The Agilent Technologies 16533A and 16534A digitizing oscilloscopes
offer basic oscilloscope functionality. The oscilloscope can be easily
correlated with other instruments in the Agilent Technologies 16700A/
B-series logic analysis system.
Getting Started
•“Calibrating the Oscilloscope” on page 10
•“Probing” on page 14
•“Acquiring a Waveform” on page 31
•“Combining the Oscilloscope with a Logic Analyzer” on page 35
Refining Your Measurement
•“Triggering” on page 38
•“Vertical and Horizontal Scaling” on page 52
•“Changing the Sample Rate” on page 54
•“Comparing Channels” on page 56
•“Using Markers” on page 75
Tip s
•“What Do the Display Symbols Mean?” on page 57
•“Changing Waveform Display and Grid” on page 46
•“Automatic Measurements and Algorithms” on page 61
•“Differences from a Standard Digitizing Oscilloscope” on page 77
•“Using Waveform Memories” on page 78
•“Loading and Saving Oscilloscope Configurations” on page 79
Table of Compatible Probes14
Selecting the Proper Probe15
Compensating the Compensated Passive Divider Probe17
Probe Loading18
Descriptions of Probe Types22
Surface Mount Probing29
Acquiring a Waveform31
Autoscale32
Specifying a Measurement33
Combining the Oscilloscope with a Logic Analyzer35
Trigger Concepts38
Edge Triggering40
Pattern Triggering 41
Delayed Triggering42
Getting a Stable Trigger43
The Trigger Setup Window44
5
Contents
Changing Waveform Display and Grid46
Zooming In46
Changing the Persistence of the Waveform46
Viewing Noisy Waveforms with Averaging48
Changing Display Colors50
Changing the Grid50
Vertical and Horizontal Scaling52
Changing the Sample Rate54
Comparing Channels56
What Do the Display Symbols Mean?57
Display Setup Window59
6
Contents
Automatic Measurements and Algorithms61
How the Scope Makes Measurements 62
Average Voltage (Vavg) 63
Period63
Rise Time 63
Fall Time64
Negative and Positive Pulse Width (
Frequency 65
Base Voltage (Vbase)66
Top Voltage (Vtop)66
Preshoot67
Overshoot68
Peak-to-Peak Voltage (Vpp) 68
Minimum Voltage (Vmin)69
Maximum Voltage (Vmax) 69
Time of Minimum Voltage (Tmin)70
Time of Maximum Voltage (Tmax)70
Voltage Amplitude (Vamp)70
Vdcrms (Root Mean Square Voltage, DC)71
About the Measurements71
Increasing the Accuracy of Your Measurements73
±Width) 64
Using Markers75
About Automatic Time Markers76
Differences from a Standard Digitizing Oscilloscope77
Using Waveform Memories78
Loading and Saving Oscilloscope Configurations79
When Something Goes Wrong80
Error Messages 80
Calibration Problems80
Triggering Problems80
Other Problems81
7
Contents
Specifications and Characteristics85
What is a Specification88
What is a Characteristic88
What is a Calibration Procedure88
What is a Function Test89
The oscilloscope requires a full operational accuracy calibration by you
or a service department whenever
•it has been 6 months or 1,000 hours of use since last full calibration.
•the ambient temperature changes more than 10 degrees C from the
temperature at the time of the last full calibration.
•the frame configuration changes.
•you need to optimize measurement accuracy.
You will get more accurate measurements from the oscilloscope if you
perform the operational accuracy calibration at least once a year.
NOTE:Channel skew calibration requires a multi-board oscilloscope. The procedure
cannot be performed on single-board (2-channel) oscilloscopes.
To calibrate the oscilloscope
This is also covered in the Logic Analysis System Installation Guide.
Since this procedure requires you to turn off the system, print this
information if you do not have access to the Installation Guide.
1. If your oscilloscope has more than two channels, disconnect the short
cables on the back of the module that connect the boards.
2. Unprotect the memory.
a. Turn off the Agilent Technologies 16700A/B-series frame.
b. Take the oscilloscope module out of the frame. See the Logic Analysis
3. Turn on the 16700A/B-series frame and wait for it to finish booting.
You will get a more accurate calibration if you warm up the system for 30
minutes before calibrating the oscilloscope.
4. Select the oscilloscope icon, and choose Calibration...
5. Select the procedure ADC through Logic Trigger.
The calibration software will tell you what cables need to be attached.
6. Select the Run button.
7. Select the procedure Ext Trig Skew and connect the cables as directed.
8. Select the Run button.
9. Optional - Calibrate the oscilloscope as a multi-board module.
a. Perform the ADC through Logic Trigger and Ext Trig Skew calibrations
on each oscilloscope board first.
b. In the system window, choose Exit from the File menu.
c. Connect the oscilloscopes together with the short board interconnect
cables. Connect the first board’s TRIG OUT to the next board’s TRIG IN
until all boards are connected.
d. Start a session.
e. Select the oscilloscope icon and choose Calibration.
f. Select the procedure Channel Skew and connect the cables as
directed.
10. After you have finished calibrating, protect the memory. Follow the steps
given above for unprotecting, setting the switch to PROTECT instead.
The ADC calibration procedure produces a linearization table which is
applied to the data out of the analog-to-digital converters (ADC) to
undo the effects of a non-linear, analog-to-digital conversion.
Gain
The Gain calibration procedure measures the actual attenuation of the
attenuators and measures the actual gain of the preamps.
Offset
The Offset calibration procedure determines the actual offset value
that places a null signal in center screen.
Hysteresis
The Hysteresis calibration procedure determines the hardware setting
which is closest to achieving a hysteresis of 0.28 screen divisions.
Trigger Level
The Trigger Level calibration procedure determines the actual trigger
level values for all possible voltage levels across the screen.
Trigger Delay
The Trigger Delay calibration procedure determines a time delay which
correctly lines up the point at which a trace crosses the trigger level
with the trigger time.
Logic Trigger
The Logic Trigger calibration procedure determines settings which
affect the accuracy of duration trigger measurements.
Ext Trig Skew
The Ext Trig Skew calibration procedure lines up the external trigger
edge with the trigger time when triggering on the external channel.
The Channel Skew calibration procedure is only available for multiboard oscilloscope modules. It deskews the trigger channel and data
channels which are on different boards.
The probes covered in the topics below are 1:1 Passive Probes, Active
Probes, Current Probes, Compensated Passive Divider Probes,
Differential Probes, and Resistive Divider Probes.
•“Table of Compatible Probes” on page 14
•“Selecting the Proper Probe” on page 15
•“Compensating the Compensated Passive Divider Probe” on page 17
•“Probe Loading” on page 18
•“Descriptions of Probe Types” on page 22
•“Surface Mount Probing” on page 29
Table of Compatible Probes
* Most frequently used
Agilent
Model Probe Type Band- Input Div Input R Input C
Numbers width Z ratio
“Channel Setup Window” on page 33 for setting input impedance and
coupling
Selecting the Proper Probe
Use the flowchart below for selecting the proper type of probe. A
comparison of features, tradeoffs, and applications of the probes are
available after the flowchart.
Tradeoffs Bigger than a passive probe, high cost, requires power, and
lower bandwidth than other probes.
Applications Measuring waveforms not referenced to the scope ground,
troubleshooting power supplies, and differential amplifier probing.
Resistive Divider Probe
Features
Highest bandwidth, lowest capacitive load, lower cost than
active probes, flat pulse response, good timing measurement accuracy.
Tradeoffs Relatively heavy resistive loading.
Applications ECL probing, GaAs probing, and transmission line probing.
See Also“Descriptions of Probe Types” on page 22
“Table of Compatible Probes” on page 14
Compensating the Compensated Passive
Divider Probe
Before you can have a flat frequency response when using a
Compensated Passive Divider Probe, the probe’s cable capacitance and
scope input capacitance must be compensated. One of the
compensating capacitors in the probe is adjustable so you can optimize
the step response for flatness.
1. Connect the probe to the BNC Output, labeled AC/DC CAL, on the back of
the oscilloscope.
2. Connect the probe ground lead to ground.
3. Select the oscilloscope icon and choose Calibration...
4. At the bottom of the calibration window, set BNC Output to Probe Comp
and close the window.
5. Select the oscilloscope icon and choose Setup/Display...
7. You should see a waveform similar to one of the following.
8. If necessary, adjust the probe’s compensating capacitor. Set the scope to
keep running by selecting the Run Repetitive button.
Probe Loading
Probe Resistance and
Capacitance
Characteristics
There are two major factors influencing probe selection: the load the
probe imposes on your circuit and the required bandwidth of your
circuit with the probe. This is discussed in three sections, below.
Probe Resistance and Capacitance Characteristics (see page 18)
Probe Ground Lead Characteristics (see page 20)
Understanding System Bandwidth at the Probe Tip (see page 20)
The probe load has both resistive and capacitive components. In
addition, the inductance in the probe ground lead causes ringing.
The probe resistance to ground forms a voltage divider network with
the source resistance of your circuit. This reduces the waveform
amplitude and the dc offset. For example, if the probe’s resistance is 9
times the Thevenin equivalent resistance of your circuit, the waveform
amplitude is reduced by about 10 percent. Therefore, if your waveform
has a +5 V to 0.8 V range, the scope probe system shows a 4.5 V to 0.72
V range.
NOTE:At high frequencies, the probe reactance dominates the resistance.
The probe capacitive loading (Cin) to ground forms an RC circuit with
the resistance of your circuit (R
the probe and scope (R
). The time constant of this RC circuit slows
in
) and the resistance looking into
source
the rise time of any transitions, increases the slew rate, and introduces
delay in the actual transition time. The approximate rise time of a
simple RC circuit is:
t
R
RC
Tot al
= 2.2R
= [RinR
Tot alCin
source
where
]/[Rin + R
source
]
Thus, for circuit resistance of 100 ohm, a scope probe system
resistance of 1 Mohm, and a probe capacitance of 8 pF, the real rise
time due to probe loading is:
Therefore, the rise time of your circuit cannot be faster than
approximately 1.8 ns, even though it might be faster without the probe.
If the output of the circuit under test is current-limited (as is often the
case for CMOS), the slew rate is limited by the relationship dV/dT = I/C.
Perhaps you have connected a scope to a circuit for troubleshooting
only to have the circuit operate correctly after connecting the probe.
The capacitive loading of the probe can attenuate a glitch, reduce
ringing or overshoot of your waveform, or slow an edge just enough
that a setup or hold time violation no longer occurs.
NOTE:If you print this page, subscripts and superscripts appear on the main line of
text. If a number seems to be in an odd place in the printed copy, it is probably
a superscript.
The inductance of the probe’s ground lead forms an LC circuit with the
probe’s capacitance and the output capacitance of the circuit under
test, including any parasitic capacitance of PC board traces, and so on.
The ringing frequency (F) of this circuit is:
F = (2 (3.14) (LC)
1/2)-1
If the rise time of the waveform is sufficient to stimulate this ringing,
the ringing can appear as part of your captured waveform. To calculate
the ringing frequency, you can assume that the probe’s ground lead has
an inductance of approximately 25 nH per inch. So, a probe with a
capacitance of 8 pF and a 4-inch ground lead has a ringing frequency of
approximately:
1/2)-1
F = (2 (3.14) [(25 nH) (4 inches) (8 pF)]
= 178 MHz
Understanding
System Bandwidth at
the Probe Tip
The 178 MHz does not include your circuit capacitance. Therefore, a
waveform with a rise time of less than 1.9 ns can stimulate ringing.
= 0.35/178 MHz = 1.9 ns
t
rise
To minimize the ringing effect, you should use a probe ground lead that
is as short as possible. Some probes add a ferrite bead to the ground
lead to reduce ringing. However, adding the ferrite bead also increases
the ground impedance which reduces the common mode rejection of
the probe.
System bandwidth is the bandwidth of the scope probe system. System
bandwidth affects measurements because the probe becomes part of
the circuit being measured. The rise time that is measured depends on
the actual rise time, the rise time of the scope probe system, and the
rise time of the RC circuit formed by the source resistance and the
scope probe system resistance and capacitance.
t
meas
= [t
act
2
+ t
RC
2
+ t
sys
2
1/2
]
where
= the measured rise time.
t
meas
= the actual rise time of the waveform being measured.
t
act
= the rise time of the RC circuit formed by the source resistance
t
RC
and the scope probe system resistance and capacitance.
= the rise time of the scope probe system.
t
sys
NOTE:Often the bandwidth of the scope probe system is specified. The rise time is
calculated using the following equation.
= 0.35/SystemBW
t
sys
If the rise time of the scope probe system is not specified, it can be calculated
using the following formula.
probe
2
+ t
= [t
t
sys
scope
1/2
2
]
For example, if the scope probe system rise time is 600 ps, the probe
loading rise time (t
) is 600 ps, and the waveform has a 1-ns rise time,
RC
then the measured rise time is:
t
= [(1 ns)2 + (600 ps)2 + (600 ps)2]
meas
1/2
= 1.3 ns
The answer is in error by 30%.
However, if the scope probe system rise time is 190 ps, the probe
loading rise time is 190 ps, and the waveform has a 1-ns rise time, then
the measured rise time is:
= [(1 ns)2 + (190 ps)2 + (190 ps)2]
t
meas
1/2
= 1.03 ns
Now the error is only 3%.
You may find it useful to memorize three system bandwidth rules:
1. The combined rise time of the scope probe system and the probe loading
should be less than 1/3 of the rise time of the waveform you are measuring
to keep errors below 5%, and less than 1/7 of the rise time of the waveform
you are measuring to keep errors below 1%.
2. Rise time and bandwidth are related by the following approximations: rise
time = 0.35/bandwidth and bandwidth = 0.35/rise time.
3. Rise times add approximately as the square root of the sum of the squares
(for systems with minimal peaking).
NOTE:Because every scope probe has a different loading effect on your circuit, you
should use the equation given for the type of scope probe you are using.
See Also“Descriptions of Probe Types” on page 22
Descriptions of Probe Types
For each of the probe types listed below, the description gives a
summary of features and tradeoffs and a short text description. Most of
the probe types also give a sample rise time calculation.
•“1:1 Passive Probes” on page 22
•“Active Probes” on page 24
•“Compensated Passive Divider Probes” on page 25
•“Current Probes” on page 27
•“Differential Probes” on page 27
•“Resistive Divider Probes” on page 28
1:1 Passive Probes
Features No attenuation of waveform.
Tradeoffs High capacitive loading and low bandwidth.
Applications Measuring small, low-bandwidth waveforms when no
attenuation can be tolerated such as power supply ripple.
The 1:1 passive probes provide a way to connect the input impedance
of the scope directly to your circuit with minimum attenuation due to
the resistive loading of the probe. However, 1:1 probes do have very
high capacitive loading which is much larger than that of the scope.
There are two types of 1:1 passive probes. One type is designed to work
with the scope’s input set to high impedance (1 Mohm) and uses a
lossy cable to keep the probe from ringing. The other type is designed
to work with the scope’s input set to low impedance (50 ohm) and uses
a 50-ohm coaxial cable.
Example Rise Time
Calculation
Given the following circuit using the Agilent Technologies 1162A
probe,
the input resistance is:
= R
R
in
= 1 Mohm
scope
The total resisitance is:
= (RinR
R
Tot al
= 1 Mohm(50 ohm)/(1 Mohm + 50 ohm) = 50 ohm
R
Tot al
source
)/(Rin + R
source
)
From the Table of Compatible Probes, the probe capacitance is 50 pF.
Therefore, the capacitive load is:
= C
C
in
probe
+ C
= 50 pF + 7 pF = 57 pF
scope
The rise time due to circuit loading is:
= 2.2R
t
RC
Tot alCin
tRC = 2.2(50 ohm)(57 pF) = 6.2 ns
From the Table of Compatible Probes, the scope probe system has a
bandwidth of 25 MHz. Therefore, the rise time of the scope probe
system is: t
Applications ECL, CMOS, GaAs probing, analog circuit probing,
transmission line probing, source resistance
probing, most accurate for general measurements of circuits of
unknown impedance.
An active probe has a buffer amplifier at the probe tip. This buffer
amplifier drives a 50-ohm cable terminated in 50 ohms at the scope
input. Active probes offer the best overall combination of resistive
loading, capacitive loading, and bandwidth.
≥10 kohm, op amp
Example Rise Time
Calculation
Given the following circuit using the Agilent Technologies 1152A
probe,
the input resistance is:
= 100 kohm. The total input resistance is:
R
in
= (RinR
R
Tot al
= 100 ohm(50 ohm)/(100 ohm + 50 ohm) = 50 ohm
R
Tot al
source
)/(Rin + R
source
)
The rise time due to circuit loading is:
= 2.2R
t
RC
Tot alCtip
tRC = 2.2(50 ohm)(0.6 pF) = 66 ps
Because the rise time of the scope probe system is not given in the
Table of Compatible Probes, we will have to calculate it using the
bandwidth of the probe (2.5 GHz) and the bandwidth of the scope (500
MHz). Therefore, the rise time of the scope probe system is:
= 0.35/ProbeBW = 0.35/2.5 GHz = 140 ps
t
probe
= 0.35/ScopeBW = 0.35/500 MHz = 700 ps
t
scope
t
= [t
sys
t
= [(140 ps)2 + (700 ps)2]
sys
probe
2
+ t
scope
2
1/2
]
1/2
= 714 ps
The measured rise time is:
t
meas
= [t
act
2
+ t
RC
2
+ t
sys
2
1/2
]
t
= [(2 ns)2 + (66 ps)2 + (714 ps)2]
meas
1/2
= 2.12 ns
Compensated Passive Divider Probes
Features Very low resistive loading, accurate amplitude measurements,
large dynamic range, and low cost.
Tradeoffs Capacitive loading <10 pF, lower bandwidth than active or
50-ohm resistive divider probes.
Applications General purpose probing, probing high-impedance nodes
≥10 Kohm), op amp probing, CMOS probing (if bandwidth is
(
adequate), TTL probing (if bandwidth is adequate).
The compensated passive divider probe is the most common type of
scope probe. The 9-Mohm resistor in the tip forms a 10:1 voltage
divider with the 1-Mohm input resistance of the scope.
To have a flat frequency response, the probe tip capacitance is
compensated by the probe’s cable capacitance, a compensating
capacitor, and the scope input capacitance. The compensating
capacitor is adjustable so you can optimize the step response for
flatness.
Not all 9-Mohm divider probes work with all 1-Mohm scope inputs. The
probe data sheet shows the range of scope input capacitance it can
accommodate. You must make sure that the input capacitance of the
scope is within that range.
Features Measures both ac and dc currents on a scope, with minimal
circuit loading.
Tradeoffs Large size.
Applications Power measurements, automotive measurements,
industrial measurements, motors, dynamoes, and alternators.
Scopes are designed to measure voltage, but by using a current probe
you can measure current. A current probe measures current in a wire
by enclosing the wire. Therefore, no electrical connection is needed.
Current probes generally use one of two technologies. The simplest
uses the principle of a transformer, with one winding of the
transformer being the measured wire. Because transformers only work
with alternating voltages and currents, current probes of this type
cannot measure direct current.
The other type of current probe uses the Hall effect principle. The Hall
effect produces an electric field in response to an applied magnetic
field. While this technique requires a power supply, it measures both
alternating and direct current.
Differential Probes
Features High common mode rejection ratio, easy viewing of small
waveforms with large dc offsets, more accurate than subtracting one
channel from another.
Tradeoffs Bigger than a passive probe, high cost, requires power, and
lower bandwidth than other probes.
Applications Measuring waveforms not referenced to the scope ground,
troubleshooting power supplies, and differential amplifier probing.
A differential probe is a high-impedance differential amplifier with two
probe tips; a non-inverting input and an inverting input. These two
inputs feed a differential amplifier which in turn drives the 50-ohm
input of the scope. The main advantage of differential probes is their
ability to reject waveforms that are common to both inputs. This type
of probe is often used in floating ground applications.
You could duplicate a differential probe by using two passive probes
and subtracting the two scope channels. However, the electrical paths
of the differential probe are carefully matched to give a high common
mode rejection ratio (CMRR). The higher the CMRR, the smaller the
waveforms you can view in the presence of unwanted noise.
Resistive Divider Probes
Features Highest bandwidth, lowest capacitive load, lower cost than
active probes, flat pulse response, good timing measurement accuracy.
Tradeoffs Relatively heavy resistive loading.
Applications ECL probing, GaAs probing, and transmission line
probing.
Resistive divider probes are designed for scopes with a 50-ohm input
impedance. The probe tips of the Agilent Technologies 1163A or
54006A have either a 450-ohm or 950-ohm series resistor. The probe
cable is a 50-ohm transmission line. Because the cable is terminated in
50 ohms at the scope input, it looks like a purely resistive 50-ohm load
when viewed from the probe tip. Therefore, the resistive divider probe
is flat over a wide range of frequencies, limited primarily by the
parasitic capacitance and inductance of the 450-ohm or 950-ohm
resistor and the fixture that holds it. The resistive load of the probe to
your circuit is either 500 ohm or 1 kohm, depending on the probe.
Example Rise Time
Calculation
This type of probe has the smallest capacitive load of any probe. The
small capacitance and wide bandwidth make this probe type a good
choice for wide bandwidth measurements or time-critical
measurements.
Given the following circuit using the Agilent Technologies 1163A
probe,
From the Table of Compatible Probes, the bandwidth of the scope
probe system is 1.5 GHz. Therefore, the rise time of the scope probe
system is:
= 0.35/SystemBW
t
sys
= 0.35/1.5 GHz = 230 ps
t
sys
The measured rise time is:
= [(t
t
meas
t
= [(2 ns)2 + (165 ps)2 + (230 ps)2]
meas
)2 + (tRC)2 + (t
act
sys
)2]
1/2
1/2
= 2.02 ns
Surface Mount Probing
The Agilent Technologies 10467A 0.5 mm MicroGrabber Accessory Kit
is designed for using the Agilent Technologies 116x family of probes
when you are probing fine-pitch (0.5 mm to 0.8 mm) SMT (Surface
Mount Technology) devices. The kit contains enough parts for two
probes.
The Agilent Technologies 116x probe tip plugs into the single-lead end
of the dual-lead adapter. The MicroGrabber connects to the red lead.
You can also use a MicroGrabber on the black lead, which you should
connect to your circuit’s ground. You can also connect the dual-lead
end to circuit pins that are 0.635 mm (0.025 inch) in diameter.
The kit is intended for use with voltages no greater than
ac peak).
±40 V (dc and
30
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