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Fundamental Noise Basics and Calculations

                                                        Fundamental Noise Basics and Calculations  57

                       TABLE 3.5 Comparison of Different Load Resistors for Sensitive Detection
                       Voltage follower: gain = 100¥
                       Photocurrent = 100pA                   R L = 1MW                R L = 1GW

                                                             126nV/ Hz                 4mV/ Hz
                       Thermal noise density of R L
                       Output voltage noise in 20MHz BW      56mV rms                  1.8V rms
                       Output voltage noise in 100Hz BW      0.126mV rms               4mV rms
                       Output signal voltage                 10mV rms                  10mV rms
                       S/N in 100Hz BW                       79                        2500
                       TABLE 3.6 Comparison of Different Amplifier Types
                       Voltage follower: gain = 1¥
                       Photocurrent = 100 pA               Typical bipolar       Typical FET opamp
                       R L = 1GW, 100Hz detection BW      opamp (e.g., OP07)      (e.g., LMC7101)
                       Input bias current (i b)             10nA                   64pA
                       Input offset voltage (V os)          0.25mV                 10mV
                       Input noise voltage density (e n )   12nV/ Hz               37nV/ Hz
                       Input noise current density (i n )   0.2pA/ Hz              1.5fA/ Hz
                       Signal output                        0.1V                   0.1V
                                                            0.25mV                 10mV
                       Static offset voltage due to V os
                                                            10V                    64mV
                       Offset voltage due to i b
                       Amplifier voltage noise in BW         120nV rms              370nV rms
                       Amplifier current noise in BW         2mV rms                15mV rms
                       Load resistor thermal noise in BW    40mV rms               40mV rms
                       S/N in BW                            50                     2300
                         The next thing we can do is to realize that the TV remote control needs a sig-
                       naling bandwidth only of the order of a few tens of hertz. Hence let’s addi-
                       tionally restrict the bandwidth by adding a low-pass filter with an upper cutoff
                       frequency of 100Hz. The 1GW load thermal noise voltage drops further to 4mV
                       rms. Suddenly we have a S/N ª 2500, and the system is starting to look useful.
                       Table 3.5 summarizes the calculations.
                         Having analyzed the S/N for a noiseless amplifier, we can go on to add the
                       opamp voltage and current noise generators to our 1GW design. This is shown
                       in Table 3.6.
                         It is clear that in this application the use of the FET opamp is preferable due
                       to its low bias current. The bipolar opamp’s high bias current leads to a large
                       static offset voltage. The FET opamp greatly reduces this effect, as well as the
                       related noise contribution from its current noise generator. Nevertheless it would
                       be useful to reduce the 64-mV output offset voltage due to bias current, for
                       example by using an amplifier with even smaller bias current.


           3.10 TRY IT! Another Attempt at Visible Shot
           Noise Measurements
                         Let’s look again at noise onscreen. This time we’ll increase the load resistor and add
                         some gain to make it more detectable with an oscilloscope. Connect a small-area


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