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Specular lighting depends on the viewer position and adds an exponential drop-off factor, so the object is much brighter when the surface reflects the light straight into the viewer, and it drops off very quickly after that That behavior is described in the following equation: Cs = max(0, s N)shininess Cs Here, Cs is the specular color contribution, N is the surface normal, and Cs is the color of the specular light source What s new here is s, which is an average of the vector from the surface to the viewer position and the vector from the surface to the light Fortunately, OpenGL ES 11 also includes a specular lighting model The theory was that I should be able to turn that on and get all the sparkles I wanted.

(31.82)

Equation (31.82) is plotted in Fig. 31.12 for different values of . All the curves cross at / n = 2. For / n 2, transmissibility, although below unity, increases with

Downloaded from Digital Engineering Library @ McGraw-Hill (www.digitalengineeringlibrary.com) Copyright 2004 The McGraw-Hill Companies. All rights reserved. Any use is subject to the Terms of Use as given at the website.

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Hardware as well as software for each project is presented in an easy-tounderstand format, which will allow anyone with a basic interest in electronics and microprocessors to assemble, as well as program, any of the projects described in this book The CD-ROM accompanying the book also includes three appendixes that are an invaluable aid to the reader and hobbyist alike Appendix 1 contains many full data sheets of the integrated circuits used for projects covered in the book Appendix 2 includes many useful tables and charts for help in understanding and programming the STAMP 2 Appendix 3 presents useful contacts and names, STAMP 2 news/mail groups, and manufacturers The CD-ROM for STAMP 2 Communications and Control Projects also includes all the programs for the projects in this book You can easily load any of the programs in just a few minutes.

Before, when the petals were completely unlit, the vertices didn t need to contain a normal as part of their structure Now, as you can see in the specular reflection equation, I needed that normal to compute the highlights, so I had to extend the vertex format to include them as well..

an increase in damping, contrary to normal expectations. At higher frequencies, transmissibility goes to zero. Since the force amplitude me 2 in the case of an unbalanced machine is dependent upon the operating speed of the machine, transmissibility can be defined as T= FT me

2 1 + (2 n) 2 2 2 (1 / n) + (2

2 n)

The CD-ROM also includes a STAMP 2 manual, application notes, and many additional free programs for other interesting projects One of the reasons the STAMP 2 has been so successful is that it can be interfaced with many different types of sensors and external devices quite readily The BASIC STAMP 2 can often be interfaced with the outside world with oneor two-wire interfaces Many applications such as analog-to-digital conversion or temperature sensing, as well as external memory devices can be interfaced with two wires One-wire devices or I2C devices are very easy to interface to the STAMP 2 The Dallas Semiconductor 1-Wire devices are available as sensors, external memory, and they even have a one-wire weather station that can be used with the STAMP 2.

(31.83)

Finally, all I had left to do was to tweak the lighting parameters (primarily the shininess exponential factor) until I got the desired results. The following code adds a specular color to an OpenGL light:

where FT is the amplitude of the transmitted force. Equation (31.83) is plotted in Fig. 31.24. Transmissibility starts from zero at zero operating frequency, and curves for different damping ratios cross at / n = 2. For higher values of operating speed, transmissibility increases indefinitely with frequency. Passive Isolation. When a sensitive instrument is isolated from a vibrating foundation, it is called passive isolation. Consider the system shown in Fig. 31.15, where the base has a motion u = U0 sin t. The equation of motion of the system is given in Eq. (31.46). The ratio of the response and excitation amplitudes is k+i c X = Xf k m 2 + i c (31.84)

(5.16)

This is best shown by example. Using the planetary train of the previous example, we form Table 5.1, and the equation from the column for gear 5 is n3 N2N4 (n2 n3) = n5 N4N5

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