Frequency Response of Amplifiers
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RANDOM VIBRATION—AN OVERVIEW by Barry Controls, Hopkinton, MA
RANDOM VIBRATION—AN OVERVIEW by Barry Controls, Hopkinton, MA ABSTRACT Random vibration is becoming increasingly recognized as the most realistic method of simulating the dynamic environment of military applications. Whereas the use of random vibration specifications was previously limited to particular missile applications, its use has been extended to areas in which sinusoidal vibration has historically predominated, including propeller driven aircraft and even moderate shipboard environments. These changes have evolved from the growing awareness that random motion is the rule, rather than the exception, and from advances in electronics which improve our ability to measure and duplicate complex dynamic environments. The purpose of this article is to present some fundamental concepts of random vibration which should be understood when designing a structure or an isolation system. INTRODUCTION Random vibration is somewhat of a misnomer. If the generally accepted meaning of the term "random" were applicable, it would not be possible to analyze a system subjected to "random" vibration. Furthermore, if this term were considered in the context of having no specific pattern (i.e., haphazard), it would not be possible to define a vibration environment, for the environment would vary in a totally unpredictable manner. Fortunately, this is not the case. The majority of random processes fall in a special category termed stationary. This means that the parameters by which random vibration is characterized do not change significantly when analyzed statistically over a given period of time - the RMS amplitude is constant with time. For instance, the vibration generated by a particular event, say, a missile launch, will be statistically similar whether the event is measured today or six months from today. -
PH-218 Lec-12: Frequency Response of BJT Amplifiers
Analog & Digital Electronics Course No: PH-218 Lec-12: Frequency Response of BJT Amplifiers Course Instructors: Dr. A. P. VAJPEYI Department of Physics, Indian Institute of Technology Guwahati, India 1 High frequency Response of CE Amplifier At high frequencies, internal transistor junction capacitances do come into play, reducing an amplifier's gain and introducing phase shift as the signal frequency increases. In BJT, C be is the B-E junction capacitance, and C bc is the B-C junction capacitance. (output to input capacitance) At lower frequencies, the internal capacitances have a very high reactance because of their low capacitance value (usually only a few pf) and the low frequency value. Therefore, they look like opens and have no effect on the transistor's performance. As the frequency goes up, the internal capacitive reactance's go down, and at some point they begin to have a significant effect on the transistor's gain. High frequency Response of CE Amplifier When the reactance of C be becomes small enough, a significant amount of the signal voltage is lost due to a voltage-divider effect of the source resistance and the reactance of C be . When the reactance of Cbc becomes small enough, a significant amount of output signal voltage is fed back out of phase with the input (negative feedback), thus effectively reducing the voltage gain. 3 Millers Theorem The Miller effect occurs only in inverting amplifiers –it is the inverting gain that magnifies the feedback capacitance. vin − (−Av in ) iin = = vin 1( + A)× 2π × f ×CF X C Here C F represents C bc vin 1 1 Zin = = = iin 1( + A)× 2π × f ×CF 2π × f ×Cin 1( ) Cin = + A ×CF 4 High frequency Response of CE Amp.: Millers Theorem Miller's theorem is used to simplify the analysis of inverting amplifiers at high-frequencies where the internal transistor capacitances are important. -
Cascode Amplifiers by Dennis L. Feucht Two-Transistor Combinations
Cascode Amplifiers by Dennis L. Feucht Two-transistor combinations, such as the Darlington configuration, provide advantages over single-transistor amplifier stages. Another two-transistor combination in the analog designer's circuit library combines a common-emitter (CE) input configuration with a common-base (CB) output. This article presents the design equations for the basic cascode amplifier and then offers other useful variations. (FETs instead of BJTs can also be used to form cascode amplifiers.) Together, the two transistors overcome some of the performance limitations of either the CE or CB configurations. Basic Cascode Stage The basic cascode amplifier consists of an input common-emitter (CE) configuration driving an output common-base (CB), as shown above. The voltage gain is, by the transresistance method, the ratio of the resistance across which the output voltage is developed by the common input-output loop current over the resistance across which the input voltage generates that current, modified by the α current losses in the transistors: v R A = out = −α ⋅α ⋅ L v 1 2 β + + + vin RB /( 1 1) re1 RE where re1 is Q1 dynamic emitter resistance. This gain is identical for a CE amplifier except for the additional α2 loss of Q2. The advantage of the cascode is that when the output resistance, ro, of Q2 is included, the CB incremental output resistance is higher than for the CE. For a bipolar junction transistor (BJT), this may be insignificant at low frequencies. The CB isolates the collector-base capacitance, Cbc (or Cµ of the hybrid-π BJT model), from the input by returning it to a dynamic ground at VB. -
Amplifier Frequency Response
EE105 – Fall 2015 Microelectronic Devices and Circuits Prof. Ming C. Wu [email protected] 511 Sutardja Dai Hall (SDH) 2-1 Amplifier Gain vO Voltage Gain: Av = vI iO Current Gain: Ai = iI load power vOiO Power Gain: Ap = = input power vIiI Note: Ap = Av Ai Note: Av and Ai can be positive, negative, or even complex numbers. Nagative gain means the output is 180° out of phase with input. However, power gain should always be a positive number. Gain is usually expressed in Decibel (dB): 2 Av (dB) =10log Av = 20log Av 2 Ai (dB) =10log Ai = 20log Ai Ap (dB) =10log Ap 2-2 1 Amplifier Power Supply and Dissipation • Circuit needs dc power supplies (e.g., battery) to function. • Typical power supplies are designated VCC (more positive voltage supply) and -VEE (more negative supply). • Total dc power dissipation of the amplifier Pdc = VCC ICC +VEE IEE • Power balance equation Pdc + PI = PL + Pdissipated PI : power drawn from signal source PL : power delivered to the load (useful power) Pdissipated : power dissipated in the amplifier circuit (not counting load) P • Amplifier power efficiency η = L Pdc Power efficiency is important for "power amplifiers" such as output amplifiers for speakers or wireless transmitters. 2-3 Amplifier Saturation • Amplifier transfer characteristics is linear only over a limited range of input and output voltages • Beyond linear range, the output voltage (or current) waveforms saturates, resulting in distortions – Lose fidelity in stereo – Cause interference in wireless system 2-4 2 Symbol Convention iC (t) = IC +ic (t) iC (t) : total instantaneous current IC : dc current ic (t) : small signal current Usually ic (t) = Ic sinωt Please note case of the symbol: lowercase-uppercase: total current lowercase-lowercase: small signal ac component uppercase-uppercase: dc component uppercase-lowercase: amplitude of ac component Similarly for voltage expressions. -
I. Common Base / Common Gate Amplifiers
I. Common Base / Common Gate Amplifiers - Current Buffer A. Introduction • A current buffer takes the input current which may have a relatively small Norton resistance and replicates it at the output port, which has a high output resistance • Input signal is applied to the emitter, output is taken from the collector • Current gain is about unity • Input resistance is low • Output resistance is high. V+ V+ i SUP ISUP iOUT IOUT RL R is S IBIAS IBIAS V− V− (a) (b) B. Biasing = /α ≈ • IBIAS ISUP ISUP EECS 6.012 Spring 1998 Lecture 19 II. Small Signal Two Port Parameters A. Common Base Current Gain Ai • Small-signal circuit; apply test current and measure the short circuit output current ib iout + = β v r gmv oib r − o ve roc it • Analysis -- see Chapter 8, pp. 507-509. • Result: –β ---------------o ≅ Ai = β – 1 1 + o • Intuition: iout = ic = (- ie- ib ) = -it - ib and ib is small EECS 6.012 Spring 1998 Lecture 19 B. Common Base Input Resistance Ri • Apply test current, with load resistor RL present at the output + v r gmv r − o roc RL + vt i − t • See pages 509-510 and note that the transconductance generator dominates which yields 1 Ri = ------ gm µ • A typical transconductance is around 4 mS, with IC = 100 A • Typical input resistance is 250 Ω -- very small, as desired for a current amplifier • Ri can be designed arbitrarily small, at the price of current (power dissipation) EECS 6.012 Spring 1998 Lecture 19 C. Common-Base Output Resistance Ro • Apply test current with source resistance of input current source in place • Note roc as is in parallel with rest of circuit g v m ro + vt it r − oc − v r RS + • Analysis is on pp. -
Dynamic Microphone Amplifier
Dynamic Microphone Preamp Description: A low noise pre-amplifier suitable for amplifying dynamic microphones with 200 to 600 ohm output impedance. Notes: This is a 3 stage discrete amplifier with gain control. Alternative transistors such as BC109C, BC548, BC549, BC549C may be used with little change in performance. The first stage built around Q1 operates in common base configuration. This is unusuable in audio stages, but in this case, it allows Q1 to operate at low noise levels and improves overall signal to noise ratio. Q2 and Q3 form a direct coupled amplifier, similar to my earlier mic preamp . Input and Output Impedance: As the signal from a dynamic microphone is low typically much less than 10mV, then there is little to be gained by setting the collector voltage voltage of Q1 to half the supply voltage. In power amplifiers, biasing to half the supply voltage allows for maximum voltage swing, and highest overload margin, but where input levels are low, any value in the linear part of the operating characteristics will suffice. Here Q1 operates with a collector voltage of 2.4V and a low collector current of around 200uA. This low collector current ensures low noise performance and also raises the input impedance of the stage to around 400 ohms. This is a good match for any dynamic microphone having an impedances between 200 and 600 ohms. The output impedance at Q3 is low, the graph of input and output impedance versus frequency is shown below: Gain and Frequency Response: The overall gain of this pre-amplifier is around +39dB or about 90 times. -
Lecture23-Amplifier Frequency Response.Pptx
EE105 – Fall 2014 Microelectronic Devices and Circuits Prof. Ming C. Wu [email protected] 511 Sutardja Dai Hall (SDH) Lecture23-Amplifier Frequency Response 1 Common-Emitter Amplifier – ωH Open-Circuit Time Constant (OCTC) Method At high frequencies, impedances of coupling and bypass capacitors are small enough to be considered short circuits. Open-circuit time constants associated with impedances of device capacitances are considered instead. 1 ωH ≅ m ∑RioCi i=1 where Rio is resistance at terminals of ith capacitor C with all other v ! R $ i R = x = r #1+ g R + L & capacitors open-circuited. µ 0 π 0 m L ix " rπ 0 % For a C-E amplifier, assuming C = 0 L 1 1 ωH ≅ = Rπ 0 = rπ 0 Rπ 0Cπ + Rµ 0Cµ rπ 0CT Lecture23-Amplifier Frequency Response 2 1 Common-Emitter Amplifier High Frequency Response - Miller Effect • First, find the simplified small -signal model of the C-E amp. • Replace coupling and bypass capacitors with short circuits • Insert the high frequency small -signal model for the transistor ! # rπ 0 = rπ "rx +(RB RI )$ Lecture23-Amplifier Frequency Response 3 Common-Emitter Amplifier – ωH High Frequency Response - Miller Effect (cont.) v R r Input gain is found as A = b = in ⋅ π i v R R r r i I + in x + π R || R || (r + r ) r = 1 2 x π ⋅ π RI + R1 || R2 || (rx + rπ ) rx + rπ Terminal gain is vc Abc = = −gm (ro || RC || R3 ) ≅ −gm RL vb Using the Miller effect, we find CeqB = Cµ (1− Abc )+Cπ (1− Abe ) the equivalent capacitance at the base as: = Cµ (1−[−gm RL ])+Cπ (1− 0) = Cµ (1+ gm RL )+Cπ Chap 17-4 Lecture23-Amplifier Frequency Response 4 2 Common-Emitter Amplifier – ωH High Frequency Response - Miller Effect (cont.) ! # • The total equivalent resistance ReqB = rπ 0 = rπ "rx +(RB RI )$ at the base is • The total capacitance and CeqC = Cµ +CL resistance at the collector are ReqC = ro RC R3 = RL • Because of interaction through 1 ω = Cµ, the two RC time constants p1 ! # rπ 0 "Cπ +Cµ (1+ gm RL )$+ RL (Cµ +CL ) interact, giving rise to a dominant pole. -
Frequency Response and Bode Plots
1 Frequency Response and Bode Plots 1.1 Preliminaries The steady-state sinusoidal frequency-response of a circuit is described by the phasor transfer function Hj( ) . A Bode plot is a graph of the magnitude (in dB) or phase of the transfer function versus frequency. Of course we can easily program the transfer function into a computer to make such plots, and for very complicated transfer functions this may be our only recourse. But in many cases the key features of the plot can be quickly sketched by hand using some simple rules that identify the impact of the poles and zeroes in shaping the frequency response. The advantage of this approach is the insight it provides on how the circuit elements influence the frequency response. This is especially important in the design of frequency-selective circuits. We will first consider how to generate Bode plots for simple poles, and then discuss how to handle the general second-order response. Before doing this, however, it may be helpful to review some properties of transfer functions, the decibel scale, and properties of the log function. Poles, Zeroes, and Stability The s-domain transfer function is always a rational polynomial function of the form Ns() smm as12 a s m asa Hs() K K mm12 10 (1.1) nn12 n Ds() s bsnn12 b s bsb 10 As we have seen already, the polynomials in the numerator and denominator are factored to find the poles and zeroes; these are the values of s that make the numerator or denominator zero. If we write the zeroes as zz123,, zetc., and similarly write the poles as pp123,, p , then Hs( ) can be written in factored form as ()()()s zsz sz Hs() K 12 m (1.2) ()()()s psp12 sp n 1 © Bob York 2009 2 Frequency Response and Bode Plots The pole and zero locations can be real or complex. -
Evaluation of Audio Test Methods and Measurements for End-Of-Line Loudspeaker Quality Control
Evaluation of audio test methods and measurements for end-of-line loudspeaker quality control Steve Temme1 and Viktor Dobos2 (1. Listen, Inc., Boston, MA, 02118, USA. [email protected]; 2. Harman/Becker Automotive Systems Kft., H-8000 Székesfehérvár, Hungary) ABSTRACT In order to minimize costly warranty repairs, loudspeaker OEMS impose tight specifications and a “total quality” requirement on their part suppliers. At the same time, they also require low prices. This makes it important for driver manufacturers and contract manufacturers to work with their OEM customers to define reasonable specifications and tolerances. They must understand both how the loudspeaker OEMS are testing as part of their incoming QC and also how to implement their own end-of-line measurements to ensure correlation between the two. Specifying and testing loudspeakers can be tricky since loudspeakers are inherently nonlinear, time-variant and effected by their working conditions & environment. This paper examines the loudspeaker characteristics that can be measured, and discusses common pitfalls and how to avoid them on a loudspeaker production line. Several different audio test methods and measurements for end-of- the-line speaker quality control are evaluated, and the most relevant ones identified. Speed, statistics, and full traceability are also discussed. Keywords: end of line loudspeaker testing, frequency response, distortion, Rub & Buzz, limits INTRODUCTION In order to guarantee quality while keeping testing fast and accurate, it is important for audio manufacturers to perform only those tests which will easily identify out-of-specification products, and omit those which do not provide additional information that directly pertains to the quality of the product or its likelihood of failure. -
Lecture 19 Common-Gate Stage
4/7/2008 Lecture 19 OUTLINE • Common‐gate stage • Source follower • Reading: Chap. 7.3‐7.4 EE105 Spring 2008 Lecture 19, Slide 1Prof. Wu, UC Berkeley Common‐Gate Stage AvmD= gR • Common‐gate stage is similar to common‐base stage: a rise in input causes a rise in output. So the gain is positive. EE105 Spring 2008 Lecture 19, Slide 2Prof. Wu, UC Berkeley EE105 Fall 2007 1 4/7/2008 Signal Levels in CG Stage • In order to maintain M1 in saturation, the signal swing at Vout cannot fall below Vb‐VTH EE105 Spring 2008 Lecture 19, Slide 3Prof. Wu, UC Berkeley I/O Impedances of CG Stage 1 R = in λ =0 RRout= D gm • The input and output impedances of CG stage are similar to those of CB stage. EE105 Spring 2008 Lecture 19, Slide 4Prof. Wu, UC Berkeley EE105 Fall 2007 2 4/7/2008 CG Stage with Source Resistance 1 g vv= m Xin1 + RS gm 1 vv g AgR==out x m vmD1 vvxin + RS gm R gR ==D mD 1 1+ gRmS + RS gm • When a source resistance is present, the voltage gain is equal to that of a CS stage with degeneration, only positive. EE105 Spring 2008 Lecture 19, Slide 5Prof. Wu, UC Berkeley Generalized CG Behavior Rgout= (1++g mrR O) S r O • When a gate resistance is present it does not affect the gain and I/O impedances since there is no potential drop across it (at low frequencies). • The output impedance of a CG stage with source resistance is identical to that of CS stage with degeneration. -
Calibration of Radio Receivers to Measure Broadband Interference
NBSIR 73-335 CALIBRATION OF RADIO RECEIVERS TO MEASORE BROADBAND INTERFERENCE Ezra B. Larsen Electromagnetics Division Institute for Basic Standards National Bureau of Standards Boulder, Colorado 80302 September 1973 Final Report, Phase I Prepared for Calibration Coordination Group Army /Navy /Air Force NBSIR 73-335 CALIBRATION OF RADIO RECEIVERS TO MEASORE BROADBAND INTERFERENCE Ezra B. Larsen Electromagnetics Division Institute for Basic Standards National Bureau of Standards Boulder, Colorado 80302 September 1973 Final Report, Phase I Prepared for Calibration Coordination Group Army/Navy /Air Force u s. DEPARTMENT OF COMMERCE, Frederick B. Dent. Secretary NATIONAL BUREAU OF STANDARDS. Richard W Roberts Director V CONTENTS Page 1. BACKGROUND 2 2. INTRODUCTION 3 3. DEFINITIONS OF RECEIVER BANDWIDTH AND IMPULSE STRENGTH (Or Spectral Intensity) 5 3.1 Random noise bandwidth 5 3.2 Impulse bandwidth in terms of receiver response transient 7 3.3 Voltage-response bandwidth of receiver 8 3.4 Receiver bandwidths related to voltage- response bandwidth 9 3.5 Impulse strength in terms of random-noise bandwidth 10 3.6 Sum-and-dif ference correlation radiometer technique 10 3.7 Impulse strength in terms of Fourier trans- forms 11 3.8 Impulse strength in terms of rectangular DC pulses 12 3.9 Impulse strength and impulse bandwidth in terms of RF pulses 13 4. EXPERIMENTAL PROCEDURE AND DATA 16 4.1 Measurement of receiver input impedance and phase linearity 16 4.2 Calibration of receiver as a tuned RF volt- meter 20 4.3 Stepped- frequency measurements of receiver bandwidth 23 4.4 Calibration of receiver impulse bandwidth with a baseband pulse generator 37 iii CONTENTS [Continued) Page 4.5 Calibration o£ receiver impulse bandwidth with a pulsed-RF source 38 5. -
High-Frequency Amplifier Response
Section H5: High-Frequency Amplifier Response Now that we’ve got a high frequency models for the BJT, we can analyze the high frequency response of our basic amplifier configurations. Note: in the circuits that follow, the actual signal source (vS) and its associated source resistance (RS) have been included. As discussed in the low frequency response section of our studies, we always knew that this source and resistance was there but we just started our investigations with the input to the transistor (vin). Remember - the analysis process is the same and the relationship between vS and vin is a voltage divider! Again, in some instances in the following discussion, I will be using slightly different notation and taking a different approach than your author. As usual, if this results in confusion, or you are more comfortable with his technique, let me know and we’ll work it out. High Frequency Response of the CE and ER Amplifier The generic common-emitter amplifier circuit of Section D2 is reproduced to the left below and the small signal circuit using the high frequency BJT model is given below right (based on Figures 10.17a and 10.17b of your text). Note that all external capacitors are assumed to be short circuits at high frequencies and are not present in the high frequency equivalent circuit (since the external capacitors are large when compared to the internal capacitances – recall that Zc=1/jωC gets small as the frequency or capacitance gets large). We can simplify the small signal circuit by making the following observations and approximations: ¾ Cce is very small and may be neglected.