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energy, or EG < hc/l. On this basis it turns out that silicon is useful for wavelengths shorter that 1 m. Germanium is useful at 1.3 m and InSb and InAs at 1.55 m. The total current flowing in a photodiode consists of the actual current generated by the photons, plus what is termed the dark current. This is the current that flows even when no signal is present. Ideally it should be zero, but in practice it is of the order of a few nanoamperes, and it can contribute to the noise. Denoting the dark current by Id the total current is I Iph Id (12.68)

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Find the slope-intercept equation of the tangent line to the graph of the function at the indicated point: 1 x+2 , at x = 1 (a) f (x) = 2 , at x = 2 (b) f (x) = 3 x x 1 Let f (x) = x+2 for all x = 2. Find f ( 2). x 2

Bit position 20 (LSB) 21 22 23

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This current is accompanied by shot noise (a name that is a hangover from vacuum tube days), the mean square spectral density of which is 2qI in A2/Hz with I in amperes. This would be for a diode without any internal amplification such as a PIN diode. An avalanche photo diode (APD) multiplies the signal current by a factor M and at the same time generates excess noise, represented by an excess noise factor, F, so that the mean square spectral density is (2qI)MF. F increases with increase in M (see Jones, 1988, p. 240). Typical values are of the order M 100, F 12. For a PIN diode, M 1 and F 1. The analysis to follow is based on that given in Jones (1988). The equivalent circuit for the input stage of an optical receiver is shown in Fig. 12.14, where R is the parallel combination of diode resistance, input load resistance and preamplifier input resistance, and C is the parallel combination of diode capacitance, preamplifier input capacitance and stray circuit capacitance. Resistance R will generate thermal noise current, the spectral density of which is 4kT/R (k is Boltzmann s constant and T is the temperature, which may be taken as room temperature). The preamplifier transistor will also generate shot noise, which when

The equivalent input circuit for an optical receiver. {it2} is the mean square spectral density for the current noise source, and 2 {va } the mean square spectral density for the voltage noise source. is is the signal current.

3.2.2 AVOIDING COLLISIONS Let s see how you can use this information to control the behavior of the robot. We will start by locating the robot near the center of the screen and making it move upward (north) using the program in Fig. 3.4. Since the robot will be pointed north when it is created, this program will make it move forward until it hits the north wall and causes an error. One way to avoid this error is to monitor the bumpers and stop moving the robot forward when they indicate that an object has been touched. The program in Fig. 3.5 shows how this can be done. If you are unfamiliar with any of the programming statements used here, refer to Sec. C.9. Instead of just telling the robot to move forward 500 times (as in Fig. 3.4), the program of Fig. 3.5 uses a for-next loop to make the robot consider moving forward 500 times. The if-then statement inside the loop checks the bumpers and if none of them are on (the value returned is 0) then the robot moves forward one position. Notice that when using a program to move the robot you will usually move the robot only one position at a time so we can monitor the environment before moving again. Figure 3.6 shows two example programs that perform similar actions to the program in Fig. 3.5, but using different RobotBASIC statements.

13.8 13.9

referred to the input has a spectral density 2q/Iin in A2/Hz, where Iin is the transistor gate (JFET) or base (BJT) current in amperes. Using curly brackets {.} for the spectral density values (see Jones, 1988), the total noise current spectral density at the input is 5i26 5 2qIM 2F 1 t 4kT 1 2qItr A2/Hz R (12.69)

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