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  • Operational Amplifiers:

    The operational amplifier is a direct-coupled high gain amplifier usable from 0 to over 1MH Z to which feedback is added to control its overall response characteristic i.e. gain and bandwidth. The op-amp exhibits the gain down to zero frequency.

    Such direct coupled (dc) amplifiers do not use blocking (coupling and by pass) capacitors since these would reduce the amplification to zero at zero frequency. Large by pass capacitors may be used but it is not possible to fabricate large capacitors on a IC chip. The capacitors fabricated are usually less than 20 pf. Transistor, diodes and resistors are also fabricated on the same chip.

    Differential Amplifiers:

    Differential amplifier is a basic building block of an op-amp. The function of a differential amplifier is to amplify the difference between two input signals.

    How the differential amplifier is developed? Let us consider two emitter-biased circuits as shown in fig. 1.

    Fig. 1

    The two transistors Q1 and Q2 have identical characteristics. The resistances of the circuits are equal, i.e. RE1 = R E2, RC1 = R C2 and the magnitude of +VCC is equal to the magnitude of VEE. These voltages are measured with respect to ground.

    To make a differential amplifier, the two circuits are connected as shown in fig. 1. The two +VCC and VEE supply terminals are made common because they are same. The two emitters are also connected and the parallel combination of RE1 and RE2 is replaced by a resistance RE. The two input signals v1 & v2 are applied at the base of Q1 and at the base of Q2. The output voltage is taken between two collectors. The collector resistances are equal and therefore denoted by RC = RC1 = RC2.

  • Ideally, the output voltage is zero when the two inputs are equal. When v1 is greater then v2 the output voltage with the polarity shown appears. When v1 is less than v2, the output voltage has the opposite polarity.

    The differential amplifiers are of different configurations.

    The four differential amplifier configurations are following:

    1. Dual input, balanced output differential amplifier. 2. Dual input, unbalanced output differential amplifier. 3. Single input balanced output differential amplifier. 4. Single input unbalanced output differential amplifier.

  • Fig. 2

    These configurations are shown in fig. 2, and are defined by number of input signals used and the way an output voltage is measured. If use two input signals, the configuration is said to be dual input, otherwise it is a single input configuration. On the other hand, if the output voltage is measured between two collectors, it is referred to as a balanced output because both the collectors are at the same dc potential w.r.t. ground. If the output is measured at one of the collectors w.r.t. ground, the configuration is called an unbalanced output.

    A multistage amplifier with a desired gain can be obtained using direct connection between successive stages of differential amplifiers. The advantage of direct coupling is that it removes the lower cut off frequency imposed by the coupling capacitors, and they are therefore, capable of amplifying dc as well as ac input signals.

    Dual Input, Balanced Output Differential Amplifier:

    The circuit is shown in fig. 1, v1 and v2 are the two inputs, applied to the bases of Q1 and Q2 transistors. The output voltage is measured between the two collectors C1 and C2 , which are at same dc potentials.

    D.C. Analysis:

    To obtain the operating point (ICC and VCEQ) for differential amplifier dc equivalent circuit is drawn by reducing the input voltages v1 and v2 to zero as shown in fig. 3.

    Fig. 3

    The internal resistances of the input signals are denoted by RS because RS1= RS2. Since both emitter biased sections of the different amplifier are symmetrical in all respects, therefore, the operating point for only one section need to be determined. The same values of ICQ and VCEQ can be used for second transistor Q2.

  • Applying KVL to the base emitter loop of the transistor Q1.

    The value of RE sets up the emitter current in transistors Q1 and Q2 for a given value of VEE. The emitter current in Q1 and Q2 are independent of collector resistance RC.

    The voltage at the emitter of Q1 is approximately equal to -VBE if the voltage drop across R is negligible. Knowing the value of IC the voltage at the collector VCis given by

    VC =VCC IC RC

    and VCE = VC VE

    = VCC IC RC + VBE

    VCE = VCC + VBE ICRC (E-2)

    From the two equations VCEQ and ICQ can be determined. This dc analysis applicable for all types of differential amplifier.

    Example - 1

    The following specifications are given for the dual input, balanced-output differential amplifier of fig.1: RC = 2.2 k, RB = 4.7 k, Rin 1 = Rin 2 = 50 , +VCC = 10V, -VEE = -10 V, dc =100 and VBE = 0.715V. Determine the operating points (ICQ and VCEQ) of the two transistors.

    Solution:

    The value of ICQ can be obtained from equation (E-1).

  • The voltage VCEQ can be obtained from equation (E-2).

    The values of ICQ and VCEQ are same for both the transistors.

    Dual Input, Balanced Output Difference Amplifier:

    The circuit is shown in fig. 1 v1 and v2 are the two inputs, applied to the bases of Q1 and Q2 transistors. The output voltage is measured between the two collectors C1 and C2, which are at same dc potentials.

    Fig. 1

    A.C. Analysis :

    In previous lecture dc analysis has been done to obtain the operatiing point of the two transistors.

    To find the voltage gain Ad and the input resistance Ri of the differential amplifier, the ac equivalent circuit is drawn using r-parameters as shown in fig. 2. The dc voltages are reduced to zero and the ac equivalent of CE configuration is used.

  • Fig. 2

    Since the two dc emitter currents are equal. Therefore, resistance r'e1 and r'e2 are also equal and designated by r'e . This voltage across each collector resistance is shown 180 out of phase with respect to the input voltages v1 and v2. This is same as in CE configuration. The polarity of the output voltage is shown in Figure. The collector C2 is assumed to be more positive with respect to collector C1 even though both are negative with respect to to ground.

    Applying KVL in two loops 1 & 2.

    Substituting current relations,

    Again, assuming RS1 / b and RS2 / b are very small in comparison with RE and re' and therefore neglecting these terms,

  • Solving these two equations, ie1 and ie2 can be calculated.

    The output voltage VO is given by

    VO = VC2 - VC1

    = -RC iC2 - (-RC iC1)

    = RC (iC1 - iC2)

    = RC (ie1 - ie2)

    Substituting ie1, & ie2 in the above expression

    Thus a differential amplifier amplifies the difference between two input signals. Defining the difference of input signals as vd = v1 v2 the voltage gain of the dual input balanced output differential amplifier can be given by

    (E-2)

    Differential Input Resistance:

    Differential input resistance is defined as the equivalent resistance that would be measured at either input terminal with the other terminal grounded. This means that the input resistance Ri1 seen from the input signal source v1 is determined with the signal source v2 set at zero. Similarly, the input signal v1 is set at zero to determine the input resistance Ri2 seen from the input signal source v2. Resistance RS1 and RS2 are ignored because they are very small.

  • Substituting ie1,

    Similarly,

    The factor of 2 arises because the re' of each transistor is in series.

    To get very high input impedance with differential amplifier is to use Darlington transistors. Another ways is to use FET.

    Output Resistance:

    Output resistance is defined as the equivalent resistance that would be measured at output terminal with respect to ground. Therefore, the output resistance RO1 measured between collector C1 and ground is equal to that of the collector resistance RC. Similarly the output resistance RO2 measured at C2 with respect to ground is equal to that of the collector resistor RC.

    RO1 = RO2 = RC (E-5)

    The current gain of the differential amplifier is undefined. Like CE amplifier the differential amplifier is a small signal amplifier. It is generally used as a voltage amplifier and not as current or power amplifier.

    Example - 1

  • The following specifications are given for the dual input, balanced-output differential amplifier: RC = 2.2 k, RB = 4.7 k, Rin 1 = Rin 2 = 50, +VCC= 10V, -VEE = -10 V, dc =100 and VBE = 0.715V.

    a. Determine the voltage gain. b. Determine the input resistance c. Determine the output resistance.

    Solution:

    (a). The parameters of the amplifiers are same as discussed in example-1 of lecture-1. The operating point of the two transistors obtained in lecture-1 are given below

    ICQ = 0.988 mA VCEQ=8.54V

    The ac emitter resistance

    Therefore, substituting the known values in voltage gain equation (E-2), we obtain

    b). The input resistance seen from each input source is given by (E-3) and (E-4):

    (c) The output resistance seen looking back into the circuit from each of the two output terminals is given by (E-5)

    Ro1 = Ro2 = 2.2 k

    Example - 2

    For the dual input, balanced output differential amplifier of Example-1:

    a. Determine the output voltage (vo) if vin 1 = 50mV peak to peak (pp) at 1 kHz and vin 2 = 20 mV pp at 1 kHz.

    b. What is the maximum peal to peak output voltage without clipping?

    Solution:

  • (a) In Example-1 we have determined the voltage gain of the dual input, balanced output differential amplifier. Substituting this voltage gain (Ad = 86.96) and given values of input voltages in (E-1), we get

    (b) Note that in case of dual input, balanced output difference amplifier, the output voltage vo is measured across the collector. Therefore, to calculate the maximum peak to peak output voltage, we need to determine the voltage drop across each collector resistor:

    Substituting IC = ICQ = 0.988 mA, we get

    This means that the maximum change in voltage across each collector resistor is 2.17 (ideally) or 4.34 VPP. In other words, the maximum peak to peak output voltage with out clipping is (2) (4.34) = 8.68 VPP.

    A dual input, balanced output difference amplifier circuit is shown in fig. 1.

    Fig. 1

    Inverting & Non inverting Inputs:

    In differential amplifier the output voltage vO is given by

  • VO = Ad (v1 v2) When v2 = 0, vO = Ad v1 & when v1 = 0, vO = - Ad v2

    Therefore the input voltage v1 is called the non inventing input because a positive voltage v1 acting alone produces a positive output voltage vO. Similarly, the positive voltage v2 acting alone produces a negative output voltage hence v2 is called inverting input. Consequently B1 is called noninverting input terminal and B2 is called inverting input terminal.

    Common mode Gain:

    A common mode signal is one that drives both inputs of a differential amplifier equally. The common mode signal is interference, static and other kinds of undesirable pickup etc.

    The connecting wires on the input bases act like small antennas. If a differential amplifier is operating in an environment with lot of electromagnetic interference, each base picks up an unwanted interference voltage. If both the transistors were matched in all respects then the balanced output would be theoretically zero. This is the important characteristic of a differential amplifier. It discriminates against common mode input signals. In other words, it refuses to amplify the common mode signals.

    The practical effectiveness of rejecting the common signal depends on the degree of matching between the two CE stages forming the differential amplifier. In other words, more closely are the currents in the input transistors, the better is the common mode signal rejection e.g. If v1 and v2 are the two input signals, then the output of a practical op-amp cannot be described by simply

    v0 = Ad (v1 v2 )

    In practical differential amplifier, the output depends not only on difference signal but also upon the common mode signal (average).

    vd = (v1 vd )

    and vC = (v1 + v2 )

    The output voltage, therefore can be expressed as

    vO = A1 v1 + A2 v2

    Where A1 & A2 are the voltage amplification from input 1(2) to output under the condition that input 2 (1) is grounded.

  • The voltage gain for the difference signal is Ad and for the common mode signal is AC.

    The ability of a differential amplifier to reject a common mode signal is expressed by its common mode rejection ratio (CMRR). It is the ratio of differential gain Ad to the common mode gain AC.

    Date sheet always specify CMRR in decibels CMRR = 20 log CMRR.

    Therefore, the differential amplifier should be designed so that r is large compared with the ratio of the common mode signal to the difference signal. If r = 1000, vC = 1mV, vd = 1 m V, then

    It is equal to first term. Hence for an amplifier with r = 1000, a 1m V difference of potential between two inputs gives the same output as 1mV signal applied with the same polarity to both inputs.

    Dual Input, Unbalanced Output Differential Amplifier:

    In this case, two input signals are given however the output is measured at only one of the two-collector w.r.t. ground as shown in fig. 2. The output is referred to as an unbalanced output because the collector at which the output voltage is measured is at some finite dc potential with respect to ground..

  • Fig. 2

    In other words, there is some dc voltage at the output terminal without any input signal applied. DC analysis is exactly same as that of first case.

    AC Analysis:

    The output voltage gain in this case is given by

    The voltage gain is half the gain of the dual input, balanced output differential amplifier. Since at the output there is a dc error voltage, therefore, to reduce the voltage to zero, this configuration is normally followed by a level translator circuit.

    Differential amplifier with swamping resistors:

    By using external resistors R'E in series with each emitter, the dependence of voltage gain on variations of r'e can be reduced. It also increases the linearity range of the differential amplifier.

    Fig. 3, shows the differential amplifier with swamping resistor R'E. The value of R'E is usually large enough to swamp the effect of r'e.

  • Fig. 3

    Dual Input, Unbalanced Output Differential Amplifier:

    In this case, two input signals are given however the output is measured at only one of the two-collector w.r.t. ground as shown in fig. 2. The output is referred to as an unbalanced output because the collector at which the output voltage is measured is at some finite dc potential with respect to ground..

  • Fig. 2

    In other words, there is some dc voltage at the output terminal without any input signal applied. DC analysis is exactly same as that of first case.

    AC Analysis:

    The output voltage gain in this case is given by

    The voltage gain is half the gain of the dual input, balanced output differential amplifier. Since at the output there is a dc error voltage, therefore, to reduce the voltage to zero, this configuration is normally followed by a level translator circuit.

    Differential amplifier with swamping resistors:

    By using external resistors R'E in series with each emitter, the dependence of voltage gain on variations of r'e can be reduced. It also increases the linearity range of the differential amplifier.

    Fig. 3, shows the differential amplifier with swamping resistor R'E. The value of R'E is usually large enough to swamp the effect of r'e.

  • Fig. 3

    Example-1

    Consider example-1 of lecture-2. The specifications are given again for the dual input, unbalanced-output differential amplifier: RC = 2.2 k, RB= 4.7 k, Rin1 = Rin2= 50, +VCC = 10V, -VEE= -10 V, dc =100 and VBE= 0.715V.

    Determine the voltage gain, input resistance and the output resistance.

    Solution:

  • Since the component values remain unchanged and the biasing arrangement is same, the ICQ and VCEQ values as well as input and output resistance values for the dual input, unbalanced output configuration must be the same as those for the dual input, balanced output configuration.

    Thus, ICQ = 0.988 mA VCEQ = 8.54 V Ri1 = Ri2 = 5.06 k Ro = 2.2 k

    The voltage gain of the dual input, unbalanced output differential amplifier is given by

    Example-2

    Repeat Example-1 for single input, balanced output differential amplifier.

    Solution:

    Because the same biasing arrangement and same component values are used in both configurations, the results obtained in Example-1 for the dual input, balanced output configuration are also valid for the single input, balanced output configuration.

    That is,

    ICQ= 0.988 mA VCEQ = 8.54 V Vd = 86.96 Ri = 5.06 k Ro1 = Ro2 = 2.2 k

    Constant Current Bias:

    In the dc analysis of differential amplifier, we have seen that the emitter current IE depends upon the value of bdc. To make operating point stable IE current should be constant irrespective value of bdc.

    For constant IE, RE should be very large. This also increases the value of CMRR but if RE value is increased to very large value, IE (quiescent operating current) decreases. To maintain same value of IE, the emitter supply VEE must be increased. To get very high value of resistance RE and constant IE, current, current bias is used.

  • Figure 5.1

    Fig. 1, shows the dual input balanced output differential amplifier using a constant current bias. The resistance RE is replace by constant current transistor Q3. The dc collector current in Q3 is established by R1, R2, & RE.

    Applying the voltage divider rule, the voltage at the base of Q3 is

    Because the two halves of the differential amplifiers are symmetrical, each has half of the current IC3.

  • The collector current, IC3 in transistor Q3 is fixed because no signal is injected into either the emitter or the base of Q3.

    Besides supplying constant emitter current, the constant current bias also provides a very high source resistance since the ac equivalent or the dc source is ideally an open circuit. Therefore, all the performance equations obtained for differential amplifier using emitter bias are also valid.

    As seen in IE expressions, the current depends upon VBE3. If temperature changes, VBE changes and current IE also changes. To improve thermal stability, a diode is placed in series with resistance R1as shown in fig. 2.

    Fig. 2 This helps to hold the current IE3 constant even though the temperature changes. Applying KVL to the base circuit of Q3.

    Therefore, the current IE3 is constant and independent of temperature because of the added diode D. Without D the current would vary with temperature because VBE3 decreases approximately by 2mV/ C. The diode has same temperature dependence and hence the two variations cancel each

  • other and IE3 does not vary appreciably with temperature. Since the cut in voltage VD of diode approximately the same value as the base to emitter voltage VBE3 of a transistor the above condition cannot be satisfied with one diode. Hence two diodes are used in series for VD. In this case the common mode gain reduces to zero.

    Some times zener diode may be used in place of diodes and resistance as shown in fig. 3. Zeners are available over a wide range of voltages and can have matching temperature coefficient

    The voltage at the base of transistor QB is

    Fig. 3

    The value of R2 is selected so that I2 1.2 IZ(min) where IZ is the minimum current required to cause the zener diode to conduct in the reverse region, that is to block the rated voltage VZ.

    Current Mirror:

    The circuit in which the output current is forced to equal the input current is said to be a current mirror circuit. Thus in a current mirror circuit, the output current is a mirror image of the input current. The current mirror circuit is shown in fig. 4.

  • Fig. 4

    Once the current I2 is set up, the current IC3 is automatically established to be nearly equal to I2. The current mirror is a special case of constant current bias and the current mirror bias requires of constant current bias and therefore can be used to set up currents in differential amplifier stages. The current mirror bias requires fewer components than constant current bias circuits.

    Since Q3 and Q4 are identical transistors the current and voltage are approximately same

    For satisfactory operation two identical transistors are necessary.

    Example - 1

  • Design a zener constant current bias circuit as shown in fig. 5 according to the following specifications. (a). Emitter current -IE = 5 mA (b). Zener diode with Vz = 4.7 V and Iz = 53 mA. (c). ac = dc = 100, VBE = 0.715V (d). Supply voltage - VEE = - 9 V.

    Solution:

    From fig. 6 using KVL we get

    Fig. 5

    Practically we use RE = 820 k

    Practically we use R2 = 68 The designed component values are: RE = 860 R2 = 68

    Fig. 6

    Example - 2

    Design the dual-input balanced output differential amplifier using the diode constant current bias to meet the following specifications.

    1. supply voltage = 12 V. 2. Emitter current IE in each differential amplifier transistor = 1.5 mA. 3. Voltage gain 60.

  • Solution:

    The voltage at the base of transistor Q3 is

    Assuming that the transistor Q3 has the same characteristics as diode D1 and D2 that is VD = VBE3, then

    Practically we take RE = 240 .

    Practically we take R2 = 3.6 k.

    To obtain the differential gain of 60, the required value of the collector resistor is

    The following fig. 7 shows the dual input, balanced output differential amplifier with the designed component values as RC = 1K, RE = 240 , and R2 = 3.6K.

    Fig. 7

  • The operation amplifier:

    An operational amplifier is a direct coupled high gain amplifier consisting of one or more differential (OPAMP) amplifiers and followed by a level translator and an output stage. An operational amplifier is available as a single integrated circuit package.

    The block diagram of OPAMP is shown in fig. 1.

    Fig. 1

    The input stage is a dual input balanced output differential amplifier. This stage provides most of the voltage gain of the amplifier and also establishes the input resistance of the OPAMP.The intermediate stage of OPAMP is another differential amplifier which is driven by the output of the first stage. This is usually dual input unbalanced output.

    Because direct coupling is used, the dc voltage level at the output of intermediate stage is well above ground potential. Therefore level shifting circuit is used to shift the dc level at the output downward to zero with respect to ground. The output stage is generally a push pull complementary amplifier. The output stage increases the output voltage swing and raises the current supplying capability of the OPAMP. It also provides low output resistance.

    Level Translator:

    Because of the direct coupling the dc level at the emitter rises from stages to stage. This increase in dc level tends to shift the operating point of the succeeding stages and therefore limits the output voltage swing and may even distort the output signal.

    To shift the output dc level to zero, level translator circuits are used. An emitter follower with voltage divider is the simplest form of level translator as shown in fig. 2.

    Thus a dc voltage at the base of Q produces 0V dc at the output. It is decided by R1 and R2. Instead of voltage divider emitter follower either with diode current bias or current mirror bias as shown in fig. 3 may be used to get

    Fig. 2

  • Fig. 3

    Fig. 4, shows a complete OPAMP circuit having input different amplifiers with balanced output, intermediate stage with unbalanced output, level shifter and an output amplifier.

    better results.

    In this case, level shifter, which is common collector amplifier, shifts the level by 0.7V. If this shift is not sufficient, the output may be taken at the junction of two resistors in the emitter leg.

  • Fig. 4

    Example-1:

    For the cascaded differential amplifier shown in fig. 5, determine:

    The collector current and collector to emitter voltage for each transistor. The overall voltage gain. The input resistance. The output resistance.

    Assume that for the transistors used hFE = 100 and VBE = 0.715V

  • Fig. 5

    Solution:

    (a). To determine the collector current and collector to emitter voltage of transistors Q1 and Q2, we assume that the inverting and non-inverting inputs are grounded. The collector currents (IC IE) in Q1 and Q2 are obtained as below:

    That is, IC1 = IC2 =0.988 mA.

    Now, we can calculate the voltage between collector and emitter for Q1 and Q2 using the collector current as follows:

    VC1 = VCC = -RC1 IC1 = 10 (2.2k) (0.988 mA) = 7.83 V = VC2

    Since the voltage at the emitter of Q1 and Q2 is -0.715 V,

    VCE1 = VCE2 = VC1 -VE1 = 7.83 + 0715 = 8.545 V

    Next, we will determine the collector current in Q3 and Q4 by writing the Kirchhoff's voltage equation for the base emitter loop of the transistor Q3:

    VCC RC2 IC2 = VBE3 - R'E IC3 - RE2 (2 IE3) + VBE= 0 10 (2.2k) (0.988mA) - 0.715 - (100) (IE3) (30k) IE3 + 10=0

  • 10 - 2.17 - 0.715 + 10 - (30.1k) IE3 = 0

    Hence the voltage at the collector of Q3 and Q4 is

    VC3 = VC4= VCC RC3 IC3 = 10 (1.2k) (0.569 mA)

    = 9.32 V

    Therefore,

    VCE3 = VVCE4 = VC3 VE3 = 9.32 7.12 = 2.2 V

    Thus, for Q1 and Q2: ICQ = 0.988 mA VCEQ = 8.545 V and for Q3 and Q4: ICQ = 0.569 mA VCEQ = 2.2 V

    [Note that the output terminal (VC4) is at 9.32 V and not at zero volts.]

    (b). First, we calculate the ac emitter resistance r'e of each stage and then its voltage gain.

    The first stage is a dual input, balanced output differential amplifier, therefore, its voltage gain is

    Where

    Ri2 = input resistance of the second stage

    The second stage is dual input, unbalanced output differential amplifier with swamping resistor R'E, the voltage gain of which is

  • Hence the overall voltage gain is

    Ad= (Ad1) (Ad2) = (80.78) (4.17) = 336.85

    Thus we can obtain a higher voltage gain by cascading differential amplifier stages.

    (c).The input resistance of the cascaded differential amplifier is the same as the input resistance of the first stage, that is

    Ri = 2ac(re1) = (200) (25.3) = 5.06 k

    (d). The output resistance of the cascaded differential amplifier is the same as the output resistance of the last stage. Hence,

    RO = RC = 1.2 k

    Example-2:

    For the circuit show in fig. 6, it is given that =100, VBE =0715V. Determine

    The dc conditions for each state The overall voltage gain The maximum peak to peak output voltage swing.

    Fig. 6

  • Solution:

    (a). The base currents of transistors are neglected and VBE drops of all transistors are assumed same.

    From the dc equivalent circuit,

    and

    b) The overall voltage gain of the amplifier can be obtained as below:

    Therefore, voltage gain of second stage

    The input impedance of second stage is

    The effective load resistance for first stage is

    Therefore, the voltage gain of first stage is

  • The overall voltge gain is AV = AV1 AV2

    (c). The maximum peak to peak output votage swing = Vopp = 2 (VC7 - VE7) = 2 x (5.52 - 3.325) = 4.39 V

    The symbolic diagram of an OPAMP is shown in fig. 1.

    741c is most commonly used OPAMP available in IC package. It is an 8-pin DIP chip.

    Parameters of OPAMP:

    The various important parameters of OPAMP are follows:

    1.Input Offset Voltage:

    Input offset voltage is defined as the voltage that must be applied between the two input terminals of an OPAMP to null or zero the output fig. 2, shows that two dc voltages are applied to input terminals to make the output zero.

    Vio = Vdc1 Vdc2

    Vdc1 and Vdc2 are dc voltages and RS represents the source resistance. Vio is the difference of Vdc1 and Vdc2. It may be positive or negative. For a 741C OPAMP the maximum value of Vio is

    Fig. 2

  • 6mV. It means a voltage 6 mV is required to one of the input to reduce the output offset voltage to zero. The smaller the input offset voltage the better the differential amplifier, because its transistors are more closely matched.

    2. Input offset Current:

    The input offset current Iio is the difference between the currents into inverting and non-inverting terminals of a balanced amplifier.

    Iio = | IB1 IB2 |

    The Iio for the 741C is 200nA maximum. As the matching between two input terminals is improved, the difference between IB1 and IB2 becomes smaller, i.e. the Iio value decreases further.For a precision OPAMP 741C, Iio is 6 nA

    3.Input Bias Current:

    The input bias current IB is the average of the current entering the input terminals of a balanced amplifier i.e.

    IB = (IB1 + IB2 ) / 2

    For 741C IB(max) = 700 nA and for precision 741C IB = 7 nA

    4. Differential Input Resistance: (Ri)

    Ri is the equivalent resistance that can be measured at either the inverting or non-inverting input terminal with the other terminal grounded. For the 741C the input resistance is relatively high 2 M. For some OPAMP it may be up to 1000 G ohm.

    5. Input Capacitance: (Ci)

    Ci is the equivalent capacitance that can be measured at either the inverting and noninverting terminal with the other terminal connected to ground. A typical value of Ci is 1.4 pf for the 741C.

    6. Offset Voltage Adjustment Range:

    741 OPAMP have offset voltage null capability. Pins 1 and 5 are marked offset null for this purpose. It can be done by connecting 10 K ohm pot between 1 and 5 as shown in fig. 3.

  • Fig. 3

    By varying the potentiometer, output offset voltage (with inputs grounded) can be reduced to zero volts. Thus the offset voltage adjustment range is the range through which the input offset voltage can be adjusted by varying 10 K pot. For the 741C the offset voltage adjustment range is 15 mV.

    Parameters of OPAMP:

    7. Input Voltage Range :

    Input voltage range is the range of a common mode input signal for which a differential amplifier remains linear. It is used to determine the degree of matching between the inverting and noninverting input terminals. For the 741C, the range of the input common mode voltage is 13V maximum. This means that the common mode voltage applied at both input terminals can be as high as +13V or as low as 13V.

    8. Common Mode Rejection Ratio (CMRR).

    CMRR is defined as the ratio of the differential voltage gain Ad to the common mode voltage gain ACM

    CMRR = Ad / ACM.

    For the 741C, CMRR is 90 dB typically. The higher the value of CMRR the better is the matching between two input terminals and the smaller is the output common mode voltage.

    9. Supply voltage Rejection Ratio: (SVRR)

    SVRR is the ratio of the change in the input offset voltage to the corresponding change in power supply voltages. This is expressed in m V / V or in decibels, SVRR can be defined as

  • SVRR = D Vio / D V

    Where D V is the change in the input supply voltage and D Vio is the corresponding change in the offset voltage.

    For the 741C, SVRR = 150 V / V.

    For 741C, SVRR is measured for both supply magnitudes increasing or decreasing simultaneously, with R3 10K. For same OPAMPS, SVRR is separately specified as positive SVRR and negative SVRR.

    10. Large Signal Voltage Gain:

    Since the OPAMP amplifies difference voltage between two input terminals, the voltage gain of the amplifier is defined as

    Because output signal amplitude is much large than the input signal the voltage gain is commonly called large signal voltage gain. For 741C is voltage gain is 200,000 typically.

    11. Output voltage Swing:

    The ac output compliance PP is the maximum unclipped peak to peak output voltage that an OPAMP can produce. Since the quiescent output is ideally zero, the ac output voltage can swing positive or negative. This also indicates the values of positive and negative saturation voltages of the OPAMP. The output voltage never exceeds these limits for a given supply voltages +VCC and VEE. For a 741C it is 13 V.

    12. Output Resistance: (RO)

    RO is the equivalent resistance that can be measured between the output terminal of the OPAMP and the ground. It is 75 ohm for the 741C OPAMP.

    Example - 1

    Determine the output voltage in each of the following cases for the open loop differential amplifier of fig. 4:

    a. vin 1 = 5 m V dc, vin 2 = -7 Vdc b. vin 1 = 10 mV rms, vin 2= 20 mV rms

  • Fig. 4

    Specifications of the OPAMP are given below: A = 200,000, Ri = 2 M , R O = 75, + VCC = + 15 V, - VEE = - 15 V, and output voltage swing = 14V.

    Solution:

    (a). The output voltage of an OPAMP is given by

    Remember that vo = 2.4 V dc with the assumption that the dc output voltage is zero when the input signals are zero.

    (b). The output voltage equation is valid for both ac and dc input signals. The output voltage is given by

    Thus the theoretical value of output voltage vo = -2000 V rms. However, the OPAMP saturates at 14 V. Therefore, the actual output waveform will be clipped as shown fig. 5. This non-sinusoidal waveform is unacceptable in amplifier applications.

  • Fig. 5

    13. Output Short circuit Current :

    In some applications, an OPAMP may drive a load resistance that is approximately zero. Even its output impedance is 75 ohm but cannot supply large currents. Since OPAMP is low power device and so its output current is limited. The 741C can supply a maximum short circuit output current of only 25mA.

    14. Supply Current :

    IS is the current drawn by the OPAMP from the supply. For the 741C OPAMP the supply current is 2.8 m A.

    15. Power Consumption:

    Power consumption (PC) is the amount of quiescent power (vin= 0V) that must be consumed by the OPAMP in order to operate properly. The amount of power consumed by the 741C is 85 m W.

    Parameters of OPAMP:

    16. Gain Bandwidth Product:

  • The gain bandwidth product is the bandwidth of the OPAMP when the open loop voltage gain is reduced to 1. From open loop gain vs frequency graph At 1 MHz shown in. fig. 6, It can be found 1 MHz for the 741C OPAMP frequency the gain reduces to 1. The mid band voltage gain is 100, 000 and cut off frequency is 10Hz.

    Fig. 6

    17. Slew Rate:

    Slew rate is defined as the maximum rate of change of output voltage per unit of time under large signal conditions and is expressed in volts / m secs.

    To understand this, consider a charging current of a capacitor shown in fig. 7.

  • Fig. 6

    If 'i' is more, capacitor charges quickly. If 'i' is limited to Imax, then rate of change is also limited.

    Slew rate indicates how rapidly the output of an OPAMP can change in response to changes in the input frequency with input amplitude constant. The slew rate changes with change in voltage gain and is normally specified at unity gain.

    If the slope requirement is greater than the slew rate, then distortion occurs. For the 741C the slew rate is low 0.5 V / m S. which limits its use in higher frequency applications.

    18. Input Offset Voltage and Current Drift:

    It is also called average temperature coefficient of input offset voltage or input offset current. The input offset voltage drift is the ratio of the change in input offset voltage to change in temperature and expressed in m V / C. Input offset voltage drift = ( D Vio / D T).

    Similarly, input offset current drift is the ratio of the change in input offset current to the change in temperature. Input offset current drift = ( D Iio / D T).

    For 741C,

    D Vio / D T = 0.5 m V / C. D Iio/ D T = 12 pA / C.

    Example - 1

    A 100 PF capacitor has a maximum charging current of 150 A. What is the slew rate?

    Solution:

    C = 100 PF=100 x 10-12 F I = 150 A = 150 x 10-6 A

  • Slew rate is 1.5 V / s.

    Example - 2

    An operational amplifier has a slew rate of 2 V / s. If the peak output is 12 V, what is the power bandwidth?

    Solution:

    The slew rate of an operational amplifier is

    As for output free of distribution, the slews determines the maximum frequency of operation fmax for a desired output swing.

    so So bandwidth = 26.5 kHz.

    Example - 3

    For the given circuit in fig. 1. Iin(off) = 20 nA. If Vin(off) = 0, what is the differential input voltage?. If A = 105, what does the output offset voltage equal?

  • Fig. 1

    Solutin:

    Iin(off) = 20 nA Vin(off) = 0

    (i) The differential input voltage = Iin(off) x 1k = 20 nA x 1 k = 20 V

    (ii) If A = 105 then the output offset voltage Vin(off) = 20 V x 105 = 2 volt

    Output offset voltage = 2 volts.

    Example - 4

    R1 = 100, Rf = 8.2 k, RC = 10 k. Assume that the amplifier is nulled at 25C. If Vin is 20 mV peak sine wave at 100 Hz. Calculate Er, and Vo values at 45C for the circuit shown in fig. 2.

    Fig. 2

    Solution:

    The change in temperature T = 45 - 25 = 20C.

  • Error voltage = 51.44 mV

    Output voltage is 1640 mV peak ac signal which rides either on a +51.44 mV or -51.44 mV dc level.

    Example - 5

    Design an input offset voltage compensating network for the operational amplifier A 715 for the circuit shown in fig. 3. Draw the complete circuit diagram.

    Fig. 3

    Solution:

    From data sheet we get vin = 5 mV for the operational amplifier A 715.

    V = | VCC | = | - VEE | = 15 V

  • Now,

    If we select RC = 10, the value of Rb should be Rb = (3000) RC = 30000 = 304

    Since R > Rmax, let RS = 10 Rmax where Rmax = Ra / 4. Therefore,

    If a 124 potentiometer is not available, we may prefer to use to the next lower value avilable, such as 104, so that the value of Ra will be larger than Rb by a factor of 10. If we select a 10 k potentiometer a s the Ra value, Rb is 12 times larger than Ra, Thus

    Ra = 10 k potentiometer Rb = 30 k Rc = 10.

    The final circuit, which also includes the pin connections for the A 715, shown in fig. 4.

    Fig. 4

    The ideal OPAMP :

  • An ideal OPAMP would exhibit the following electrical characteristic.

    1. Infinite voltage gain Ad 2. Infinite input resistance Ri, so that almost any signal source can drive it and there

    is no loading of the input source. 3. Zero output resistance RO, so that output can drive an infinite number of other

    devices. 4. Zero output voltage when input voltage is zero. 5. Infinite bandwidth so that any frequency signal from 0 to infinite Hz can be

    amplified without attenuation. 6. Infinite common mode rejection ratio so that the output common mode noise

    voltage is zero. 7. Infinite slew rate, so that output voltage changes occur simultaneously with input

    voltage changes.

    There are practical OPAMPs that can be made to approximate some of these characters using a negative feedback arrangement.

    Equivalent Circuit of an OPAMP:

    Fig. 5, shows an equivalent circuit of an OPAMP. v1 and v2are the two input voltage voltages. Ri is the input impedance of OPAMP. Ad Vd is an equivalent Thevenin voltage source and RO is the Thevenin equivalent impedance looking back into the terminal of an OPAMP.

    Fig. 5

    This equivalent circuit is useful in analyzing the basic operating principles of OPAMP and in observing the effects of standard feedback arrangements

    vO = Ad (v1 v2) = Ad vd.

  • This equation indicates that the output voltage vO is directly proportional to the algebraic difference between the two input voltages. In other words the OPAMP amplifies the difference between the two input voltages. It does not amplify the input voltages themselves. The polarity of the output voltage depends on the polarity of the difference voltage vd.

    Ideal Voltage Transfer Curve:

    The graphic representation of the output equation is shown in fig. 6 in which the output voltage vO is plotted against differential input voltage vd, keeping gain Ad constant.

    Fig. 6

    The output voltage cannot exceed the positive and negative saturation voltages. These saturation voltages are specified for given values of supply voltages. This means that the output voltage is directly proportional to the input difference voltage only until it reaches the saturation voltages and thereafter the output voltage remains constant.

    Thus curve is called an ideal voltage transfer curve, ideal because output offset voltage is assumed to be zero. If the curve is drawn to scale, the curve would be almost vertical because of very large values of Ad.

    Open loop OPAMP Configuration:

    In the case of amplifiers the term open loop indicates that no connection, exists between input and output terminals of any type. That is, the output signal is not fedback in any form as part of the input signal.

    In open loop configuration, The OPAMP functions as a high gain amplifier. There are three open loop OPAMP configurations.

    The Differential Amplifier:

    Fig. 1, shows the open loop differential amplifier in which input signals vin1 and vin2 are applied to the positive and negative input terminals.

  • Fig. 1

    Since the OPAMP amplifies the difference the between the two input signals, this configuration is called the differential amplifier. The OPAMP amplifies both ac and dc input signals. The source resistance Rin1 and Rin2 are normally negligible compared to the input resistance Ri. Therefore voltage drop across these resistances can be assumed to be zero.

    Therefore

    v1 = vin1 and v2 = vin2.

    vo = Ad (vin1 vin2 )

    where, Ad is the open loop gain.

    The Inverting Amplifier:

    If the input is applied to only inverting terminal and non-inverting terminal is grounded then it is called inverting amplifier.This configuration is shown in fig. 2.

    v1= 0, v2 = vin.

    vo = -Ad vin

  • Fig. 2

    The negative sign indicates that the output voltage is out of phase with respect to input 180 or is of opposite polarity. Thus the input signal is amplified and inverted also.

    The non-inverting amplifier:

    In this configuration, the input voltage is applied to non-inverting terminals and inverting terminal is ground as shown in fig. 3.

    v1 = +vin v2 = 0

    vo = +Ad vin

    This means that the input voltage is amplified by Ad and there is no phase reversal at the output.

    Fig. 3

    In all there configurations any input signal slightly greater than zero drive the output to saturation level. This is because of very high gain. Thus when operated in open-loop, the output of the OPAMP is either negative or positive saturation or switches between positive and negative saturation levels. Therefore open loop op-amp is not used in linear applications.

  • Closed Loop Amplifier:

    The gain of the OPAMP can be controlled if fedback is introduced in the circuit. That is, an output signal is fedback to the input either directly or via another network. If the signal fedback is of opposite or out phase by 180 with respect to the input signal, the feedback is called negative fedback.

    An amplifier with negative fedback has a self-correcting ability of change in output voltage caused by changes in environmental conditions. It is also known as degenerative fedback because it reduces the output voltage and,in tern,reduces the voltage gain.

    If the signal is fedback in phase with the input signal, the feedback is called positive feedback. In positive feedback the feedback signal aids the input signal. It is also known as regenerative feedback. Positive feedback is necessary in oscillator circuits.

    The negative fedback stabilizes the gain, increases the bandwidth and changes, the input and output resistances. Other benefits are reduced distortion and reduced offset output voltage. It also reduces the effect of temperature and supply voltage variation on the output of an op-amp.

    A closed loop amplifier can be represented by two blocks one for an OPAMP and other for a feedback circuits. There are four following ways to connect these blocks. These connections are shown in fig. 4.

    These connections are classified according to whether the voltage or current is feedback to the input in series or in parallel:

    Voltage series feedback Voltage shunt feedback Current series feedback Current shunt feedback

  • Fig. 4

    In all these circuits of fig. 4, the signal direction is from input to output for OPAMP and output to input for feedback circuit. Only first two, feedback in circuits are important.

    Voltage series feedback:

    It is also called non-inverting voltage feedback circuit. With this type of feedback, the input signal drives the non-inverting input of an amplifier; a fraction of the output voltage is then fed back to the inverting input. The op-amp is represented by its symbol including its large signal voltage gain Ad or A, and the feedback circuit is composed of two resistors R1 and Rf. as shown in fig. 5

  • Fig. 5

    The feedback voltage always opposes the input voltage, (or is out of phase by 180 with respect to input voltage), hence the feedback is said to be negative.

    The closed loop voltage gain is given by

    The product A and B is called loop gain. The gain loop gain is very large such that AB >> 1

  • This shows that overall voltage gain of the circuit equals the reciprocal of B, the feedback gain. It means that closed loop gain is no longer dependent on the gain of the op-amp, but depends on the feedback of the voltage divider. The feedback gain B can be precisely controlled and it is independent of the amplifier.

    Physically, what is happening in the circuit? The gain is approximately constant, even though differential voltage gain may change. Suppose A increases for some reasons (temperature change). Then the output voltage will try to increase. This means that more voltage is fedback to the inverting input, causing vd voltage to decrease. This almost completely offset the attempted increases in output voltage.

    Similarly, if A decreases, The output voltage decreases. It reduces the feedback voltage vf and hence, vd voltage increases. Thus the output voltage increases almost to same level.

    Different Input voltage is ideally zero.

    Again considering the voltage equation,

    vO = Ad vd

    or vd = vO / Ad

    Since Ad is very large (ideally infinite)

    \ vd 0.

    and v1 = v2 (ideal).

    This says, that the voltage at non-inverting input terminal of an op-amp is approximately equal to that at the inverting input terminal provided that Ad is very large. This concept is useful in the analysis of closed loop OPAMP circuits. For example, ideal closed loop voltage again can be obtained using the results

  • Input Resistance with Feedback:

    fig. 1, shows a voltage series feedback with the OPAMP equivalent circuit.

    Fig. 1 In this circuit Ri is the input resistance (open loop) of the OPAMP and Rif is the input resistance of the feedback amplifier. The input resistance with feedback is defined as

  • Since AB is much larger than 1, which means that Rif is much larger that Ri. Thus Rif approaches infinity and therefore, this amplifier approximates an ideal voltage amplifier.

    Output Resistance with Feedback:

    Output resistance is the resistance determined looking back into the feedback amplifier from the output terminal. To find output resistance with feedback Rf, input vin is reduced to zero, an external voltage Vo is applied as shown in fig. 2.

    Fig. 2

    The output resistance (Rof ) is defined as

  • This shows that the output resistance of the voltage series feedback amplifier is ( 1 / 1+AB ) times the output resistance Ro of the op-amp. It is very small because (1+AB) is very large. It approaches to zero for an ideal voltage amplifier.

    Reduced Non-linear Distortion:

    The final stage of an OPAMP has non-linear distortion when the signal swings over most of the ac load line. Large swings in current cause the r'e of a transistor to change during the cycle. In other words, the open loop gain varies throughout the cycle of when a large signal is being applied. It is this changing voltage gain that is a source of the non-linear distortion.

    Noninverting voltage feedback reduces non-linear distortion because the feedback stabilizes the closed loop voltage gain, making it almost independent of the changes in open loop voltage gain. As long as loop gain, is much greater than 1, the output voltage equals 1/B times the input voltage. This implies that output will be a more faithful reproduction of the input .

    Consider, under large signal conditions, the open loop OPAMP circuit produces a distortion voltage, designated vdist. It can be represented by connecting a source vdist in series with Avd. Without negative feedback all the distortion voltage vdist appears at the output. But with negative feedback, a fraction of vdist is feedback to inverting input. This is amplified and arrives at the output with inverted phase almost completely canceling the original distortion produced by the output stage.

  • The first term is the amplified output voltage. The second term in the distortion that appears at the final output. The distortion voltage is very much, reduced because AB>>1

    Bandwidth with Feedback:

    The bandwidth of an amplifier is defined as the band of frequencies for which the gain remains constant. Fig. 3, shows the open loop gain vs frequency curve of 741C OPAMP. From this curve for a gain of 2 x 105 the bandwidth is approximately 5Hz. On the other hand, the bandwidth is approximately 1MHz when the gain is unity.

    Fig. 3

    The frequency at which gain equals 1 is known as the unity gain bandwidth. It is the maximum frequency the OPAMP can be used for. Furthermore, the gain bandwidth product obtained from the open loop gain vs frequency curve is equal to the unity gain bandwidth of the OPAMP. Since the gain bandwidth product is constant obviously the higher the gain the smaller the bandwidth and vice versa. If negative feedback is used gain decrease from A to A / (1+AB). Therefore the closed loop bandwidth increases by (1+AB).

    Bandwidth with feedback = (1+ A B) x (B.W. without feedback)

    ff= fo (1+A B)

    Output Offset Voltage:

  • In an OPAMP even if the input voltage is zero an output voltage can exist. There are three cause of this unwanted offset voltage.

    1. Input offset voltage. 2. Input bias voltage. 3. Input offset current.

    Fig. 4, shows a feedback amplifier with an output offset voltage source in series with the open loop output AVd. The actual output offset voltage with negative feedback is smaller. The reasoning is similar to that given for distortion. Some of the output offset voltage is fed back to the inverting input. After amplification an out of phase voltage arrives at the output canceling most of the original output offset voltage.

    When loop gain AB is much greater than 1, the closed loop output offset voltage is much smaller than the open loop output offset voltage.

    Fig. 4

    Voltage Follower:

    The lowest gain that can be obtained from a non-inverting amplifier with feedback is 1. When the non-inverting amplifier gives unity gain, it is called voltage follower because the output voltage is equal to the input voltage and in phase with the input voltage. In other words the output voltage follows the input voltage.

    To obtain voltage follower, R1 is open circuited and Rf is shorted in a negative feedback amplifier of fig. 4. The resultant circuit is shown in fig. 5.

  • vout = Avd= A (v1 v2)

    v1 = vin

    v2 =vout

    v1 = v2 if A >> 1

    vout = vin.

    The gain of the feedback circuit (B) is 1. Therefore

    Af = 1 / B = 1

    Fig. 5

    Voltage shunt Feedback:

    Fig. 1, shows the voltage shunt feedback amplifier using OPAMP.

    Fig. 1

    The input voltage drives the inverting terminal, and the amplified as well as inverted output signal is also applied to the inverting input via the feedback resistor Rf. This arrangement forms a negative feedback because any increase in the output signal results in a feedback signal into the inverting input signal causing a decrease in the output signal. The non-inverting terminal is grounded. Resistor R1 is connected in series with the source.

    The closed loop voltage gain can be obtained by, writing Kirchoff's current equation at the input node V2.

  • The negative sign in equation indicates that the input and output signals are out of phase by 180. Therefore it is called inverting amplifier. The gain can be selected by selecting Rf and R1 (even < 1).

    Inverting Input at Virtual Ground:

    In the fig. 1, shown earlier, the noninverting terminal is grounded and the- input signal is applied to the inverting terminal via resistor R1. The difference input voltage vd is ideally zero, (vd= vO/ A) is the voltage at the inverting terminals (v2) is approximately equal to that of the noninverting terminal (v1). In other words, the inverting terminal voltage (v1) is approximately at ground potential. Therefore, it is said to be at virtual ground.

    Input Resistance with Feedback:

  • To find the input resistance Miller equivalent of the feedback resistor Rf, is obtained, i.e. Rf is splitted into its two Miller components as shown in fig. 2. Therefore, input resistance with feedback Rif is then

    Fig. 2

    Output Resistance with Feedback:

    The output resistance with feedback Rof is the resistance measured at the output terminal of the feedback amplifier. The output resistance can be obtained using Thevenin's equivalent circuit,shown in fig. 3.

    iO = ia + ib

    Since RO is very small as compared to Rf +(R1 || R2 )

    Therefore,i.e. iO= ia

    vO = RO iO + A vd.

    vd= vi v2 = 0 - B vO

    Fig. 3

  • Similarly, the bandwidth increases by (1+ AB) and total output offset voltage reduces by (1+AB).

    Example - 1

    (a).An inverting amplifier is implemented with R1 = 1K and Rf = 100 K. Find the percentge change in the closed loop gain A is the open loop gain a changes from 2 x 105 V / V to 5 x 104 V/V. (b) Repeat, but for a non-inverting amplifier with R1 = 1K at Rf = 99 K.

    Solution: (a). Inverting amplifier

    Here Rf = 100 K R1 = 1K

    When,

    (b) Non-inverting amplifier

    Here Rf = 99 K R1 = 1K

  • Example - 2

    An inverting amplifier shown in fig. 4 with R1 = 10 and R2 = 1M is driven by a source v1 = 0.1 V. Find the closed loop gain A, the percentage division of A from the ideal value - R2 / R1, and the inverting input voltage VN for the cases A = 100 V/V, 105 and 105 V/V.

    Solution:

    we have when A = 103,

    Fig. 4

  • Example - 3

    Find VN, V1 and VO for the circuit shown in fig. 5.

    Solution:

    Applying KCL at N

    or 2VN + VN = VO.

    Now VO - Vi = 6 as point A and N are virtually shorted. VO - VN = 6 V Therefore, VO = VN + 6 V

    Therefore, VN = Vi = 3 V.

    Fig. 5

    OSCILLATOR

    Oscillators:

    An oscillator may be described as a source of alternating voltage. It is different than amplifier.

  • An amplifier delivers an output signal whose waveform corresponds to the input signal but whose power level is higher. The additional power content in the output signal is supplied by the DC power source used to bias the active device.

    The amplifier can therefore be described as an energy converter, it accepts energy from the DC power supply and converts it to energy at the signal frequency. The process of energy conversion is controlled by the input signal, Thus if there is no input signal, no energy conversion takes place and there is no output signal.

    The oscillator, on the other hand, requires no external signal to initiate or maintain the energy conversion process. Instead an output signals is produced as long as source of DC power is connected. Fig. 1, shows the block diagram of an amplifier and an oscillator.

    Fig. 1

    Oscillators may be classified in terms of their output waveform, frequency range, components, or circuit configuration.

    If the output waveform is sinusoidal, it is called harmonic oscillator otherwise it is called relaxation oscillator, which include square, triangular and saw tooth waveforms.

    Oscillators employ both active and passive components. The active components provide energy conversion mechanism. Typical active devices are transistor, FET etc.

    Passive components normally determine the frequency of oscillation. They also influence stability, which is a measure of the change in output frequency (drift) with time, temperature or other factors. Passive devices may include resistors, inductors, capacitors, transformers, and resonant crystals.

    Capacitors used in oscillators circuits should be of high quality. Because of low losses and excellent stability, silver mica or ceramic capacitors are generally preferred.

    An elementary sinusoidal oscillator is shown in fig. 2. The inductor and capacitors are reactive elements i.e. they are capable of storing energy. The capacitor stores energy in its electric field.Whenever there is voltage across its plates,and the inductor stores energy in its magnetic field whenever current flows through it. Both C and L are assumed to be loss less. Energy can be introduced into the circuit by charging the capacitor with a voltage V as shown in fig. 2. As long as the switch S is open, C cannot discharge and so i=0 and V=0.

  • Fig. 2

    Now S is closed at t = to, This means V rises from 0 to V, Just before closing inductor current was zero and inductor current cannot be changed instantaneously. Current increases from zero value sinusoidally and is given by

    The capacitor losses its charge and energy is simply transferred from capacitor to inductor magnetic field. The total energy is still same. At t = t1, all the charge has been removed from the capacitor plates and voltage reduces to zero and at current reaches to its maximum value. The current for t> t1 charges C in the opposite direction and current decreases. Thus LC oscillation takes places. Both voltage and current are sinusoidal though no sinusoidal input was applied. The

    frequency of oscillation is

    The circuit discussed is not a practical oscillator because even if loss less components were available, one could not extract energy with out introducing an equivalent resistance. This would result in damped oscillations as shown in fig. 3.

    Fig. 3

  • These oscillations decay to zero as soon as the energy in the tank is consumed. If we remove too much power from the circuit, the energy may be completely consumed before the first cycle of oscillations can take place yielding the over damped response.

    It is possible to supply energy to the tank to make up for all losses (coil losses plus energy removed), thereby maintaining oscillations of constant amplitude.

    Since energy lost may be related to a positive resistance, it follows that the circuit would gain energy if an equivalent negative resistance were available. The negative resistance, supplies whatever energy the circuit lose due to positive resistance. Certain devices exhibit negative resistance characteristics, an increasing current for a decreasing voltage. The energy supplied by the negative resistance to the circuit, actually comes from DC source that is necessary to bias the device in its negative resistance region.

    Another technique for producing oscillation is to use positive feedback considers an amplifier with an input signal vin and output vO as shown in fig. 4.

    Fig. 4

    The amplifier is inverting amplifier and may be transistorized, or FET or OPAMP. The output is 180 out of phase with input signal vO= -A vin.(A is negative)

    Now a feedback circuit is added. The output voltage is fed to the feed back circuit. The output of the feedback circuit is again 180 phase shifted and also gets attenuated. Thus the output from the feedback network is in phase with input signal vin and it can also be made equal to input signal.

    If this is so, Vf can be connected directly and externally applied signal can be removed and the circuit will continue to generate an output signal. The amplifier still has an input but the input is derived from the output amplifier. The output essentially feeds on itself and is continuously regenerated. This is positive feedback. The over all amplification from vin to vf is 1 and the total phase shift is zero. Thus the loop gain A is equal to unity.

    When this criterion is satisfied then the closed loop gain is infinite. i.e. an output is produced without any external input.

  • vO = A verror

    = A (v in + v f )

    = A (vin + vO)

    or (1-A )vO = A vin

    or

    When A = 1, vO / vin=

    The criterion A = 1 is satisfied only at one frequency.This is known as backhausen criterion.

    The frequency at which a sinusoidal oscillator will operate is the frequency for which the total phase shift introduced, as the signal proceeds form the input terminals, through the amplifier and feed back network and back again to the input is precisely zero or an integral multiple of 2p. Thus the frequency of oscillation is determined by the condition that the loop phase shift is zero.

    Oscillation will not be sustained, if at the oscillator frequency, A 1. Fig. 5, show the output for two different contions A < 1 and A >1.

    Fig. 5

    If A is less than unity then A vin is less than vin, and the output signal will die out, when the externally applied source is removed. If A>1 then A b vinis greater than vin and the output

  • voltage builds up gradually. If A = 1, only then output voltage is sine wave under steady state conditions.

    In a practical oscillator, it is not necessary to supply a signal to start the oscillations. Instead, oscillations are self-starting and begin as soon as power is applied. This is possible because of electrical noise present in all passive components.

    Therefore, as soon as the power is applied, there is already some energy in the circuit at fo, the frequency for which the circuit is designed to oscillate. This energy is very small and is mixed with all the other frequency components also present, but it is there. Only at this frequency the loop gain is slightly greater than unity and the loop phase shift is zero. At all other frequency the Barkhausen criterion is not satisfied. The magnitude of the frequency component fo is made slightly higher each time it goes around the loop. Soon the fo component is much larger than all other components and ultimately its amplitude is limited by the circuits own non-lineareties (reduction of gain at high current levels, saturation or cut off). Thus the loop gain reduces to unity and steady stage is reached. If it does not, then the clipping may occur.

    Practically, A is made slightly greater than unity. So that due to disturbance the output does not change but if A = 1 and due to some reasons if A decreases slightly than the oscillation may die out and oscillator stop functioning. In conclusion, all practical oscillations involve:

    An active device to supply loop gain or negative resistance. A frequency selective network to determine the frequency of oscillation. Some type of non-linearity to limit amplitude of oscillations.

    Example - 1

    The gain of certain amplifier as a function of frequency is A (j) = -16 x 106 / j. A feedback path connected around it has (j ) = 103 / (20 x 103 + j )2. Will the system oscillate? If so, at what frequency ?

    Solution:

    The loop gain is

    To determine, if the system will oscillate, we will first determine the frequency, if any, at which the phase angle of equals to 0 or a multiple of 360. Using phasor algebra, we have

  • This expression will equal -360 if ,

    Thus, the phase shift around the loop is -360 at = 2000 rad/s. We must now check to see if the gain magnitude |A | = 1 at = 2 x 103. The gain magnitude is

    Substituting = 2 x 103, we find

    Thus, the Barkhausen criterion is satisfied at = 2 x 103 rad/s and oscillation occurs at that frequency (2 x 103 / 2 = 318 .3 Hz).

    Transistor Phase Shift Oscillator:

    At low frequencies (around 100 kHz or less), resistors and capacitors are usually employed to determine the frequency of oscillation. Fig. 1 shows transistorized phase shift oscillator circuit employing RC network. If the phase shift through the common emitter amplifier is 180, then the oscillation may occur at the frequency where the RC network produces an additional 180 phase shift.

    Since a transistor is used as the active element, the output across R of the feedback network is shunted by the relatively low input resistance of the transistor, because input diode is a forward biased diode

  • Fig. 1

    Hence, instead of employing voltage series feedback, voltage shunt feedback is used for a transistor phase shift oscillator. The load resistance RL is also connected via coupling capacitor. The equivalent circuit using h-parameter is shown in fig. 2.

    Fig. 2

    For the circuit, the load resistance RL may be lumped with RC and the effective load resistance becomes R'L(= RC || RL). The two h-parameters of the CE transistor amplifier, hoe and hre are neglected.

    The capacitor C offers some impedance at the frequency of oscillation and, therefore, it is kept as it is, while the coupling capacitor behaves like ac short. The input resistance of the transistor is Rihie. Therefore the resistance R3 is selected such that R=R3+Ri=R3+hie. This choice makes the three R C selections alike and simplifies the calculation. The effect of biasing resistor R1 , R2, & REon the circuit operation is neglected.

    Since this is a voltage shunt feedback, therefore instead of finding VR /VO, we should find the current gain of the feedback loop.

  • The simplified equivalent circuit is shown in fig. 3.

    Fig. 3

    Applying KVL,

    Since I3 and Ib must be in phase to satisfy Barkhausen criterion, therefore

  • Also initially I3 > Ib, therefore, for oscillation to start,

    Therefore, the two conditions must be satisfied for oscillation to start and sustain.

    Exampl - 1

    (a). Show that the OPAMP phase shifter shown in fig. 4

    .

    (b) Cascade two identical phase shifters of the type sown in fig. 4. Complete the loop with an inverting amplifier. Show that the system will oscillate at the frequency f = 1 / 2RC provided that the amplifier gain exceeds unity.

    (c) Show that the circuit produces two quadrature sinusoids (sine wave differing in phase by 90).

  • Fig. 4

    Solution:

    (a)The voltage the non-inverting terminal input of the OPAM is given by

    Since the differential input voltage of OPAMP is negligible small, therefore, the voltage at the inverting terminal is also given by

    The input impedance of the OPAMP is very large, therefore,

    or Vi - 2V2 = -VO

    Substituting v2 in above equation, we get,

    Substituting XC, we get

  • Therefore,

    and the phase angle between VO and Vi is given by

    The magnitude of VO / Vi is unity for all frequencies and the phase shift provided by this circuit is 0 for R = 0 and 180 for R > infinity.

    (b). If two such phase shifters are connected in cascade and an inverting amplifier with gain is connected in the feedback loop, then the net loop gain becomes

    Loop gain = Gain of phase shifter 1 x Gain of phase shifter 2 x = 1 x 1x =

    Therefore, the oscillation takes place if gain =1, but it is kept >1 so that the losses taking place in the amplifier can be compensated.

    The total phase shift around the loop is given by

    total phase shift = -2 tan-1 (RC) - 2 tan-1(RC) + 180

    Further, for oscillation to take place the net phase shift around the loop would be 0.Therefore,

    -2 tan-1 (RC) - 2 tan-1(RC) + 180 =0 or RC = 1 or f = 1 / 2R C

    (c). The phase shift provided by amplifier in the feedback path is 180, therefore, the phase shift provided by the phase shifters should also be 180 to have 360 or 0 phase shift. Thus ,the phase shift provided by the individual shifter will be 90 as both are identical. Therefore, the sine wave produces by two phase shifters are 90 apart and the circuit produces two quadrature sinusoids.

  • Wien Bridge Oscillator:

    The Wien Bridge oscillator is a standard oscillator circuit for low to moderate frequencies, in the range 5Hz to about 1MHz. It is mainly used in audio frequency generators.

    The Wien Bridge oscillator uses a feedback circuit called a lead lag network as shown in fig. 1.

    At very low frequencies, the series capacitor looks open to the input signal and there is no output signal. At very high frequencies the shunt capacitor looks shorted, and there is no output. In between these extremes, the output voltage reaches a maximum value. The frequency at which the output is maximized is called the resonant frequency. At this frequency, the feedback fraction reaches a maximum value of 1/3.

    At very low frequencies, the phase angle is positive, and the circuit acts like a lead network. On the other hand, at very high frequencies, the phase angle is negative, and the circuit acts like a lag network. In between, there is a resonant frequency fr at which the phase angle equals 0.

    The output of the lag lead network is

    Fig. 1

  • The gain of the feedback circuit is given by

    The phase angle between Vout and Vinis given by

    These equations shows that maximum value of gain occurs at XC = R, and phase angle also becomes 0. This represents the resonant frequency of load lag network. Fig. 2, shows the gain and phase vs frequency.

  • Fig. 2

    How Wien Bridge Oscillator Works:

    Fig. 3, shows a Wien Bridge oscillator. The operational amplifier is used in a non-inverting configuration, and the lead-lag network provides the feedback. Resistors Rf and R1 determine the amplifier gain and are selected to make the loop gain equal to 1. If the feedback circuit parameters are chosen properly, there will be some frequency at which there is zero phase shift in the signal fed back to non inverting terminal. Because the amplifier is non inverting, it also contributes zero phase shift, so the total phase shift around the loop is 0 at that frequency, as required for oscillation.

    The oscillator uses positive and negative feedback. The positive feedback helps the oscillations to build up when the power is turn on. After the output signal reaches the desired level the negative feedback reduces the loop gain is 1. The positive feedback is through the lead lag network to the non-inverting input. Negative feedback is through the voltage divider to the inverting input.

  • Fig. 3

    At power up, the tungsten lamp has a low resistance, and therefore, negative feedback is less. For this, reason, the loop gain AB is greater than 1, and oscillations can build up at the resonant frequency fr. As the oscillations build up, the tungsten lamp heats up slightly and its resistance increases. At the desired output level the tungsten lamp has a resistance R'. At this point

    Since the lead lag network has a gain (=B) of 1/3, the loop gain AB equals unity and than the output amplitude levels off and becomes constant. The frequency of oscillation can be adjusted by selecting R and C as

    The amplifier must have a closed loop cut off frequency well above the resonant frequency, fr.

  • Fig. 4

    Fig. 4, shows another way to represent Wein Bridge oscillator. The lead lag network is the left side of the bridge and the voltage divider is the right side. This ac bridge is called a Wein Bridge. The error voltage is the output of the Wein Bridge. When the bridge approaches balance, the error voltage approaches zero.

    Example -1:

    Design a Wien-bridge oscillator that oscillates at 25 kHz.

    Solution:

    Let C1 = C2 = 0.001 F. Then, the frequency of oscillation is given by,

    or,

    Let R1 = 10 K. Then,

    or, Rf = 20K

    Tuned Oscillator:

  • A variety of oscillator circuits can be built using LC tuned circuits. A general form of tuned oscillator circuit is shown in fig. 1. It is assumed that the active device used in the oscillator has very high input resistance such as FET, or an operational amplifier.

    Fig. 1 Fig. 2

    Fig. 2 shows linear equivalent circuit of fig. 1 using an amplifier with an open circuit gain Av and output resistance RO. It is clear from the topology of the circuit that it is voltage series feedback type circuit.

    The loop gain of the circuit A can be obtained by considering the circuit to be a feedback amplifier with output taken from terminals 2 and 3 and with input terminals 1 and 3. The load impedance ZL consists of Z2 in parallel with the series combination of Z1 and Z3. The gain of the the amplifier without feedback will be given by

    The feedback circuit gain is given by

    Therefore, the loop gain is given by

  • If the impedances are pure reactances (either inductive or capacitive), then Z1 = jX1, Z2= jX2 and Z3= jX3. Then

    For the loop gain to be real (zero phase shift around the loop),

    X1 + X2 + X3 = 0

    and

    Therefore, the circuit will oscillate at the resonant frequency of the series combination of X1, X2 and X3. Since A must be positive and at leat unity in magnitude, then X1 and X2 must have the same sign (Av is positive).In other words, they must be the same kind of reactance, either both inductive or both capacitive.

    The Colpitts Oscillator:

    Wein bridge oscillator is not suited to high frequencies (above 1MHz). The main problem is the phase shift through the amplifier.

    The alternative is an LC oscillator, a circuit that can be used for frequencies between 1MHz and 500MHz. The frequency range is beyond the frequency limit of most OPAMPs. With an amplifier and LC tank circuit, we can feedback a signal with the right amplitude and phase is feedback to sustain oscillations. Fig. 3, shows the circuit of colpitts oscillator.

  • Fig. 3 Fig. 4

    The voltage divider bias sets up a quiescent operating point. The circuit then has a low frequency voltage gain of rc / r'e where rc is the ac resistance seen by the selector. Because of the base and collector lag networks, the high frequency voltage gain is less then rc / r'e.

    Fig. 4, shows a simplified ac equivalent circuit. The circulating or loop current in the tank flows through C1 in series with C2. The voltage output equals the voltage across C1. The feedback voltage vf appears across C2. This feedback voltage drives the base and sustains the oscillations developed across the tank circuit provided there is enough voltage gain at the oscillation frequency. Since the emitter is at ac ground the circuit is a CE connection.

    Most LC oscillators use tank circuit with a Q greater than 10. The Q of the feedback circuit is given by

    Because of this, the approximate resonant frequency is

    This is accurate and better than 1% when Q is greater than 1%. The capacitance C is the equivalent capacitance the circulation current passes through. In the Colpitts tank the circulating current flows through C1 in series with C2.

    Therefore C = C1 C2 / (C1 +C2)

  • The required starting condition for any oscillator is A > 1 at the resonant frequency or A > 1/ . The voltage gain A in the expression is the gain at the oscillation frequency. The feedback gain is given by

    = vf / vout XC1 / XC2

    Because same current flow through C1 and C2, therefore

    = C1/ C2; A > 1/ v; A> C1 / C2

    This is a crude approximation because it ignores the impedance looking into the base. An exact analysis would take the base impedance into account because it is in parallel with C2 .

    With small , the value of A is only slightly larger than 1/. and the operation is approximately close A. When the power is switched on, the oscillations build up, and the signal swings over more and more of ac load line. With this increased signal swing, the operation changes from small signal to large signal. As this happen, the voltage gain decreases slightly. With light feedback the value of A can decreases to 1 without excessive clapping.

    With heavy feedback, the large feedback signal drives the base into saturation and cut off. This charges capacitor C3 producing negative dc clamping at the base and changing the operation from class A to class C. The negative damping automatically adjusts the value of A to 1.

    Example - 1

    Design a Colpitts oscillator that will oscillate at 100 kHz.

    Solution:

    Let us choose R1 = Rf = 5 k and C = 0.001 F. From the frequency expression,

    The quality factor (Q) of the LC circuit is given by:

    Hartley Oscillator:

    Fig. 5, shows Hartley oscillator when the LC tank is resonant, the circulating current flows through L1 in series with L2. Thus, the equivalent inductance is L = L1 + L2.

  • Fig. 5

    In the oscillator, the feedback voltage is developed by the inductive voltage divider, L1 & L2. Since the output voltage appears across L1 and the feedback voltage across L2, the feedback fraction is

    = V / Vout = XL2 / XL1 = L2 / L1

    As usual, the loading effect of the base is ignored. For oscillations to start, the voltage gain must be greater than 1/ . The frequency of oscillation is given by

    Similarly, an opamp based Hartley oscillator circuit is shown in fig. 6.

  • Fig. 6

    Crystal Oscillator:

    Some crystals found in nature exhibit the piezoelectric effect i.e. when an ac voltage is applied across them, they vibrate at the frequency of the applied voltage. Conversely, if they are mechanically pressed, they generate an ac voltage. The main substances that produce this piezoelectric effect are Quartz, Rochelle salts, and Tourmaline.

    Rochelle salts have greatest piezoelectric activity, for a given ac voltage, they vibrate more than quartz or tourmaline. Mechanically, they are the weakest they break easily. They are used in microphones, phonograph pickups, headsets and loudspeakers.

    Tourmaline shows the least piezoelectric activity but is a strongest of the three. It is also the most expensive and used at very high frequencies.

    Quartz is a compromise between the piezoelectric activity of Rochelle salts and the strength of tourmaline. It is inexpensive and easily available in nature. It is most widely used for RF oscillators and filters.

    The natural shape of a quartz crystal is a hexagonal prism with pyramids at the ends. To get a useable crystal out of this it is sliced in a rectangular slap form of thickness t. The number of slabs we can get from a natural crystal depends on the size of the slabs and the angle of cut.

    Fig. 1

    For use in electronic circuits, the slab is mounted between two metal plates, as shown in fig. 1. In this circuit the amount of crystal vibration depends upon the frequency of applied voltage. By changing the frequency, one can find resonant frequencies at which the crystal vibrations reach a maximum. Since the energy for the vibrations must be supplied by the ac source, the ac current is maximized at each resonant frequency. Most of the time, the crystal is cut and mounted to vibrate best at one of its resonant frequencies, usually the fundamental or lowest frequency. Higher resonant frequencies, called overtones, are almost exact multiplies of the fundamental frequency e.g. a crystal with a fundamental frequency of 1 MHz has a overtones of 2 MHz, 3 MHz and so on. The formula for the fundamental frequency of a crystal is

  • f = K / t.

    where K is a constant that depends on the cut and other factors, t is the thickness of crystal, f is inversely proportional to thickness t. The thinner the crystal, the more fragile it becomes and the more likely it is to break because of vibrations. Quartz crystals may have fundamental frequency up to 10 MHz. To get higher frequencies, a crystal is mounted to vibrate on overtones; we can reach frequencies up to 100 MHz.

    AC Equivalent Circuit:

    When the mounted crystal is not vibrating, it is equivalent to a capacitance Cm, because it has two metal plates separated by dielectric, Cm is known as mounting capacitance.

    Fig. 2

    When the crystal is vibrating, it acts like a tuned circuit. Fig. 2, shows the ac equivalent circuit of a crystal vibrating at or near its fundamental frequency. Typical values are L is henrys, C in fractions of a Pico farad, R in hundreds of ohms and Cm in Pico farads

    Ls = 3Hz, Cs = 0.05 pf, Rs = 2K, Cm = 10 pf.

    The Q of the circuit is very very high. Compared with L-C tank circuit. For the given values, Q comes out to be 3000. Because of very high Q, a crystal leads to oscillators with very stable frequency values.

    The series resonant frequency fS of a crystal is the sonant frequency of the LCR branch. At this frequency, the branch current reaches a maximum value because Ls resonant with CS.

    Above fS, the crystal behaves inductively. The parallel resonant frequency is the frequency at which the circulating or loop current reaches a maximum value. Since this loop current must flow through the series combination of CS and Cm, the equivalent Cloop is

  • Since Cloop > CS, therefore, fp > fS.

    Since Cm > CS, therefore, Cm || CS is slightly lesser than CS. Therefore fP is slightly greater than fS. Because of the other circuit capacitances that appear across Cm the actual frequency will lie between fS and fP. fS and fP are the upper and lower limits of frequency. The impedance of the crystal oscillator can be plotted as a function of frequency as shown in fig. 3.

    At frequency fS, the circuit behaves like resistive circuit. At fP the impedance reaches to maximum, beyond fP, the circuit is highly capacitive.

    The frequency of an oscillator tends to change slightly with time. The drift is produced by temperature, aging and other causes. In a crystal oscillator the frequency drift with time is very small, typically less than 1 part in 106 per day. They can be used in electronic wristwatches. If the drift is 1 part in 1010, a clock with this drift will take 30 years to gain or lose 1 sec.

    Fig. 3

    Crystals can be manufactured with values of fs as low as 10 kHz; at these frequencies the crystal is relatively thick. On the high frequency side, fs can be as high as 1- MHz; here the crystal is very thin.

    The temperature coefficient of crystals is usually small and can be made zero. When extreme temperature stability is required, the crystal may be housed in an oven to maintain it at a constant temperature. The high Q of the crystal also contributes to the relatively drift free oscillation of crystal oscillators.

    Example - 1

    The parameters of the equivalent circuit of a crystal are given below:

    L = 0.4 H, CS = 0.06 pF, R = 5 k, Cm = 1.0 pF.

  • Determine the series and parallel resonant frequencies of the crystal.

    Solution:

    With reference to fig. 2, the admittance of the crystal Y is given by

    where,

    and

    The resonant frequencies are obtained by putting B = 0. Thus,

    Consider the term CS R2 / LS = CS R / [L R]. In a crystal, the time constant (L / R) is very much greater than CS R. Thus the ratio is very much less than 1. For the values given, this ratio is of the order of10-6. Neglecting this term in comparison with 2, we get two roots as

    where, s and p are the series and parallel resonant frequencies respectively. Substituting the values, we get

    s = 6.45 M Hz. and p = 6.64 MHz

    Crystal Oscillators:

    Fig. 4, shows a colpitts crystal oscillator.

  • Fi. 4

    The capacitive voltage divider produces the feedback voltage for the base of transistor. The crystal acts like an inductor that resonates with C1 and C2. The oscillation frequency is between the series and parallel resonant frequencies.

    Example-2:

    If the crystal of example-1 is used in the oscillator circuit as shown fig. 5, determine the values of R for the circuit to oscillate.

    Fig. 5

    Solution:

  • The equivalent circuit of crystal (discussed earlier) shows that it has a parallel resonant fr frequency (p) at which the impedance becomes maximum. The amplified signal output of the circuit is applied across the potential divider consisting of R and the crystal circuit. At the resonant frequency the impedance of crystal becomes maximum (magnitude R) and thus the loop gain will be greater than or equal to unity. At frequencies away from p the loop gain becomes less than unity. The loop base shift is also zero around p. Thus both the conditions required for sustained oscillations are satisfied and the circuit oscillates.

    The value of G of the crystal at =p is given by

    Thus the resistor R should be less than 5x106 .

    Differential Amplifier:

    The basic differential amplifier is shown in fig. 1.

    Fig. 1

    Since there are two inputs superposition theorem can be used to find the output voltage. When Vb= 0, then the circuit becomes inverting amplifier, hence the output due to Va only is

    Vo(a) = -(Rf / R1) Va

    Similarly when, Va = 0, the configuration is a inverting amplifier having a voltage divided network at the noninverting input

  • Example - 1

    Find vout and iout for the circuit shown in fig. 2. The input voltage is sinusoidal with amplitude of 0.5 V.

    Fig. 2

    Solution:

    We begin by writing the KCL equations at both the + and terminals of the op-amp.

    For t