7 The op-amp and negative feedback

7.1 Introduction

This chapter introduces the operational amplifier, or op-amp, as an abstract electronic component. The internals of opamps will be detailed in chapter 8; This type of amplifier has two characteristics that we already used in feedback systems: it has a subtraction point and a high voltage gain. The term operational amplifier stems from the era where signal conditioning and operations on signals were done only in the analog domain: the 1940’s to 1960’s. Using op-amps many mathematical operations could be implemented wrapping proper feedback circuitry around them. Using op-amps, multipliers, adders, differentiators and more can easily be implemented. Drawbacks of op-amp based signal operations include noise, and spread issues (not addressed in this book), frequency dependencies and impedance related issues. Nowadays signal processing is preferably done in the digital domain, which is more power efficient at low frequencies, does not have impedance or spread related limitations and is quite easy to generate.

Nowadays, op-amp-like configurations — a gain stage with feedback wrapped around it in some way — are still widely used in electronics at all places where digital signal processing cannot be used: in signal conditioning, basic amplifiers, analog-digital conversion, in RF circuitry, in A-D conversions and D-A conversions and more. In this chapter mainly simple applications of op-amps are discussed, along with the major non-idealities and their impact.

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Figure 7.1: The op-amp: a) abstract model b) symbol

The symbol of an op-amp is shown in Figure 7.1: it is essentially a voltage amplifier with a differential input voltage that generates an output voltage vOUT = A (v+ v). For an ideal op-amp, the voltage gain A , the input impedance rin Ω and the output impedance rout = 0Ω. The circuitry inside the op-amp is not dealt with in this chapter: it consists of a number of basic building blocks — similar to the ones in chapter 5 with some additional ones, see chapter 8 — that all together make the op-amp.

7.2 Linear applications

Op-amp based circuits are frequently used for analog signal processing applications. These mainly include linear processing such as current-to-voltage conversion, voltage gain, filtering, integration and more. In the following subsections a number of these applications are discussed in some detail. Extending it to other signal processing functions is quite straight-forward.

7.2.1 Non-inverting voltage amplifier

One of the basic configurations of an op-amp is given in Figure 7.2. Negative feedback is wrapped around the op-amp, while the total circuit is driven at the +-input. For clarity, the non-ideal input and output resistance and the voltage controlled voltage source that models the operation of the op-amp are shown in grey. Below, a number of properties for this circuit configuration are derived.

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Figure 7.2: Non-inverting amplifier

The voltage gain of the circuit above can be easily calculated using some simplifications (idealisations): rin Ω and rout 0Ω. An example of the derivation of the voltage gain is:

vOUT = A(v+ v) v+ = vG v = R2 R1 + R2 vOUT vOUT = A (vG R2 R1 + R2 vOUT ) vOUT = A vG 1 + R2 R1+R2 A

The relation for the voltage gain immediately follows:

vOUT vG = A 1 + R2 R1+R2 A vOUT vG | A = R1 + R2 R2 (7.1)

The input resistance of the circuit can easily be determined. Firstly this input resistance is derived explicitly assuming a finite value for rin,opamp. The hardest part of this is — with the brute force approach — to neatly find all the simple relations iteratively and to keep track of what’s already been described:

rin = vg ig ig = vg v rin,opamp v = R2rin,opamp R1 + R2rin,opamp vout + R2R1 R1R2 + rin,opamp vg vout = A (vg v) v = vg A R2rin,opamp R1+R2rin,opamp + R2R1 R1R2+rin,opamp 1 + A R2rin,opamp R1+R2rin,opamp

Substituting all these relations gives the desired result. Note that the relation for rin below is rewritten a few times. This does not change the relation: they are identical and hence they all are just as correct as the other. The main purpose however is to get a readable relation:

ig = vg rin,opamp ( 1 1 + A R2rin,opamp R1+R2rin,opamp R2R1 R1R2+rin,opamp 1 + A R2rin,opamp R1+R2rin,opamp ) rin = rin,opamp (1 + A R2rin,opamp R1+R2rin,opamp 1 R2R1 R1R2+rin,opamp ) = rin,opamp (1 + A R2rin,opamp R1+R2rin,opamp rin,opamp R1R2+rin,opamp ) = (R1R2 + rin,opamp) (1 + A R2rin,opamp R1 + R2rin,opamp )

It looks like a lot of work, and it is. However, if we assume rin,opamp to be much larger than R1 and R2, then the derivation becomes much more simple:

rin = vg ig ig = vg v rin,opamp v R2 R1 + R2 vout vout = A (vg v) vA R2 R1+R2 vg 1 + R2 R1+R2 A rin rin,opamp (1 + R2 R1 + R2 A)

This relation clearly shows that the input impedance of the non-inverting amplifier configuration is quite high for large values of A. The limit, for A the input impedance of this system is Ω for any positive rin,opamp: even for e.g. rin,opamp = 1μΩ with A you will get an infinite system-input resistance.

The output resistance of the circuit is calculated in pretty much the same way as described above. Assuming that the output port of the system is driven by a voltage source — with vg = 0 — and assuming an infinite input resistance but with a nonzero rout,opamp0Ω:

rout = vout iout iout = vout R1 + R2 + vout A (v+ v) rout,opamp v+ = vg = 0 v = βvout iout = vout ( 1 R1 + R2 + 1 + A β rout,opamp ) rout = (R1 + R2)rout,opamp 1 + A β

In words: the output resistance of the system is the resistance of the β network at the output, in parallel to the output resistance of the op-amp, decreased by a factor (1 + ). Usually this last term is dominant — the most low-ohmic — mainly due to the large .

7.2.2 Inverting voltage amplifier

A different basic circuit, if not the basic circuit, for an op-amp is shown in Figure 7.3. Topology wise, the main difference with respect to the non-inverting circuit of Figure 7.2 is that the circuit in Figure 7.3 has both the input signal and the feedback signal at the inverting input of the op-amp. This has a major impact on many properties.

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Figure 7.3: Inverting amplifier configuration

The voltage gain of the configuration of Figure 7.3 can be easily obtained if we assume rin ∞Omega and rout = 0Omega:

H = vout vg vout = A (v+ v) v+ = 0 v = vg R1 R1 + R2 + vout R2 R1 + R2 vout = A vg R1 R1+R2 1 + A R2 R1+R2

For the signal transfer:

H = A R1 R1 + (A + 1) R2 H|A = R1 R2 (7.2)

The circuit of Figure 7.3 is called an inverting op-amp configuration, since it has a negative voltage gain. Other characteristics of the circuit are covered below; again it is assumed for simplicity that rin Ω and rout 0Ω.

The input resistance of this circuit can be calculated in various ways; one of those methods is driving the input by vg and deriving the input current ig, after which rin = viniin:

rin = vg ig ig = vg v R2 v = vout A vout = A vg R1 R1+R2 1 + A R2 R1+R2 v = vg R1 R1+R2 1 + A R2 R1+R2 ig = vg R2 1 + R2 R1+R2 A R1 R1+R2 1 + R2 R1+R2 A rin = R2 ( 1 + R2 R1+R2 A 1 + R2 R1+R2 A R1 R1+R2 )

This last expression for rin is correct, but also quite ugly. There are (infinitely) many ways of writing this equation, where some representations are more “readable” than others. A few examples are given below:

rin = R2 (1 + R2 R1+R2 A + R1 R1+R2 R1 R1+R2 1 + R2 R1+R2 A R1 R1+R2) ) = R2 (1 + R1 R1+R2 1 + R2 R1+R2 A R1 R1+R2 ) = R2 (1 + R1 R1 + R2 + R2 A R1 ) = R2 + R1 1 + A

The latter form is very readable, and shows that for a large A, the input resistance almost equals R2. If we let A , then the equation simplifies to:

rin = R2

First obtaining the complete answer and subsequently substituting A gives the correct answer, but it is much easier to assume A a priori. In that case (for a finite output voltage), the differential input voltage will be something finite = 0 V. This simplifies the derivation to:

rin = vg ig ig = vg v R2 v = v+ = 0 ig = vg R2 rin = R2

A different but simple derivation can be performed by acknowledging that the input resistance of the circuit is equal to the sum of R2, and the input resistance as seen on the -input of the op-amp.

The output resistance of the inverting op-amp circuit can be calculated in many ways, all working towards Ohm’s Law applied to the output port of the system. Driving the output port with an independent signal source yields:

rout = vout iout iout = vout R1 + R2 + vout A (v+ v) rout,opamp v+ = 0 v = βvout β = R2 R1 + R2, but we are not using this now iout = vout ( 1 R1 + R2 + 1 + A β rout,opamp ) rout = (R1 + R2)rout,opamp 1 + A β

It would be great if you’ve just experienced a déjà vu, since this derivation is almost identical to that of the non-inverting amplifier, a few pages back. Here, we again “see” the resistance of the β circuit at the output, parallel to the output resistance of the op-amp, decreased by a factor (1 + ). The output resistance is very low for a high or for a low rout,opamp.

7.2.3 Virtual ground

The inverting amplifier was covered in §7.2.2. For this circuit, the +-input of the amplifier was grounded, and the potential of the -input was almost equal to 0 V. Because the potential at the -input is almost at ground potential, though it is not actually grounded, this (type of) node is usually referred to a virtual ground. We analyse a number of issues for the part of the inverting amplifier on the right hand side of R2, see Figure 7.4.

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Figure 7.4: Input impedance... virtual ground point...

The input impedance of the circuit in Figure 7.4 is (with rout = 0Ω):

rin = vin iin vin = v v = vout A vout = v iin R1 v = v A + iin R1 A = iin R1 A + 1 vin = iin R1 A + 1 rin = R1 A + 1

So, for a large A, this input resistance is very low. For the limit case that A , the input impedance is 0Ω. The interesting part of this virtual ground node is that the (total) input current “sees” a low impedance, while this current is forced through an arbitrary impedance (here R1). This means that the circuit can function as a current-to-voltage converter: the input current sees an ideal (low impedance) input resistance and the input current is converted to an output voltage via R1.

7.2.4 Miller’s theorem

The phenomenon from the previous section can also be described using the Miller-effect[8]. Generalizing the resistance in the circuit of Figure 7.4 to an impedance Z, the voltage drop across this Z equals (1 + A) vin. The input impedance due to the combination of the amplifier with voltage gain A and the feedback impedance Z is:

Zin = Z 1 + A

Using a feedback resistor across a voltage amplifier with gain A results in a low input resistance for the circuit in Figure 7.4. Similarly, using a feedback capacitor results in a low input impedance, which corresponds to a high input capacitance Cin = Cfb (1 + A). Note that when wrapping this kind of feedback around a non-inverting amplifier it is also possible to create negative input resistances, negative input capacitances and more useful stuff.

7.2.5 The integrator

There is a variety of interesting frequency-dependent linear applications for the op-amp. One of the most simple applications is the integrator. For the configuration of Figure 7.5, we assume the op-amp to be ideal, meaning that A and rin Ω and rout = 0Ω. For this circuit, the output signal is

vout = Z1 Z2 vin (7.3) vout = vZ1 (iZ2(vin)) (7.4)

in the frequency domain and in time domain respectively.

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Figure 7.5: Basics for an integrator (or something else)

The vin vout relation of an integrator in time domain is something like vout = B vindt. By equating this to (7.4), it follows that an integrator can be created by:

These two generalizations are presented in Figure 7.6; a derivation of the relation between the input and output voltage is given below for the integrator using a capacitor. Obviously, the derivation for the integrator circuit with an inductor is very similar.

vout(t) = v vC(t) vC(t) = vC(0) + 1 C τ=0ti(τ) i(t) = vin(t) R2 vout(t) = vC(0) 1 RC τ=0tv in(τ)

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Figure 7.6: Integrator realisations

Substitution of the impedances in (7.3) yields an expression for an integrator in frequency domain: vout = 1 jωRC vin. From this it can be concluded that the term 1 corresponds to integration.

7.2.6 The differentiator

After the explanation, derivation, realization and obtaining some general knowledge of interesting facts considering the integrator, it may come to no surprise that we can also create differentiators with an op-amp circuit. Just like in §7.2.5, we can create a relation vout = B vin ∂t with the circuit in Figure 7.5 by:

The two situations are given in Figure 7.7. A derivation of the large-signal transfer is given below. The derivation for the differentiator with an inductor is completely analogous.

vout(t) = v vR(t) vR(t) = R1 iC(t) iC(t) = C2 vin(t) ∂t vout(t) = R1C2 vin(t) ∂t

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Figure 7.7: Differentiator realisations

Again, substitution of the (frequency domain) impedances in (7.3) yields an expression for a differentiator in frequency domain: vout = jωRC vin. From this it can be concluded that the term corresponds to differentiation; in Laplace transformation it is written as s. Note that both the circuit configurations and the transfer functions are their exact complement.

7.2.7 Summation of currents

Summing currents is fairly easy, according to Kirchhoff’s current law: the summed current flowing out of a node is equal to the sum of the currents flowing into that node. The only thing we need is a node that can drain the summed current: a zero-impedance node, and an output that gives some useful information about this summed current.

In §7.2.3, an op-amp circuit that converts an input current to an output voltage was discussed. For this circuit, the input node is virtual ground (very low ohmic). The circuit in Figure 7.4 can be reused to create a circuit that sums currents by only applying multiple input current sources, see the figure below:

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Figure 7.8: Current summing circuit with an ideal op-amp

It can easily be derived that the output voltage can be written as vout = R1 i=1..niin,i. Subtracting currents is just as easy by reversing the direction of an input current source. Changing current directions can, for instance, be done with a current mirror if we are using a unipolar current.

7.2.8 Summation of voltages

Adding voltages is quite easy if all the voltages are “floating”, i.e. if the terminals of the sources that provide the voltages to add are not referred to any other voltage level. In reality, this is however hardly ever the case. Noting that summing current is easy using the circuit in Figure 7.8, summing voltages can be done by first doing a V-I conversion and then using the current adder circuit in §7.2.7:

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Figure 7.9: Voltage summation with an ideal op-amp

The circuit in Figure 7.9 consists of n linear voltage-to-current converters (resistors), a current summation point (virtual ground point created by an op-amp with feedback) and a current-to-voltage converter (resistor R1). The transfer function can easily be determined (again with an ideal op-amp), for example using superposition:

vout = iR1 R1 iR1 = i=1..niin,i iin,i = vin,i rin,i vout = R1 i=1..nvin,i rin,i

If all input conversion resistors are equal, then the relation above simplifies to

vout = R1 rin i=1..nvin,i

The transfer can also be calculated using a non-ideal op-amp, but then the calculations become somewhat more complex.

7.2.9 Subtraction of voltages

As briefly discussed in §7.2.7, changing a current adder into a current subtractor is fairly straightforward. Subtracting voltages can be realized in a number of ways:

The latter method is generally used and results in the circuit in Figure 7.10.

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Figure 7.10: Differential stage for amplification of (vin,1 vin,2)

The signal transfer of this circuit can easily be determined by using the principle of superposition. By assuming (for simplicity) A :

vout = vout(v1)|v2=0 + vout(v2)|v1=0 vout(v1)|v2=0 = R2 R1 v1 vout(v2)|v1=0 = R4 R3 + R4 R1 + R2 R1 v2

To ensure vout to be proportional to (v1 v2), the next equation must be satisfied:

R3 R4 = R1 R2
(7.5)

resulting in a signal transfer given by

vout = R2 R1(v1 v2)
(7.6)

The input resistance of both inputs can again be calculated fairly easily by assuming A . The input resistance “seen” by source v1 equals R1; the input resistance “seen” from source v2 is equal to R3 + R4. We can make these input resistances equal by choosing a proper value for R3 and R4. Simple math then results in:

R4 = R1R2 R1 + R2
(7.7)

R3 = R12 R1 + R2
(7.8)

The output impedance of the circuit in Figure 7.10 is quite relevant if the circuit drives something else, which is always the case. For an op-amp with feedback and A , it is straight forward to derive that the output resistance is always rout 0Ω

7.2.10 Filters

Analog filters are required for many different applications54 . First-order filters can be constructed very easily using op-amps: a cascade of a first-order RC filter or a first-order RL filter and a unity gain voltage buffer stage using an op-amp does the job. The op-amp then takes care of a high ohmic load for the filter, while its low output impedance enables driving other circuitry without changing the filter characteristics55 .

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Figure 7.11: First-order filter with an op-amp: Z1 and Z2 determine the filter characteristics,R3 and R4 determine the gain and output resistance, together with the op-amp.

Using an ideal op-amp, the transfer function of the circuit in Figure 7.11 is:

H() = R3 + R4 R3 v+ v+ = Z2 Z1 + Z2 vin H() = R3 + R4 R3 Z2 Z1 + Z2

Using this principle, we can create a number of different filters. Usually, such filters have only one reactive element (C or L), resulting in a first-order filter. In general, the possibilities are:

Higher order filters can be easily constructed using cascades of first order and second order filters. The work by Sallen and Key [9] is well known for creating op-amp based filters.

Figure 7.11 shows the topology of a simple first order filter, wrapped around an opamp. For a generic nth-order filter, it can be shown that its transfer can be rewritten in a cascade of 1st and 2nd-order sections. This latter 2nd may not be simplified to a cascade of first-order transfers due to requiring real values corner frequencies.

To simplify the design of second order filters wrapped around an opamp (here), many easy-to-use standard configurations are available in literature. The most widely known are the so-called Sallen and Key [9] configurations. The basic topologies for the second order low-pass and high-pass filter configurations are shown below.

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Basic topologies for 2nd -order Sallen&Key (left) low pass and (right) high pass filters

Sallen and Key derived the transfer function, and rewrite that in a corner-frequency-independent form. Also rules to transform a low-pass filter into e.g. a high pass filter are provided by Sallen and Key. Below, a short review of only the low pass filters is provided. For the 2nd-order low pass configuration:

H() = K 1 + j ω ω0Q + ( ω0 )2 K = R3 + R4 R3 ω0 = 1 R1 R2 C1 C2 Q = R1 R2 C1 C2 R1C1 + R2C1 + R1C2(1 K)

This set of equation can be used in multiple ways to get a filter with (radian) corner frequency ω0 and quality factor Q. Using R1 = R2 = R and C1 = C2 = C simplifies the design procedure quite a bit as then

ω0 = 1 RC Q = 1 3 K

The only thing left is now to determine the ω0 and Q for the first and second order parts that make up your nth order filter. These ω0 and Q depend on the type of filtering characteristic you aim for. Well known characteristics include the Butterworth, Bessel and Chebyshev characteristics that yield a maximally flat frequency response in the passband, a smooth phase transition and a maximum steepness respectively. The ω0 and Q can be calculated from the characteristic polynomials for specific filter characteristics; below the polynomials for low-pass Butterworth filters are shown in Laplace notation with the frequency normalized to 1 rad/s.

order polynomial
1 (s + 1)
2 (s + 2s + 1)
3 (s + 1)(s2 + s + 1)
4 (s2 + 0,765s + 1)(s2 + 1,848s + 1)
5 (s + 1)(s2 + 0,618s + 1)(s2 + 1,618s + 1)
6 (s2 + 0,518s + 1)(s2 + 1,932s + 1)(s2 + 2s + 1)
Butterworth filter polynomials

The mapping of these polynomials on normalized ω0 and Q can easily be derived:

order FSF Q FSF Q FSF Q
1 1.0
2 1.0 0.7071
3 1.0 1.0000 1.0
4 1.0 0.5412 1.0 1.3065
5 1.0 0.6180 1.0 1.6181 1.0
6 1.0 0.5177 1.0 0.7071 1.0 1.9320
Butterworth filter parameters

This table should be read as follows:

Whereas for Butterworth filters the corner frequency of each individual section equals that of the overall filter, this is not the case for other filter characteristics. As example, the table below shows the (FSF,Q) for a Chebyshev filter with a maximum 1dB ripple in the pass band. Note here that FSF may deviate quite a bit from 1:

order FSF Q FSF Q FSF Q
1 0.5088
2 1.0500 0.9565
3 0.9971 2.0176 0.4942
4 0.9932 0.7845 0.5286 3.5600
5 0.9941 1.3988 0.6652 5.5538 0.2895
6 0.9953 0.7608 0.7468 2.1977 0.3532 8.0012
Chebyshev filterparameters (1 dB ripple)

Transforming the characteristic polynomials into high pass filters is relatively easy: replacing s by 1s, which is based on the symmetry (in a Bode plot, with respect to the frequency axis) between the low pass and high pass transfer functions. A lot more to write and say about filter design, but way too little space and time.

7.3 Feedback with non-linear elements

Many linear applications of the op-amp are discussed in §7.2. The applications of op-amps, however, is not limited to linear applications. This section presents feedback using non-linear elements. Although this is not used in modern times, it does give insight in negative feedback circuits. For that reason below a logarithmic expander and compressor are discussed; other non-linear circuits using op-amps include multipliers and an “ideal” rectifier.

7.3.1 Logarithmic conversion

A well known non-linear application — at least in the previous millennium — of an op-amp is the logarithmic converter; this converter has an output signal proportional to the logarithm of the input signal:

vOUT log(vIN)

Examining the signal transfer of a normal inverting amplifier, using an op-amp and two linear resistors vOUT = Rfeedback Rin vIN it can be derived that this transfer is the result of the V-I converter with Rin and subsequent I-V conversion of the current generated by Rin using Rfeedback. In mathematical form:

vOUT = vRfeedback (iRin(vIN))

From here, we conclude that we can create a logarithmic converter in (at least) 2 ways:

The first resistive element can be realized with a diode-like element; the second element cannot be realized very easily. If we use the above principle, then we get the circuit in the figure below:

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Logarithmic converter

The transfer of this circuit has to be calculated using large-signal (time domain) analyses, due to the non-linearities. With an ideal op-amp and neglecting the factor “-1” in the diode equation, we get:

vOUT = vD(iD) vD(iD) = kT q ln (iD I0 1) iD = iR = vIN R vOUT = kT q ln ( vIN R I0 )

7.3.2 Exponential converters

A strongly related non-linear application of op-amp circuits is the exponential converter; this type of circuit performs the complementary operation of the circuit in §7.3.1. Starting with an inverting amplifier configuration, where

vOUT = vRfeedback (iRin(vIN))

then we see that to create an exponential converter, (at least) two methods result:

Again, the diode-like element allows us to realise one of these possibilities, resulting in the next circuit:

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Exponential converter

The transfer function can now simply be derived if we assume the op-amp to be ideal (an infinite gain and other convenient issues):

vOUT = R ID0 eqvIN kT
(7.9)

7.4 Op-amp non-idealities

So far, we have always assumed op-amps to be ideal. As stated at the beginning of this chapter, the most important assumptions for an ideal op-amp are:

In reality, we have not got any ideal op-amps, simply because they are built up from non-ideal electronic components. The most important non-ideal effects of op-amps will be discussed in this subchapter.

7.4.1 Frequency-dependent gain

An op-amp is actually built from transistors and passive components (resistors, capacitors). The underlying circuits must always consist of multiple amplifier stages, all with their own bandwidth (limitation), since the op-amp is required to have a very high voltage gain with high input impedance and low output impedance.

The op-amp has, almost by definition, a frequency-dependent transfer function. From chapter 6 it should be no big surprise that most op-amps are designed to be dominantly first-order (idiot-proof that is). The effect of frequency dependency of op-amps on any system property is easily derived by calculating the desired property for an unspecified voltage gain A and after deriving that, substituting the actual — frequency dependent — A(). For unity-gain-stable op-amps, that are dominantly first order, this just boils down to substituting A() = A0 1+jωτ or something similar. To get readable results, sometimes the result must still be rewritten.

7.4.2 First-order behavior and slew rate

While analysing op-amps, we have so far assumed the op-amp to be capable of delivering any output current level. However, this is not the case:

Both effects and the impact of those effects will be discussed within this subchapter.

7.4.3 Internal current limitation and load

A typical setup of an op-amp is shown in Figure 7.12: the circuit consists of a differential pair (a differential version of a CEC, sse chapter 8) followed by a CSC and CDC amplifier stage. The node connecting the differential pair and the CSC is loaded by capacitor Csr. The exact operation of the entire circuit schematic is not of interest right now; but it is important that the current flowing into or out of (e.g.) capacitor Cst is (lower and upper) limited.

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Figure 7.12: Example of circuit where the maximal rise/fall speed (slew rate) is internally limited: the opamp consists of a differential pair ( balanced CEC), CSC and CDC; slew rate limitation implemented by Csr.

The presence of the capacitor causes:

This internal slew rate limitation results in a limited slew rate of the op-amp’s output voltage. This limitation (slew rate, in short: SR) is:

|dvOUT dt |max SR = ACSC ACDC Imax C

where ACSC is the voltage gain of the common-source stage formed by the PMOS transistor and ACDC is the voltage gain of the common-drain stage stage implemented by the MOS transistor.

If the op-amp ideally would create an output signal vOUT = V out sin(ω t), with a maximum slew rate of (ω V out), then we can directly see that the maximum output voltage for which the signal’s angular frequency ω would be undistorted is:

V out,max = SR ω

Figure 7.13 illustrates the impact of slewing on signals. The smallest two sine waves corresponds to the undistorted signal, without any slewing effect. For the larger (thick, red) sine, the signal is distorted because the required slew rate to get an undistorted sine is larger than the slew-rate limitation imposed by the circuit. In this example, slewing at the rising edge is assumed. The gray curve markes the undistorted version of the actual slewing-distorted curve and is included to clearly see the impact of slewing. It can be seen in the figure that slewing results in a rather distorted signal.

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Figure 7.13: The impact of slewing on (here) sines: the smallest two sines do not result in slewing, whereas the larger slews at — here only — the rising edge. The gray curve would correspond to a sine that is not affected by slewing.

In Figure 7.13, the slewing effect has only been shown in the rising side of the sine while an undistorted sine was included to see the impact of slewing. Op-amps can have a symmetric or asymmetric slewing, depending on the internal circuit schematic and biasing.

7.4.4 Internal current restrictions and external load

In the previous section, the slewing was due to the internal current limitation of an internal capacitor. However, the output current of an op-amp is usually also limited, which can cause slewing due to the output current limitation combined with an external (load) capacitance; same story, same effect, same misery.