LeCroy Digital Oscilloscopes Manual
Text of the manual
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Chestnut Ridge, NY 10977–6499
Tel: (914) 578 6020, Fax: (914) 578 5985
LeCroy SA
2, rue du Pré-de-la-Fontaine
1217 Meyrin 1/Geneva, Switzerland
Tel: (41) 22 719 21 11, Fax: (41) 22 782 39 15
Internet: www.lecroy.com
Copyright © April 1998, LeCroy. All rights reserved. Information in this publication supersedes all
earlier versions. Specifications subject to change.
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LCXXX-HG-E
Rev C
0498
A broad overview of the Digital Storage Oscilloscope, zooming
on LeCroy Color DSOs.
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Basic Elements...................................................................1–2
Bandwidth............................................................................1–3
Sample Rate .......................................................................1–4
Memory Length...................................................................1–4
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Acquisition Technique ........................................................1–5
Analog–Digital Conversion.................................................1–6
Number of Channels ..........................................................1–6
Triggering............................................................................1–6
6LJQDO9LHZLQJ............................................................................1–7
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Pulse Parameters...............................................................1–8
Waveform Math..................................................................1–8
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Time Domain ......................................................................1–9
Frequency Domain .............................................................1–9
Statistical Domain...............................................................1–9
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Removable Hard Disk Drive (HDD).................................1–10
Interfaces...........................................................................1–11
An illustrated tour of the scope, then ‘hands-on’ for a run
through its basic functions.
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,QVWDOODWLRQ&KHFN.....................................................................2–4
,QLWLDOL]DWLRQ.................................................................................2–4
:DYHIRUP$FTXLVLWLRQ.............................................................2–7
TRACE ON/OFF.................................................................2–8
TIMEBASE Controls...........................................................2–9
Vertical Controls................................................................2–10
TRIGGER Controls...........................................................2–11
ZOOM................................................................................2–12
CURSORS/MEASURE....................................................2–14
Waveform Parameters.....................................................2–16
Summed Averaging..........................................................2–17
Fast Fourier Transform (FFT)..........................................2–20
Waveform Storage ...........................................................2–21
Save and Recall Setup.....................................................2–23
Performing the most common measurements using the
scope, in a series of easy-to-follow, step-by-step tutorials.
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The basic steps for setting up practically any measurement.
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How to set up the scope for digitizing on all eight bits.
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Parameter measurement and statistical values made easy.
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Ensure accurate measurements.
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Reduce non-systematic noise and improve the signal-to-noise ratio.
'9LHZLQJZLWK$QDORJ3HUVLVWHQFH ...........................3–31
Explore the new dimensions Analog Persistence reveals.
&RORUVWKDW/LQNDQG'LVWLQJXLVK......................................3–39
Color Association makes signal viewing clearer and easier.
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For a choice of single-shot waveform segments without deadtime.
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Perform signal power distribution as a function of frequency.
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Use the WPO3 option to display and calculate signal jitter.
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Process acquisitions of a few sample points.
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Telecom-measure pulse-shaped signals to industry standards.
6WRULQJWR5HPRYDEOH+DUG'LVN....................................3–109
The portable PC Card hard disk drive (HDD) simplifies storage.
&DOFXODWLQJRQ/RQJ:DYHIRUPV.....................................3–114
Handle longer FFTs and multiple long-waveform zoom, math and
storage.
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Find and capture glitches with the SMART Trigger.
&DSWXULQJ5DUH3KHQRPHQD..............................................3–135
Use the SMART Trigger to increase knowledge of rare waveforms.
7ULJJHULQJRQ/RVW6LJQDOV................................................3–144
Ideal for detecting interruptions in data streams.
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By GPIB, floppy or RS232 communication port.
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Copy screen TIFFs and BMPs to computer.
The title itself is explicit: this is a practical guide that
shows you what the scope can do as you operate it.
The guide offers a helping hand to both the
beginner and the experienced operator of digital
storage oscilloscopes (DSOs). It can be opened at
almost any page and used to enable you to get the
most out of the instrument.
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³an overview of the principles of DSO operation, including data
sampling, triggering, recording, how sampling rate affects usable
bandwidth and how long memory improves sampling rate.
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³shows you around the scope and step-by-step how to capture
waveforms and perform basic measurements.
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³ a set of tutorials describing — again, step-by-step — how to
make the most useful measurements using the scope's advanced
functions.
“HANDS ON” FOR THE COMPLETE PICTURE IN SIGNAL CAPTURE,
VIEW AND ANALYSIS.
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Why and how is the Digital Storage Oscilloscope
(DSO) so useful? What are the many ways in
which it can be put to work for you?
Part 1 maps the digital landscape and
shows you where to find and mine its
riches. Basic concepts are explained and
the main digital concepts and techniques
outlined. The advantages of your LeCroy
scope are also covered.
Having completed Part 1, you’ll then be
ready to zoom in on your scope in Part 2.
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The digital oscilloscope is the essential instrument
used to capture, view and analyze waveforms,
measure signal characteristics and document the
output.
There
are
three
main
DS0
categories.
Top-end models with a bandwidth of around
400 MHz or more are the most suitable for R&D-type
work. The 100–200 MHz models are good for
professional and general purposes. And the
sub-100 MHz, low-cost scopes, are useful for work
on low-frequency signals.
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The way in which each element of the DSO works separately
and in conjunction with the other elements:
Ø Amplifier — amplifies the input signal so that it can be
measured
Ø Analog-to-Digital Converter (ADC) — converts the
analog signal into digital form by translating it into a
series of sample points that are then measured and
transformed into digital codes representing the signal
samples
Ø Acquisition Memory System — stores resulting digital
data
Û System Memory of up to 64 MB
Ø Processor — controls the entire system and performs
special monitoring and measurement functions
Ø Display System — translates stored data into a graphic
display of the signal.
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The character of your signals will determine the primary
specifications of the DSO you will want to use. While your DSO’s
secondary specifications will be determined by the demands of your
applications. In assessing the overall signal representation quality of
a digital oscilloscope, particular consideration needs to be given to
the cardinal parameters of bandwidth, sample rate, and
acquisition memory length.
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The bandwidth specification of a DSO indicates the ability of its front-
end amplifier to faithfully track an incoming signal. The DSO’s
bandwidth is defined as the frequency at which a sinusoidal input
signal has been attenuated to about 70 % of its real amplitude. This
point, at which the vertical amplitude error is about 30 %, is called the
–3 dB point. It is generally advisable to use an instrument whose
bandwidth is five times greater than the highest frequency
component of the signal to be studied.
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The higher the sample rate the better the signal resolution. This is
particularly important for single-shot waveform capture and
measurement. The danger with low sample rates is that important
information may be lost between samples. Accurate waveform
capture requires a sample rate of at least five times the highest
frequency component to be captured. For repetitive signals the
sample rate is a less critical factor, as the signal can be captured
over many cycles.
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Acquisition memory length determines the number of input signal
samples that can be stored. The greater the capacity for stored
samples, the faster the possible sample rate for a given waveform
duration. The signal captured with a long-memory DSO has a
greater resolution, while for short-memory DSOs, the high sample
rates quoted are only available at a few fast time-base settings.
Long-memory DSOs allow operation at the highest possible sample
rate, and over a far greater number of timebase settings.
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The DSO can perform the same operations as an analog
oscilloscope and much more:
Capture of one-off (single-shot) events, stored in memory
Data stays on screen while the scope waits for the next trigger
View of the waveform before the instant of triggering, recording an
event’s cause and effect.
Analysis of signals, providing precise measurement results
Documentation of signals, and the transfer of data via storage
media to PC, or direct to print using an internal or external printer,
or to a plotter.
The DSO’s fidelity in reconstructing the input signal is mainly affected
by these three parameters (by others, too). The bandwidth must be
sufficient to allow all the signal components to pass through the
signal-conditioning system. And the sample rate has to be high
enough to provide a good definition of the signal. Long memory
maintains the sample rate for large time windows.
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In addition to the primary specifications described above, capture
techniques, trigger system, number of channels, availability and type
of probes, and ADC specification all impact the usability and
performance of the DSO.
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Single-shot acquisition is the DSO’s basic acquisition technique,
which makes the instrument very suitable for the study of signal
phenomena that have a low-repetition rate or are not repeated —
hence single-shot. The timebase sweeps and stops at a time after
receiving the trigger signal defined by the user. The captured input
data signal is transferred to memory for viewing, measurement and
analysis.
The DSO may also employ a technique called Random Interleaved
Sampling (RIS) to increase its effective sampling rate in viewing
repetitive signals. LeCroy’s high-performance model has a maximum
rate of 10 giga-samples per second.
For slower timebases, there exists Roll Mode, where the signal
being acquired can be displayed in real time while being captured in
memory, scrolling as on a strip-chart recorder.
Because digital scopes acquire input signals by sampling, they can
miss glitches at the lower sample rates. But LeCroy’s Peak Detect
System captures glitches occurring between these samples. When
the system is activated, the scope samples at a very fast rate,
continuously checking for glitches using a built-in algorithm.
Meanwhile, it displays information in accordance with the sweep rate
actually set. When a glitch is detected, the scope will display it as a
thin spike on the displayed waveform.
Another of the LeCroy scope’s methods for acquiring signals is
Sequence Mode, which captures individually multiple trigger events
separated by dead periods that would otherwise be unacquirable.
When triggering in this mode, the scope grabs a pre-programmed
number of samples, resets its trigger, and awaits another event. The
resulting waveform is a splicing together of all the waveforms
acquired. This eliminates the information-poor deadtime that would
appear between triggers if the scope triggered on the first event and
then continued to run. Sequence Mode allows acquisition of closely-
spaced trigger events.
$QDORJ²'LJLWDO&RQYHUVLRQ High-speed DSO performance is made possible by the use of
advanced ADCs whose vertical resolution will guarantee a clear
representation of the signal. These ADCs measure the voltage level
at evenly spaced intervals and store the digitized value in high-speed
dedicated memory. The shorter the intervals, the faster the digitizing
rate — and the finer the time structure able to be seen. The higher
the resolution of the ADC, the better is its sensitivity to small voltage
changes. And the greater its memory capacity, the longer the
recording time that will be available.
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Your LeCroy DSO has four channels, as well as an external trigger
channel and a CAL BNC output connector. The CAL BNC can be
used as the source of a calibration signal, an output pulse on the
occurrence of each trigger, or an output pulse signaling a Pass/Fail
condition.
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The power of a DSO in any given application depends on a
combination of several features, and particularly on whether it is able
to trigger on the event of interest. A trigger system far more
sophisticated than that found in conventional oscilloscopes is needed
for capturing rare phenomena such as glitches or spikes, logic
states, missing bits, timing jitter, microprocessor crashes, network
hang-ups or bus contention problems. Your LeCroy scope
incorporates this more sophisticated system.
Unlike manufacturers who put their ‘best’ trigger design into their
more expensive scopes and a less adequate one into the lower-
bandwidth, economy models, LeCroy offers all its DSO users, at
every bandwidth, both a standard edge trigger and a powerful
SMART Trigger for capturing elusive events.
A push-button control switches from one of these triggers to the
other. Moreover, the LeCroy DSO has a variety of advanced trigger
modes. The functioning of these modes is based on two important
features. The first is the ability to preset the logic state of the trigger
sources: channels CH 1, CH 2, CH 3, CH 4, and EXT and EXT/10.
The second is a counter that can be preset and used to count a
number of events between 1 and 109, or to measure time intervals
from 2.5 ns–20 s in steps of 1 % of the time scale.
In combination, these twin capabilities open the door to a wide variety
of trigger conditions. But great care has been taken to maintain the
SMART Trigger’s ‘user-friendliness’, without losing this versatility.
Icons illustrate the trigger conditions on-screen for every mode.
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The DSO’s display system translates stored data into a graphic
representation of the signal and shows it on the screen. Also
displayed are internal status and measurement results, as well as
operational, measurement and waveform-analysis menus.
The LeCroy DSO’s large screen and a waveform grid that fills the
viewing area accelerate visual processing and facilitate more
effective communication of on-screen information. Other advanced
display techniques give major performance improvements over
conventional analog or digital scopes. A hardcopy of the screen
contents can be produced at the press of a front-panel screen-dump
button. Multiple waveforms can be viewed on separate grids,
ensuring the best utilization of the ADCs’ dynamic range. XY and
variable persistence displays are also provided, as is Enhanced
Resolution Mode.
A wide range of processing functions can be performed. Four traces
— A, B, C and D — are available for zooming exclusively or together
with waveform mathematics. The horizontal expansion can be huge,
greatly improving the time resolution on the viewed trace. Several
traces can be zoomed onto the same waveform for precise timing
measurements.
performance is at the heart of test engineering.
Most DSOs can measure parameters, but analyzing their
statistics can be a time-consuming chore. LeCroy’s parameter
measurements and statistics allow worst-case analysis of circuit
performance and make the process much faster.
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Cursor readouts allow use of full ADC resolution to measure a
waveform’s absolute or relative times and amplitudes. However,
most users measure the same waveform parameters, such as
risetime, falltime, pulse width, overshoot, undershoot, peak
voltage, peak-to-peak voltage, maximum, minimum, standard
deviation, rms value, frequency, and period. These and many
other parameters are available using your LeCroy oscilloscope.
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Waveform math allows the display of final answers, rather than
raw data. For example, inputs from voltage and current
transformers can be multiplied together to display power. An
important LeCroy DSO feature is the ability to ‘daisy-chain’ math
functions: a power trace can be integrated to display energy, for
instance.
A great advantage of digitizing is the added ability to analyze data.
Once the analog signal has been converted into digital data, the data
can be analyzed either by the DSO’s internal digitizer processor or by
an external computer. Most current digitizers have a wide analysis
spectrum built-in. Depending on the model and its options, LeCroy
DSOs offer a selection of the following analytical features.
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The optional time domain waveform analysis package — includes
zooming, summed averaging of up to one million sweeps,
derivatives, logarithm, square root, absolute value, ratio, six digital
filters and standard arithmetic operations. The zoom feature on high-
performance models expands the waveform so that the individual
data are very clearly separated.
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Spectrum analysis greatly extends the DSO’s processing power and
offers two clear advantages over FFT (Fast Fourier Transform)
analyzers: higher frequency components, and the ability to monitor
both time and frequency information. Fourier transform converts
sampled waveform information into a unique set of sine wave
components. The data is usually plotted as amplitude vs frequency,
exposing information not easily visible in the time domain (amplitude
vs time). Ideally, it can be used for such analyses as measuring
frequency components of communication signals and monitoring drift
in an oscillator. The frequency resolution of an FFT is directly
proportional to the number of time-domain points the FFT algorithm
can handle.
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The existence of measured waveforms in digital representations
permits convenient use of the data inherent in those measurements.
As well as analysis of signals in the frequency domain and the ability
to perform mathematical operations and signal averaging on data,
trends can be determined and histograms of the data analyzed.
The histogram is a graph of the distribution of values of a measured
parameter. For example, when measuring the risetime of a repetitive
signal for which all the measurements are equal, the histogram will
be a straight vertical line without breadth. However, variations in
risetimes create a plot with some horizontal structure, implying
variations in the measurements. Your LeCroy DSO is able not only to
create such histograms, but also to allow measurement of their
characteristics. This is extremely useful when analyzing pulse
amplitudes, widths or timing jitter.
Other LeCroy analysis techniques include Pass/Fail testing, Mask
Comparison
testing,
EYE-diagram
analysis
for
telecom
applications, and the specialized testing for magnetic media
applications, DDM (Disk Drive Measurements) and PRML (Partial
Response Maximum Likelihood).
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Storage and recording functions are key requirements in many test
applications. The LeCroy digital scopes produce excellent output, in
the form of either digital data or hard-copy records.
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Files saved in the TIFF format can be imported into PCs and other
computers. The portable PC Card HDD (Hard Disk Drive) is a
PCMCIA Type III device much faster than a floppy disk and with far
greater capacity that can be popped in and out of your LeCroy DSO
or computer. There is an HDD adapter on the rear panel of your
scope.
Note that test data can be processed far more quickly inside a DSO,
and saved on the scope’s internal HDD, than by transfer via GPIB
link to computer.
The PC Card Memory Card drive and built-in floppy disk drive —
located on the front panel of your LeCroy DSO — can also be used
to store waveforms and screen shots. The built-in thermal printer is
quick and convenient for producing a screen-output plot. The scope
can output to a printer through its parallel port.
Your LeCroy DSO can be controlled remotely through its IEEE-488
or RS-232 ports. As well as storage, printing and transfer to memory
devices, the scope offers push-button transfer of waveforms and
settings to the LW series of arbitrary waveform generators. This
enables, for example, a reference waveform to be captured from a
known good device and used as a test stimulus applied to other
devices.
Part 2 introduces the scope’s main features and
runs through them with you. You’ll get a basic
idea of what the instrument can do and start
working with it quickly and effectively.
Following this, you’ll be ready to go on to
Part 3, and to connect your own signals to
the scope.
For complete details on all features of your
LeCroy
color
digital
oscilloscope,
see
the
accompanying 2SHUDWRU·V0DQXDO.
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The main controls you’ll be using here:
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—acquires and displays repetitive signals in less than two seconds.
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— for the unique Analog Persistence feature: each persistence
data map is displayed in various intensities of the trace color.
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— expands the waveform and grid to fill the entire screen.
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— includes trigger-mode, -level and -position selection, as well as
TIME/DIV control.
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— turns the input channels on and off, and controls the OFFSET and
the vertical sensitivity for input channels. The VAR button, also in this
group of controls, gives variable, fully calibrated sensitivity throughout
the scope’s range.
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— the dark-gray menu-entry buttons that dominate this group access
the main on-screen menus and the acquisition, processing, and
display modes. The two knobs adjust menu values and command
cursors.
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— seven buttons and two knobs that control on-screen menu
selection. Each controls the menu to its immediate left on the screen.
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— allows the selected trace to be moved and expanded or have a
mathematical operation applied to any of the scope’s channels or
other Zoom/Math functions.
Before powering up, check that the local power
source corresponds to the scope’s range — any
AC power source of 90–250V, 50 or 60 Hz. (See
the 2SHUDWRU·V0DQXDO for Safety details.)
Use the cable provided to connect to the power source.
Then turn on the scope by pushing the POWER button at the
bottom left-hand corner of the front of the scope.
Before a display appears, the instrument will perform hardware and
software self-tests, followed by a full system calibration. The front-
panel ‘standby’ LED light, located below the right-hand corner of the
screen, will be illuminated during this sequence. The full testing
procedure will take approximately ten seconds, after which the
display will appear. before powering up.)
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To initialize the scope to its default settings and
make your screen displays similar to those shown
on the following pages:
First, press
on the control panel, illustrated on the
facing page.
A column of menu boxes like the one shown here will appear at right-
of-screen. Either “Recall” or “Save” will be highlighted.
Press the top menu
button to select “5HFDOO”.
Now press the “FROM DEFAULT SETUP” menu
button.
Note: When a word or
number is highlighted on-
screen, front-panel controls
will apply to the function,
action or trace represented.
Each menu button in the
column of buttons running
down beside the screen
corresponds to the menu
immediately next to it.
The individual buttons
illustrated three-
dimensionally in this
drawing are those used for
the actions described here.
Throughout the guide, 3-D
buttons and knobs that
punctuate the text
represent particular controls
to be used, while the group
illustrations show where
they are found on the front
panel.
With the scope initialized, we’re ready to explore
some of its basic functions.
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Connect a BNC cable from the CAL output at right to the
Channel 1 (CH 1) BNC input at left.
We can now go on to acquire and display waveforms.
Press the blue
button.
This will automatically set the trigger-level, timebase and vertical
settings needed for displaying the input signal.
The screen will show a 1 kHz square wave. Both Channel 1 (the
square wave) and Channel 2 (the horizontal line) are displayed.
Channels’ time and volts per division are shown in the trace labels at
top-left of screen.
Note: Auto Setup is a
particularly useful
feature that facilitates
the display of a wide
range of repetitive
signals, including
those with duty cycles
as small as 0.1 %.
To switch off a channel — Channel 2 in this example:
Press the corresponding TRACE ON/OFF
button,
located on the CHANNELS control panel.
This action removes both the trace and its label from the screen.
knob to adjust
the timebase.
The selected time/division setting is
shown on the lower left-hand side of the
screen.
Now, to capture the signal for a shorter
period,
change
the
setting
to
0.2 ms/div.
But make sure to reset it to
0.5 ms/div for the remainder of these
exercises.
The VOLTS/DIV controls give a vertical gain selection of 2 mV–5
V/div, operating in a 1–2–5 sequence. To reduce the sensitivity:
Turn
and set the gain to 500 mV/div. The selected
volts/div setting is shown in the Channel 1 trace label.
To fine-tune the vertical gain: Press the
button.
Turn
through several complete rotations, so that
the entire signal reaches from top to bottom of the grid.
The volts/div setting still shows in the trace label
Filling the grid in this way ensures that the signal uses the full range
of digitizing levels available — 8 bits = 256 levels — for the best
vertical resolution.
To return the vertical gain to its 1–2–5 sequence: Press
again.
The
knob controls the vertical position of the acquired
race.
Note the ground marker for Channel 1,
, next to the menus.
Press
to see that its channel, too, has a trace label.
Press again to turn off Channel 2.
When more than one trace is displayed on the screen, the number of
the selected trace is highlighted on its respective trace label. The
vertical controls — including VOLTS/DIV, OFFSET and COUPLING
— will operate for this trace only.
To choose another trace: Press the desired SELECT CHANNEL
button, to which the controls will then apply.
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The
knob adjusts the trigger’s
horizontal position — from 0 % to
100 % pre-trigger, and from left- to
right-hand edge of the grid. This knob
can also be used for setting the post
trigger in seconds up to 10 000
divisions.
The trigger position is shown by
at
the bottom of the grid.
The
knob adjusts the trigger’s
vertical threshold.
Arrows on either side of the grid,
,
indicate the threshold position — arrows
that are only visible if the trigger source is one of the traces on the screen,
and then only if that trace input is DC-coupled.
The smaller knobs on
the scope’s front
panel are
acceleration-sensitive
— the faster they are
rotated, the greater
are the increments
that result.
To expand — or ‘zoom-in’ on — a small section of the trace so that
it can bee seen in more detail:
Press
Then press the corresponding
to select “'XDO” from
the “Grids” menu.
Now two grids are shown on the screen,
giving optimum viewing of the expanded
trace.
Note: The Zoom
function is an
important benefit of
the scope’s
acquisition memory. It
can also be
considered as an
additional timebase
providing alternative
sweep speeds.
to turn on Trace A .
Turn
to adjust the expansion factor and increase the
amount of zoom.
Turn
to move the expanded part of the upper trace.
Turn
to expand vertically.
Note that the
expanded part of the
upper trace shows
the section of the
original waveform
being viewed by the
zoom.
Vertical and
Horizontal settings for
the zoomed waveform
are shown in the “$”
trace label.
and use the respective
s to select:
“&XUVRUV”, “7LPH” and “$EVROXWH”.
Use the upper
‘cursor position’ knob to move the
cursor.
The Absolute Time cursor appears as a
cross-hair on the waveform. As the
cursor moves, its time value in relation
to the trigger point shows at the base of
the lower grid, while indicated in the
trace labels is its voltage/amplitude
value.
Note: Use cursors to
make fast, accurate
measurements and
eliminate guesswork.
(See the Operator’s
Manual and Accurate
Measuring with
Cursors in Part 3 of
this guide for more
about cursors.)
Press the corresponding menu
button to change the
selection from “Absolute” to “5HODWLYH”.
Now two cursor menus are available, operated by
the upper and lower knobs, respectively.
The Relative Time cursors appear as
vertical arrows on the waveform.
Shown below the grid is the relative time
difference between the cursors, while
the
trace
labels
show
the
voltage/amplitude difference.
Press the top menu
button to select “3DUDPHWHUV”.
Note: The scope’s capacities
go beyond cursor
measurements to calculate
useful pulse parameters —
automatically and with high
precision. This saves time, as
cursors need not be positioned
manually, nor do time and
voltage values need to be
estimated.
Appearing on-screen below the grid is a list of five different voltage
parameters.
Press the corresponding
buttons to select from the
“mode” menu “6WG9ROWDJH” and, next, “6WG7LPH”.
The list of voltage parameters on-screen will be changed by these
selections. The parameters are computed each time the trace is
updated.
Press the corresponding
to select “2Q” from the
“statistics” menu. You will now see the average lowest and highest
values of each parameter and the standard deviation of the
distribution of measurements.
To return to normal operation: Press the top
to select
“2II”.
The “statistics” menu is
very useful for tracking
drift or other changes in
signal behavior.
to turn off Trace A and the ZOOM function.
Press
to turn on Trace C and ZOOM on it.
Now press
The menus shown here will appear:
Use the Summed
Averaging function to
improve the vertical
resolution of repetitive
signals, or to average out
unwanted noise on a live
signal.
These menus will appear:
Press the corresponding
to select “
Note: Fast Fourier Transform
(FFT) allows acquired
waveforms to be converted into
frequency-domain traces,
revealing valuable spectral
information that would
otherwise be impossible to
detect on a time-domain
record.
Press the corresponding
to select “REDEFINE &”.
And then press those
s that will make the selections
highlighted on the screen below.
The lower trace will show the FFT transform of the square wave
on Channel 1. Now, you can use the absolute horizontal cursor to
make a frequency measurement...
But first, press
Then press the corresponding
to select “$EVROXWH”
from the “type” menu.
Move the cursor to the right of the upper trace until it
reaches the FFT trace.
Note that the readings are now labeled in Hz (horizontal) and
dBm (vertical).
The first frequency component at left-of-screen should be the
square wave’s fundamental frequency (1 kHz). The following
components (3 kHz, 5 kHz, 7 kHz...) are the harmonics that
contribute to building the square wave.
To return to normal operation: Press the top
to select
“2II”.
Now press
to return to normal
triggering.
:DYHIRUP6WRUDJH
The scope has four waveform memories: M1,
M2, M3 and M4. In this example, the waveform
will be stored in M2.
Press
to turn off Trace C and FFT.
Now press
Then
press
the
respective
s
to select “” from the “store” menu, “0”
Note: Waveform
memories allow the
temporary saving of
waveforms for later
comparison or analysis —
an important benefit of
digital oscilloscopes.
from the “to” menu, and “DO STORE ( – > 0)”.
Then press
to display the
stored trace.
Then press the
s to select
“0” from the “from Memory”
menu, and “DO RECALL ( – > 0)”.
And press
to turn off
Trace A.
Note: As many as four
waveforms can be saved
and stored until overwritten
by other waves or the scope
is switched off.
Trace A displays the
waveform saved in M2,
which can then be
repositioned and expanded
using the ZOOM controls.
s to select “6DYH” and for “TO SETUP 1”.
Now, as an exercise, randomly change Channel 1’s
Change
and the Timebase, too.
Press the
to select “5HFDOO”, for the original
settings.
Finally, press the
for “FROM SETUP 1”.
Note: Entire panel
setups, such as those
of often-performed
measurements, can be
saved and stored in
non-volatile internal
memory for later recall.
Up to four setups can
be stored (thousands
with the optional DOS-
compatible memory
card, floppy or
removable hard disk).
The tutorials in Part 3 show you how to
perform
the
most
common
types
of
measurements.
As in Part 2, the tutorials take a practical,
step-by-step approach to famliarizing you
with the use of your LeCroy color digital
oscilloscope.
C
A
P
T
U
R
E
V
I
E
W
A
N
A
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Y
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First, the initial, basic steps for most measurements...
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67(3
Note: At power-up the scope
remains set to the last-used
setup. After the Reset in Step
1 (not to be confused with use
of the RESET button, which is
only for ZOOM + MATH), it
reverts to its default power-up
settings, with both Traces 1
and 2 activated.
The traces shown depend on
the previous setup and are
switched on or off using the
corresponding TRACE
ON/OFF buttons. When CH 1
is switched off, Channel 2
alone will remain activated —
as shown here.
Connect the signal to be measured — for example, the calibrator
(CAL) — to the Channel 2 BNC input (CH 2).
Reset: press
, the top
and
simultaneously.
Then press
to turn off Trace 1, and display:
Note: The coupling must be
well adapted to avoid
reflections at input to the
oscilloscope. COUPLING, like
most of the vertical controls,
applies only to the selected
channel (highlighted on-
screen).
Press
Then press the corresponding
to select from the
‘Coupling’ menu the coupling matching the source’s
impedance — 50 Ω in this case.
The screen will display:
These three basic steps will be repeated as a
prelude to performing most of the described
measurements that follow...
The scope’s eight-bit analog–to–digital converter
(ADC) offers 256 levels of quantization. Acquisition on
all levels gives the best digitizing: the digitized signal
covers all eight screen divisions without going off-
screen (‘clipping’). Here’s how best to digitize on all
eight bits.
Connect the signal to be measured — a 1 MHz, 100 mV (peak-to-
peak) triangle wave — to CH 2.
Reset: press
, the top
and
simultaneously.
Then press
to turn off Trace 1.
Press
, then the corresponding
to select from the
“Coupling” menu the coupling matching the source’s impedance
— 50 Ω.
Press
again.
Note: The signal’s amplitude
is acquired on approximately
six divisions, corresponding to
5/8 = 192 levels or 7.32 bits of
quantification used.
67(3
The screen will display:
Use
to adjust the channel input sensitivity and
have the signal fill all eight divisions of the screen.
And to even more finely adjust the sensitivity, press
7LSV: Changing the sensitivity using the VAR button will
give a non-rounded gain — for example, 12.8 mV/DIV.
Determining the amplitude of the signal by reading visually
from the screen can be difficult. To avoid reading errors, use
CURSORS (see Accurate Measuring with Cursors, page
3–16).
A major advantage of DSOs is the capacity to
accurately measure acquired data using standard
parameters.
Your scope offers a selection of Voltage and Time
parameters, as well as parameter customization.
This tutorial shows how standard parameters are
displayed to characterize pulses vertically and
horizontally. Automatic parameter measurement
and
statistical
values
thus
become
easily
obtainable.
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Connect the signal to be measured — for example, the CAL
signal with the shape selected as “pulse (25 ns)” — to CH 1.
, the top
and
simultaneously.
Then press
to turn off Trace 2.
Press
, then the corresponding
to select
from the “Coupling” menu the coupling matching the
source’s impedance — 50 Ω.
Press
again.
The screen will display:
to select “3DUDPHWHUV”.
The screen will display:
67(3
Next, press
The five main vertical parameters of the last acquisition,
displayed beneath the grid (see previous screen):
SNSN
the difference between maximum and minimum
data values
PHDQ
the average of data values
VGHY
the standard deviation of the data values from the
mean value
UPV
the square root of the sum of the squares of the
data values divided by the number of points
DPSO
the amplitude with noise and overshoot resistant
estimator (amplitude = top base).
67(3
Now, press
to select “6WG 7LPH” from the “mode”
menu.
The five main horizontal parameters of the last pulse,
displayed beneath the grid (next screen):
SHULRG
the duration of a full cycle at 50% crossings
ZLGWK
of the first <50 pulses (+ or –) in the analyzed
region
ULVH
the transition time on the rising edge for 10–90%
amplitude
IDOO
the transition time for the falling edge from 90%–
10% amplitude
GHOD\
the time from the trigger (or t=0) to the first 50%
transition.
Note: Acquiring just one pulse
does not permit measurement
of a signal period. Therefore,
the period parameter is not
calculated and no value is
displayed.
7LSV: In order to perform the parameter calculation on a
particular section of the signal, adjust the left and right cursors
using the upper and lower knobs, respectively, on the SYSTEM
SETUP part of the front panel.
On the screen below an area of interest has been selected for
measuring the time of the pulse’s falling edge, as indicated by
“delay ()”:
Note: The number of points
used to calculate the
parameters is shown in the “to”
menu.
67(3
67(3
Use the
s to reselect the entire trace as the area of
interest, as described in the 7LS on the previous page.
Then press the corresponding menu
to select “2Q”
from the “statistics” menu.
Four different values are displayed for each parameter: average
value; lowest value; highest value; and sigma, the standard
deviation of the data values from the mean value. In order be sure
of the statistics obtained, you will need to perform a number of
acquisitions.
Note: The sweeps number
shown immediately under the
grid is the number of
acquisitions to which the
statistics calculated and
displayed apply. To restart the
statistics calculation, press the
CLEAR SWEEPS button. Only
the future acquisitions will be
included in the calculation.
All these parameters are
readable from a PC linked to
the scope by GPIB or RS232
remote control using the
“PArameter_VAlue?”
query.Also possible, using
Custom Mode, is the selection
of five different parameters
(even more with the WP03
package) relating to a variety of
traces or memories between
the available standard
parameters.
Finally, press
A variety of cursors of two basic types are used
with your LeCroy color DSO. In Standard Display,
Amplitude (Voltage) cursors are lines moved on
the grid to measure the amplitude of a signal. And
Time (Frequency) cursors are markers moved
along the waveform that can be placed at a
desired time to read the signal’s amplitude at that
time.
For details of cursor behavior in the different
cursor
and
display
modes,
see
the
2SHUDWRU·V0DQXDO.
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Connect the signal to be measured — for example, the
calibrator (CAL) — to CH 1.
67(3
Reset: press
, the top
and
simultaneously.
Then press
to turn off Trace 2.
, then the corresponding
to select
from the “Coupling” menu the coupling matching the
source’s impedance — 50 Ω.
Press
again.
Turn
to adjust the timebase,
to fill
the screen with the signal.
Press
to halt the scope and display:
Note: Pressing SINGLE is a
smooth way of stopping the
scope to allow
measurement of the
waveform captured on-
screen.
to select “&XUVRUV”.
(“$PSOLWXGH” and “$EVROXWH” will show as the default
selections in the “mode” and “type” menus, respectively.)
The screen will display:
67(3
Turn
corresponding to the “cursor Position” menu, to
move the Absolute Amplitude cursor to the top of the signal.
Note: In Absolute Amplitude
Mode, selected here by
default, a single cursor bar in
the form of a broken line is
displayed (in this example
shown placed at the very
bottom of the grid). The
vertical position of this bar on
the grid can be adjusted by
turning the corresponding
‘cursor’ knob. The difference
in amplitude, between the
cursor and the ground level
indicated by the “1” at right of
the grid, is shown in the trace
label at top left of screen.
The screen will then display:
Note: Amplitude cursors are
moved pixel by pixel up and
down the grid.
Here the difference in
amplitude between the
ground and maximum levels
of the square wave has been
measured and is shown in the
trace label.
67(3
Press the corresponding
to select “5HODWLYH” from the
“type” menu. This will activate the Relative Amplitude Mode and
display a pair of cursors.
The screen will display:
Note: In Relative Amplitude
Mode, two bars, the reference
and difference cursors, are
controlled to give readings
between the two in amplitude.
In this example, the reference
cursor, moved by turning the
upper knob corresponding to
the “Reference cursor” menu,
has been placed on the base
level of the square wave.
While the difference cursor,
adjusted using the lower knob
and “Difference cursor” menu,
has been positioned at the top
of the square wave — the
difference between the two in
this case giving the wave’s
amplitude, indicated in the
trace label.
67(3
7LSV: Press the corresponding menu button to select “Track
2Q” from the “Reference cursor” menu. Now, when the
reference cursor bar is moved using the upper knob the
difference bar will “track” it and the two lines will move in
tandem, remaining the same distance apart. However,
turning the lower, “Difference cursor” knob will change the
difference cursor position and the distance between the two
cursors. Pressing the same menu button as before will turn
off tracking.
Press the corresponding
s to select “7LPH” and
“$EVROXWH” from the “mode” and “type” menus, thereby
activating Absolute Time Mode.
The screen will then display:
Note: Time cursors are
markers moved to any point
along the trace and can be
used to measure time and
amplitude. The reference
point (t=0) is the trigger point
indicated by the vertical arrow
on the grid base. When the
markers are placed on a data
point, they change
appearance (see the
Operator’s Manual for a full
description). The Absolute
Time cursor is a cross-hair
marker. Here, the cursor —
highlighted to make it more
visible in this example — is
shown at the trigger point on
the rising edge of the square
wave.
67(3
Turn the
corresponding to the “cursor Position” menu
to change the position of the Absolute Time cursor.
The screen will then display:
The value measured
between the trigger point and
the Absolute Time cursor is
shown as the “Time” value
directly beneath the grid. The
(highlighted) cursor in this
example has been moved to
the falling edge of the square
wave.
67(3
Press the
to select “5HODWLYH” from the “type” menu
and activate Relative Time Mode.
Note: In Relative Time Mode
the cursors are a pair of
arrows that move along the
waveform. In this example,
the Reference and
Difference cursors —
upward- and downward-
pointing arrows — are shown
highlighted together at the
rising edge of the square
wave. Using the knob
corresponding to its menu,
either cursor can be moved
independently of the other to
any point on the trace. The
value representing the time
difference between the two
will appear below the grid,
while the amplitude
difference appears in the
trace label.
The screen will display:
Note: Here and in the
previous screen example,
the Relative Time Reference
and Difference cursors are
used to measure the period
and frequency of the
oscillations on the square
wave, with the result
displayed beneath the grid.
The Reference cursor has
been moved to the falling
edge of the square wave,
while the Difference cursor
has been placed at the
maximum level. Displayed in
the trace label when “'LII²
5HI” is selected is the gain
by division and difference in
amplitude between the two
cursors.
On the next screen the Relative Time cursors have been moved to
illustrate how they work:
7LSV: To display in the trace label each cursor’s absolute amplitude
relative to ground level: Press the menu button to select “'LII
5HI” from the “show” menu.
In this tutorial’s final screen, “'LII 5HI” has been selected,
displaying the amplitude values for each cursor:
Note: The absolute
amplitude values of the
Reference and Difference
cursors are shown in the
trace label respectively.
“Average” is one of the scope’s important and
powerful Math functions. Use it to reduce non-
systematic noise and improve the signal–to–noise
ratio. Here’s how.
$SSOLFDWLRQ6HWXS
Connect the signal to be measured — a 33 kHz, 1.0 V (peak-to-
peak) square wave with noise — to CH 2.
67(3
67(3
67(3
Reset: press
, the top
and
simultaneously.
Then press
to turn off Trace 1.
Press
, then the corresponding
to select
from the “Coupling” menu the coupling matching the
source’s impedance — 50 Ω.
Press
again.
The screen will display:
67(3
67(3
Press
Press the corresponding menu
to select “'XDO”
from the “Grids” menu.
The screen will now display:
67(3
67(3
67(3
Press
Press the corresponding menu
to select “REDEFINE $”.
Press the corresponding menu
to select “
Note: A choice of types of
acquired signal averaging is
available on the “Avg Type”
menu. The summed average
gives all averaged data the
same weight. While the
continuous average can be
set up to give data different
weights —for example, the
most recent acquisition could
be given greater importance
in the average calculation
ratio defined by the user.
The desired number of
sweeps— acquisitions taken
into account in the averaging
— can also be selected using
the corresponding menu
button. Here: an average of
1000 acquisitions is selected
from the “for” menu. Any trace
can be averaged: CH 1, CH 2,
CH 3 or CH 4; Trace A, B, C,
or D, or Memory 1, 2,3 or 4.
Press the corresponding menu
to select “$YHUDJH”
from the “Math Type” menu.
Now, press
to turn on Trace A.
The screen will display:
And
(SYSTEM SETUP) to restart Averaging.
The last screen shows the final result of the averaging of 1000
acquisitions. Non-systematic noise has been greatly reduced, as can
be seen from a comparison of a single CH 2 acquisition with the
1000-acquisition averaged result on Trace A.
Note: With Trace A
on, the sweep counter
in the Trace A label at
mid-left of screen will
mount until the
number of sweeps
reaches that selected.
In the meantime, the
intermediate result of
the average is
displayed (“216
swps”, as shown on
the previous page).
Once the selected
sweeps number is
reached, calculation
stops and the final
result of the average
is displayed, as here.
points from numerous acquisitions makes it
easier to view signal changes over time. But
Analog Persistence, with intensity grading,
makes this even easier by signifying the most
frequent signal path ‘three-dimensionally’. Here’s
how to use this unique feature to reveal the AM
modulation of a sinewave.
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Connect signal to be measured — an AM modulation of a
2 MHz sinewave with 100 kHz squarewave — to CH 2.
67(3
67(3
67(3
Reset: press
, the top
and
simultaneously.
Then press
to turn off Trace 1.
Press
, then the corresponding
to select
from the “Coupling” menu the coupling matching the
source’s impedance — 50 Ω.
Press
again.
Note: The AM modulation
signal has a stable trigger.
However, in the final periods
the signal shows a number of
jumps. Without LeCroy’s unique
Analog Persistence feature, it’s
not easy to characterize these
modulation variations in the
normal display mode.
67(3
The screen will display:
Now press
The screen will display:
Note: Modulation time
variations appear clearly in
Persistence Mode. Because its
source is a squarewave signal,
the modulation shown here has
different states. The number of
acquisitions included in the
display (up to one million) is
shown beneath the trace label.
In this example, 1939 sweeps
have been captured in a short
delay to obtain the result
displayed. The most recent
sweep is shown as a bright
vector trace.
The Analog Persistence feature
is also available in XY and
Sequence Modes.
67(3
Press the
for “Persistence Setup”.
Note: The “Persist” menu
offers the means to apply
persistence to all displayed
traces, or merely the top two,
when more than one trace is
displayed. Information on
each trace will be shown in its
respective trace label at left of
screen. When “Top 2” is
highlighted in the menu, this
relates to the first- and
second-from-top labels that
will appear with each
additional trace — very useful
when four traces or functions
are shown on-screen and
persistence will not be applied
to all.
The “Persist for” menu offers
a choice of persistence
duration in seconds. If the
duration is set — for example
— at one second, each
acquired trace will be
displayed for a second and
then deleted.
The default value for this
menu is “,QILQLWH”.
The screen will then display:
7LSV: Persistence Mode can be cleared and reset manually by
pressing the CLEAR SWEEPS button, or by changing any
acquisition or waveform processing condition.
Note: The image displayed
shows the changes in the
sample event over time.
Statistical integrity is preserved
because the decay is
proportional to the persistence
population for each amplitude
or time combination in the data.
The brightness level of a single
color is used to denote signal
intensity. Particular populations
are given distinguishing shades
of color. These are dynamically
updated as data from new
acquisitions are accumulated.
Population distributions in rare
events can be highlighted by
additional saturation, as
illustrated in the screen at right.
Then turn the lower ‘menu’
to adjust the value of the
saturation to 10 %.
The screen will display:
Note: By default, the most
recent sweep is shown as a
bright vector trace on top of the
persistence display. This menu
allows to show or not the last
trace on top of the persistence.
Press the corresponding menu
to select “2II” from
the “Last Trace (show)” menu.
The screen will display:
Note: Instead of the brightness
of a single color as used by the
Analog Persistence feature,
Color Graded Persistence uses
a color spectrum from red
through violet to map signal
intensity, as shown in this
example*.
Press the corresponding
to select “&RORU *UDGHG”
from the “Using” menu.
The screen now displays:
* As this guide is printed in black & white only, references are to
monochrome renditions of the colors evident on your screen.
The scope’s powerful and intelligent use of color
strongly links displayed waveforms and their
data. This color association simplifies the viewing
of information — especially in analysis of related
signals
or
signal
parts.
Here’s
how
color
association handles multiple long-waveform zooms
(see also Calculating on Long Waveforms).
$SSOLFDWLRQ6HWXS
Connect the signal to be measured — which can be a waveform
of one million points or more — to CH 2.*
67(3
67(3
Reset: press
, the top
and
simultaneously.
Then press
to turn off Trace 1.
Press
, then the corresponding
to select
from the “Coupling” menu the coupling matching the
source’s impedance — 50 Ω.
* Acquisitions of up to eight million points can be made,
depending on the scope model.
to stop the acquisition. Then
to access
the “TIMEBASE” menus.
Shown at the top of the TIMEBASE menus on the following screen is
the number of points acquired — 50 000 samples in this example. At
the same time, the “Record up to” menu displays the acquired
sample limit set by the user — “50k”.
Turn the lower ‘menu’
so that the “Record up to” number
of samples is set to at least “1M” points — for this example it is
set to “2M”.
Turn
in order to slow down the timebase, and
obtain more time per division, until the number of acquired
points displayed is the same as in this example — “2M” points.
Press
to perform a single two-million-point
acquisition and display:
Note: With the long acquisition
memory, the maximum
sampling rate is maintained at
many more timebase settings
than are possible with short-
memory scopes. Particular
advantages include:
— greater waveform detail
— high zoom factor
— protection against aliasing
— improved time resolution
— wider frequency spectrum.
(See LeCroy’s Application Note
ITI 008 for details).
Note: Functions or zooms can
be selected on any channel or
trace. The scope allows display
of four different traces in as
many grids, while preserving
eight-bit resolution.
67(3
The following steps directly illustrate the extreme practicality of the
color association system, as different parts of an acquired signal are
simultaneously expanded and viewed.
Press
to make appear the “DISPLAY SETUP” group
of menus.
Then
to select “4XDG” from the “Grids” menu.
The screen will display:
Now, press
Note: After Step 8 has been
taken, Trace A will be displayed
as the zoom (“use Math?” “1R”)
of CH 2, as indicated in the
“Trace $is ZOOM of” menu
(“”).
67(3
Press the corresponding menu
for “REDEFINE $”.
Next, turn the lower menu
to select “”.
Then press
to turn on Trace A.
The screen will display:
Use
with
and
with
to make
the original signal selection, and select the timebase
(horizontal zoom) with amplitude (vertical zoom). This allows
the selection of a part of the original signal and the part’s vertical
or horizontal expansion.
Note: The selected section is
shown on the original trace as
reinforced video. The RESET
button cancels all the zoom
changes and redisplays the
original trace.
The screen will then display a 10x zoom of CH 2 that indicates a
zone of interest:
67(3
Repeat Steps 8 and 9, this time turning on Traces B and C to
zoom other parts of CH 2.
The screen will display:
67(3
Then
and
to display the four grids in Full
Screen mode without menus.
The screen will display:
7LSV: As shown on the next screen, each of the four grids can
be shown with its own trace and parameters — up to five at
once — simultaneously.
And then the
to select “More Display Setup” from
“DISPLAY SETUP”.
Next, press the
to select one of the pre-set numbered
color schemes from “Color Scheme”.
In this example, “Color Scheme” “” has been selected:
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Now, press the
to select “8” from “Color Scheme”.
This allows the creation of a custom color palette.
7LSV Copy preset schemes to user palettes. These can
then act as references and form the bases for choosing
object colors in new customized color schemes.
The screen will display:
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Now, press the
for “CHANGE COLORS”, and then for
“COPY SCHEME 1 to U1”.
The colors assigned to the objects in “U1” will now be the same
as those of the pre-set “1”.
Next, press a
to select an object for color change.
Here, Trace B is selected.
And then a
to select the color of the object selected.
“Grass Green” has been selected to replace “Pale Blue” in the
following example.
Note: See the Operator’s
Manual for a description of
the displayed objects whose
colors can be modified.
The screen will display:
And in the final screen on the next page, “Text & Menu” has been
selected and colored “Yellow”.
acquisition, offering a choice of fixed-size,
complete-waveform segments without unwanted
deadtime (see Appendix A in the 2SHUDWRU·V
0DQXDO for the limits).
The long intervals of deadtime that often separate
consecutive single-shot events are minimized in
sequence mode. Complicated event sequences
covering large time intervals are captured in fine
detail — without the uninteresting periods
between.
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Connect the signal — a pulse train (each group of 12 pulses
separated by a long signal that need not be acquired) — to
CH 2.
, the top
and
simultaneously.
Then press
to turn off Trace 1, and display:
Press
, then the corresponding
to select
from the “Coupling” menu the coupling matching the
source’s impedance — 50 Ω.
Press
again.
Turn
to adjust the timebase, and
to
adjust the gain and fill the screen with the signal.
This schema represents
how Sequence Mode
handles sequence
acquisition. The display is
activated pressing SHOW
STATUS and selecting
“Text & Times” from the
menu that appears.
Note: This screen shows only
one of 12 train pulses.
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The screen will display:
Again turn
to adjust the timebase, this time to
display all of the train’s pulses.
Now press
The screen will now display:
Note: The “TIMEBASE”
information shown at top-
right-of-screen, consists of, in
this example:
Timebase value — 2 ms/div;
Number of samples acquired
— 10 000;
Sampling rate — 500 MS/s;
Time between samples —
2 ns/point;
Total time acquisition —
20 ms.
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Again turn
to adjust the timebase, this time
until two pulse trains are acquired.
The screen will then display:
Note: As shown at top-right-
of-screen, the sampling rate
has decreased as the total
window time acquisition has
increased. Between two
trains, a long ground-level
signal of no interest has been
acquired.
Sequence Mode, activated at
the next step, is the best way
of acquiring the zone of
interest only.
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Press
Then press the corresponding menu
to select “2Q”
from the “Sequence” menu.
Next, turn the lower ‘menu’
to display “VHJPHQWV”
in the “Sequence” menu.
Press
Now in Sequence Mode proper, the screen displays:
Note: The number of trains
acquired is now four, with the
same sampling rate as for
two. The sole difference is
that now the duration between
two train pulses is half what it
was. In the trace label, at left-
of-screen, the symbol “2x”
indicates two segments
acquired in Sequence Mode.
The TIMEBASE information
shows that two segments of
50 000 points each
(“2 F 50 000”) have been
acquired.
7LSV: The bottom menu shows the maximum number of
points per segment — in this instance, 50 000. The sampling
rate or the total number of acquired points can be adjusted.
The timebase setting in Sequence Mode is used for
determining the acquisition duration of each segment —
10 x TIME/DIV. This setting, as well as the number of
segments desired, the maximum segment length, and the
total memory available, are used for arriving at the actual
number of samples per segment, and the time per point.
Here, the Sequence Mode timebase of 2 ms/div has been
selected (corresponding to a single train duration, as
already covered at Step 5). The sampling rate is the
maximum, and the two trains are captured with a very short
delay between triggers. The acquisition is in fact two
acquisitions, each a train of pulses.
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Turn the lower ‘menu’
to set the number of segments.
On the example screen overleaf, the number of segments is set
at eight.