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Transcript
Non-ideal behaviour of op-amps:
Input bias and offset current
 Op-amps sink or source a small current at each
input –these are the bias currents for the
transistors within the op-amp.
 Op-amps require a series dc path through
which currents can flow.
 The bias currents are never actually matched as
the two input stages of the op-amp are in general
mismatched.
So we model both input bias currents as follows:
In
Ideal Op-amp
Vn
IB
IOS /2
Ip
Vp
Define:
IB 
Vo
IB
I p  In
2
and I OS  I p  I n
IOS is the input offset current.
 Usually
IOS < 0.1 IB
 The polarity of IB is determined by the type of the
input transistor.
 For npn BJT and p-channel JFETs, the input
currents and hence IB are positive.
 For pnp BJT and n-channel JFETs, the input currents
and hence IB are negative
 The polarity of IOS is determined by the direction of the
mismatch.
IB and IOS produce errors
 Negative Feedback does not reduce these
We measure IB and IOS by seeing what is the output
for zero (signal) input
 Then, non-inverting and inverting amplifiers are
the same
R2
R1
Rp
In
Ip
Eo
0V
 R 
E o   1  2   R1 / / R2  I n  R p I p
R1 



 An (unwanted) input is amplified by a gain
“noise”
“noise gain”

 R 
Noise gain   1  2 
R1 

Same for both inverting and
non-inverting configurations!
 Obvious effect on signal to noise ratio at output!
(Remember superposition)
Effect on an Integrator (with zero I/P signal)
C
R
Rp
In
Ip
t
Rp 
1 
Eo    I n 
I p  dt  E o (0)
C 0
R

t
1
    I OS dt  E o (0) when R p  R
C0
Eo
How to reduce effects of IB and IOS?
 Choose devices with low IB and IOS
 Superbeta BJTs – Superbeta BJTs have very
thin base regions and hence the recombination
component of the base current is reduced.
 IB Cancellation methods – special circuitry is
used to provide the bias currents and thus cancel
the bias currents required from outside the
device.
FET input op-amps – have low bias currents
 Choose Rp = R1 // R2 , then

R 
E o   1  2     R1 / / R2  I OS 
R1 

Temperature effects on IB and IOS :
 For BJTs, the temperature effects are often
negligible for normal temp ranges
 For FET types, IB doubles every 10C
Op-amps with very low IB require guarding to
counteract PCB surface leakage currents.
CF
R2
2
R1
3
2
3
Vi
Vo
Rp
CF
R2
R1
2
3
Rp
Vi
Vo
Input Offset Voltage
When the inputs of the op-amp are shorted
together, we should get zero OutPut
We don’t ( due to mismatches / manufacturing
tolerances)
We model this with an input offset voltage (the
voltage shift required at the input to correct the
VTC)
Vo [V]
VSATH
Vd [V]
VOS
Voltage Transfer Char.
(VTC)
VSATL
Ideal Op-amp
Vn
Vd
VOS
Vp
Vo
Now require Vd  Vp  VOS  Vn  0  Vp  Vn  VOS
Errors due to VOS
(Inverting or non-inverting configurations.)
R2
R1
VOS

R 
E o  1  2 VOS
R1 

Eo
dc “noise” with noise gain
Error in Integrator circuit
C
R
VOS
t
1
Eo 
VOS dt  E o ( 0)

RC 0
Eo
Combination of Input offset voltage and input
bias currents
Example – inverting amplifier
Practical Op-amp
R2
In
Vn
Ideal Op-amp
R1
IB
Ip
Vp
vo
vi
IOS /2
Rp
Vo
IB
(a)
(b)
Fig Q6
Equivalent circuit:
R1//R2
In
R1
Eo
R1  R2
Rp
Ip
VOS
0V
Eo
V  V

R1
Eo  R1 //R2 I n   R p I p  VOS
R1  R2
 R 
 R 
 EO  1  2 VOS  R1 // R2 I n  R p I p   1  2 VOS  R p I OS 
 R1 
 R1 
since Rp = R1 //R2
Temperature effects
 Mismatch can get worse as T changes
VOS
(Average) temperature coefficient of VOS ,
T
 usually in VC1 quoted at “room temp” 25C
VOS
VOS ( T )  VOS ( 25 C ) 
( T  25)
T
VOS
 Devices with low VOS also have low
T
Power Supply Rejection Ratio (PSRR)
Changes in supply voltage(s) affect biassing and
hence VOS
Defined as:
VOS
PSRR = V
supply
specified in VV1
i.e.
PSRR
or dB
= 20 log 10
VOS
Vsupply
dB
with Vsupply = 1V
Common-Mode Rejection Ratio (CMRR)
 important in Non-Inverting or Differential
configurations.
 Common-mode voltage affects VOS
 Example (Non-Inverting configuration)
R2
R1
VOS
Vo
Vi
Normally:
Vd  V p  Vn  0  V p  Vn
But the fact that Vp = Vi means that both I/Ps are at
a potential other than zero and this affects the bias
conditions and hence VOS
Define the Common-mode voltage as:
VCM 
V p  Vn
2
 Vi
then CMRR 
VOS
VCM
i.e. CMRR = 20 log 10
specified in VV1
or dB
VOS
dB with VCM = 1V
VCM
Offset Error Compensation
By superposition, the combined effect of IOS and
VOS is:

R 
E o   1  2   VOS   R1 / / R2  I OS
R1 


(Since polarity of both is uncertain must consider
the worst case – hence we use the absolute values)
 Some op-amps have pins for “internal” offset
nulling (correction)
 In other cases, an adjustable dc voltage is injected
to compensate for the existing offset error (as
detected by instruments)
 In circuits with more than one op-amp, it is
(generally) sufficient to null the overall error by
adjustment of just one device. (Superposition)
Frequency Response
a ( jf ) 
ao
where ao is the dc open loop gain
 f 
1  j 
 fa 
fa is the open-loop corner (or break, or 3dB, or
cut-off) frequency. In this case, it is also the openloop BANDWIDTH.
With negative feedback (Non-Inverting
configuration)
V
Vi
Vfb
As before:
R1
b
R1  R 2
Closed-loop gain is:
A( jf ) 
Ao
 f 
1  j 
 fA
a(jf)
b
Vo
ao
1
1

1  aob b 1  1
aob
f A  f a (1  aob )
Ao 
fA is the closed-loop corner (or break, or 3dB, or
cut-off) frequency. In this case, it is also the
closed-loop BANDWIDTH.
a
20 log10 ao
ab
A
20 log10 Ao
f
fa
Still 1st order
Since f t  ao f a and
fA
ft
Ao 
1
b
f A  f a  a0 f a b  f a  bf t  bf t
Hence ,
Ao f A  f t
 Constant gain-bandwidth product (GBP)
 This is an important specification of an op-amp
For the Inverting configuration, there is a
reduction in Ao and fA (and GBP)
Remember:
Vi
V
b 1
Fictitious
point in
circuit
Vfb
Closed Loop Gain , A( jf )  b  1
 Ao  1 
R
1
 2
b
R1
a(jf)
b
a ( jf )
1  a ( jf )b
Vo
fA 
R1
ft
R1  R2
GBP 
R2
ft
R1  R2
f t  a0 f a
 Input and output impedances are also affected by
frequency
For example:
For Non-Inverting configuration, Zin decreases and
Zo increases.
Time-domain considerations
 Since an op-amp behaves as a 1st order system in
both open- or closed loop connection, then the
transient (step) response has a non-zero RISETIME
 If we define the rise-time tr as the time to go from
10% to 90% of final value, then we can show
0.35
tr 
ft
Important relation between time-domain and
frequency-domain specification
So far we have confined ourselves to our standard
model that assumes linear behaviour and therefore
assumes small signals.
 For large step amplitudes, the device operates in
non-linear mode and the slope of the time
response “saturates” at a max value known as the
SLEW RATE the maximum rate at which the
output can change
 dV (t ) 
SR   o 
 dt  max