Server Properties Sheet, where the virtual server s current identity is displayed on the General tab (Figure 23.2).

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8. Suppose that the speed of red visible light in a transparent medium is 270,000 km/s. What, approximately, is the index of refraction for this substance with respect to red light (a) 0.900 (b) 1.11 (c) 0.810 (d) It cannot be calculated from this information. 9. As the magnification of a telescope is increased, (a) the image resolution decreases in direct proportion. (b) physical stability becomes more and more important. (c) the light-gathering area increases in direct proportion. (d) dimmer and dimmer objects can be seen. 10. An advantage of space telescopes over Earthbound telescopes is the fact that (a) space telescopes have less mass. (b) space telescopes do not need power supplies. (c) space telescopes are not subject to temperature changes. (d) space telescopes are not subject to airglow.

In working with FM receivers, there are some terms that need to be defined. First, let s determine the term deviation as the frequency swing of the incoming FM signal. When no modulation is present, the incoming signal is a fixed frequency carrier wave (Fc). Positive deviation (Fp) is the increase in Fc due to modulation, and negative deviation (Fn) is the decrease in Fc due to the modulation. The detector must be linear over the maximum total deviation (Fp max. - Fn max.) produced by the transmitter or distortion will occur. Before the second I-F signal reaches the detector, it is applied to a limiting amplifier inside the integrated circuit. A limiting amplifier is designed to remove any amplitude variations in the signal by amplifying the signal well beyond the limit of the amplifier. The frequency variations (FM) are not affected by the limiter. The limiter removes the affects of fading (driving through a tunnel) and impulse noise (lightning and ignition). These affects produce significant

Toolbox to the editor and use the labels shown in Figures 4-1 to 4-3.

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