A Primer on Differential Measurements,
Types of Amplifiers, Applications, and
Avoiding Common Errors
Simulated 4 mV
noise, using a conventional oscilloscope probe (upper). A differential amplifier extracts the signal from the noise
heartbeat waveform can not be measured in the presence of 500 mV
p-p
Introduction
All Measurements Are Two-Point
Voltage is always measured
between two points in a circuit. This is true whether
using a voltmeter or an oscilloscope. When an oscilloscope probe touches a point
in a circuit, a waveform usually appears on the display,
even if the ground lead is not
connected. In this situation,
the reference for the measurement is conducted
through the safety ground of
the scope chassis to the electrical ground in the circuit.
By virtue of their two probes,
digital voltmeters measure
potential between two
points. Because they are iso-
lated, these two points can
be anywhere in the circuit.
This has not always been the
case. Before the advent of the
digital voltmeter, hand-held
meters known as VOMs
(Volt-Ohm-Meters) were
used to measure “floating”
circuits. Because they were
passive, they tended to load
the circuit-under-test. Less
invasive measurements were
made with the highimpedance VTVM (Vacuum
Tube Volt Meter). The VTVM
had one major limitation –
the measurement was always
referenced to ground. The
VTVM housing was
grounded and connected to
the reference lead. With the
, 60 Hz common-mode
p-p
introduction of solid-state
gain circuits, high performance voltmeters could be
isolated from ground, allowing floating measurements to
be made.
Most oscilloscopes today,
like the venerable VTVM,
can only measure voltages
that are referenced to earth
ground, which is connected
to the scope chassis. These
are referred to as “singleended” measurements – the
probe ground provides the
reference path. Unfortunately, there are times when
this limitation lowers the
integrity of the measurement,
or makes measurement
impossible.
If the voltage to be measured
is between two circuit nodes,
neither of which is
grounded, conventional
oscilloscope probing cannot
be used. A common example
is measuring the gate drive in
a switching power supply
(see Figure 1).
Signals which are balanced
(between two leads without a
ground return) such as a
common telephone line cannot be measured directly. As
we shall see, even some
“ground referenced” signals
cannot be faithfully measured using single-ended
techniques.
When Ground Is Not Ground
We’ve all heard of “ground
loops” and been taught to
avoid them. But how do they
corrupt a scope measurement? A ground loop results
when two or more separate
ground paths are tied
Related Publications from Tektronix · · · · · · · 16
Figure 2. Ground loop formed by a scope probe. Metal chassis of both scope and device
under test are connected to safety ground and internal power supply common. Scope
probe ground connects to scope chassis at the input BNC connector.
together at two or more
points. The result is a loop of
conductor. In the presence of
a varying magnetic field, this
loop becomes the secondary
of a transformer which is
essentially a shorted turn.
The magnetic field which
excites the transformer can
be created by any conductor
in the vicinity which is carrying a non-DC current. AC
line voltage in primary
wiring or even the output
lead of a digital IC can produce this excitation. The current circulating in the loop
impedance within the loop.
Thus, at any given instant in
time, various points within a
ground loop will not be at
the same potential.
Connecting the ground lead
of an oscilloscope probe to
the ground in the circuitunder-test results in a ground
loop if the circuit is
“grounded” to earth ground
(see Figure 2). A voltage
potential is developed in the
probe ground path resulting
from the circulating current
acting on the impedance
within the path.
develops a voltage across any
page 2
Thus, the “ground” potential
at the oscilloscope’s input
BNC connector is not the
same as the ground in the
circuit being measured (i.e.,
“ground is not ground”).
This potential difference can
range from microvolts to as
high as hundreds of millivolts. Because the oscilloscope references the measurement from the shell of
the input BNC connector, the
displayed waveform may not
represent the real signal at
the probe input. The error
becomes more pronounced
being measured decreases, as
is common in transducer and
biomedical measurements.
In these situations, it’s often
tempting to remove the probe
ground lead. This technique
is only effective when measuring very low-frequency
signals. At higher frequencies, the probe begins to add
“ring” to the signal caused by
the resonant circuit from the
tip capacitance and shield
inductance (see Figure 3).
(This is why you should
always use the shortest
ground lead possible.)
as the amplitude of the signal
Figure 3. Series resonant tank circuit formed by probe-tip capacitance and ground inductance.
Figure 4. “Floating” battery-powered cellular telephone probed with a grounded oscilloscope. Capacitance
between the phone circuitry and steel bench frame forms a virtual ground loop at high frequencies.
Figure 5. Minute parasitic inductance and resistance in ground distribution system result in VG≠ V'G.
We now have a dilemma:
create a ground loop and add
error to the measurement or
remove the probe ground
lead and add ring to the
waveform!
The next technique often
tried to break ground loops is
to “float” the scope or “float”
the circuit being measured.
“Floating” refers to breaking
the connection to earth
ground by opening the
safety-ground conductor –
either at the device-undertest or at the scope. Floating
either the scope or the
device-under-test (DUT)
allows the use of a short
ground lead to minimize ring
without creating a ground
loop.
This practice is inherently
dangerous, as it defeats the
protection from electrical
shock in the event of a short
in the primary wiring. (Some
special battery-operated
portable scopes incorporate
insulation which allows safe
floating operation.) Operator
safety can be restored by
placing a suitable groundfault circuit interrupter
(GFCI) in the power cord of
the oscilloscope (or deviceunder-test) with the severed
ground. However, be aware
that without a lowimpedance ground connection, radiated and conducted
emissions from the scope
may now exceed government
standards – as well as interfere with the measurement
itself. At higher frequencies,
severing the ground may not
break the ground loop as the
“floating” circuit is actually
coupled to earth ground
through stray capacitance
(see Figure 4).
Even when the measurement
system doesn’t introduce
ground loops, the “ground is
not ground” syndrome may
exist within the device being
measured (see Figure 5).
Large static currents and
high-frequency currents act
on the resistive and induc-
page 3
tive components of the
device ground path to produce voltage gradients. In
this situation, the “ground”
potential referenced at one
point in the circuit will be
different than that referencing another point.
For example, ground at the
input of the high-gain amplifier in a system differs from
the “ground” potential at the
power supply by several
millivolts. To accurately
measure the input signal
seen by the amplifier, the
probe must reference the
ground at the amplifier input.
These effects have challenged designers of sensitive
analog systems for years. The
same effect is seen in fast
digital systems. The small
inductance within the
ground distribution system
can create a potential across
it, resulting in “ground
bounce”. Troubleshooting
systems affected by groundvoltage gradients is difficult
because of the inability to
really look at the signal
“seen” at the individual component. Connecting the oscilloscope probe ground lead to
the “ground” point of the
device results in the uncertainty of what effects the new
path adds to the ground gradient. A sure clue that a
change is occurring is seen
when the problem in the circuit either gets better (or
worse) when the probe
ground is connected. What
we really need is a method to
make a scope measurement
of the actual signal at the
input of the suspect device.
By using an appropriate differential amplifier, probe, or
isolator, accurate two-point
oscilloscope measurements
can be made without introducing ground loops or otherwise corrupting the measurement, upsetting the
device-under-test, or exposing the user to shock hazard.
There are several types of
differential amplifiers and
isolation systems available
for oscilloscopes, each optimized for a particular class
of measurements. In order to
choose the proper solution,
an understanding of terminology is necessary.
Overview of Differential
Measurements
An ideal differential amplifier amplifies the “difference”
signal between its two inputs
and totally rejects any voltage
which is common to both
inputs (see Figure 6). The
transfer equation is:
VO= AV( V
where VOis referenced to
earth ground.
The voltage of interest, or
difference signal, is referred
to as the differential voltage
or differential mode signal
and is expressed as V
is the V
transfer equation above).
Figure 6. Differential amplifier.
page 4
+in
Differential Measurement Fundamentals
The voltage which is common to both inputs is
referred to as the CommonMode Voltage expressed as
. The characteristic of a
V
CM
differential amplifier to
is referred to
CM
+ i n
– V
– V
)
– i n
term in the
–in
DM(VDM
ignore the V
as Common-Mode Rejection
or CMR. The ideal differential amplifier rejects all of the
common-mode component,
regardless of its amplitude
and frequency.
In Figure 7, a differential
amplifier is used to measure
the gate drive of the upper
MOSFET in an inverter circuit. As the MOSFET switches
on and off, the source voltage
swings from the positive sup-
ply rail to the negative rail. A
transformer allows the gate
signal to be referenced to the
source. The differential amplifier allows the scope to measure the true V
signal (a few
G S
volt swing) at sufficient resolution such as 2 V / d i v i s i o n
while rejecting the several
hundred volt transition of the
source to ground.
Common-Mode Rejection Ratio
( C M R R )
Real implementations of differential amplifiers cannot
reject all of the common
mode signal. A small amount
of common mode appears as
an error signal in the output,
making it indistinguishable
from the desired differential
signal. The measure of a differential amplifier’s ability to
eliminate the undesirable
common-mode signal is
referred to as Common-Mode
Rejection Ratio or CMRR for
short. The true definition of
CMRR is “differential-mode
gain divided by commonmode gain referred to the
input”:
A
CMRR =
D M
A
C M
Figure 7. Differential amplifier used to measure gate to source voltage of upper transistor in an inverter bridge.
Note that the source potential changes 350 volts during the measurement.
Figure 8. Common-mode error from a differential amplifier with 10,000:1 CMRR.
For evaluation purposes, we
can assess CMRR performance with no input signal.
The CMRR then becomes the
apparent V
put resulting from common
mode input. It’s expressed
either as a ratio – 10,000:1 –
or in dB:
dB = 20log
A CMRR of 10,000:1 would
be equivalent to 80 dB.
seen at the out-
DM
V
D M
(
)
V
C M
For example, suppose we
need to measure the voltage
in the output damping resistor of an audio power amplifier as shown in Figure 8. At
full load, the voltage across
the damper (V
reach 35 mV, with an output
swing (VCM) of 80 V p-p. The
differential amplifier we use
has a CMRR specification of
10,000:1 at 1 kHz. With the
amplifier driven to full
power with a 1 kHz sine
) should
DM
wave, one ten thousandth of
the common-mode signal
will erroneously appear as
at the output of the dif-
V
DM
ferential amplifier, which
would be 80 V/10,000 or
8 mV. The 8 mV represents
up to a 22% error in the true
35 mV signal!
The CMRR specification is
an absolute value, and does
not specify polarity (or
degrees of phase shift) of the
error. Therefore, the user can
not simply subtract the error
from the displayed waveform. CMRR generally is
highest (best) at DC and
degrades with increasing frequency of V
ential amplifiers plot the
CMRR specification as a
function of frequency.
Let’s look at the inverter circuit again. The transistors
switch 350 V and we expect
about a 14 V swing on the
gate. The inverter operates at
30 kHz. In trying to assess
the CMRR error, we quickly
run into a problem. The common-mode signal in the
inverter is a square wave,
and the CMRR specification
assumes a sinusoidal common-mode component.
Because the square wave
contains energy at frequencies considerably higher than
30 kHz, the CMRR will probably be worse than specified
at the 30 kHz point.
Whenever the common-mode
component is not sinusoidal,
an empirical test is the
quickest way to determine
the extent of the CMRR error
(see Figure 9). Temporarily
connect both input leads to
the MOSFET source. The
scope is now displaying only
the common-mode error. You
can now determine if the
magnitude of the error signal
is significant. Remember, the
phase difference between
and VDMis not specified.
V
CM
Therefore subtracting the displayed common-mode error
from the differential mea-
. Some differ-
CM
page 5
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