ELAN Home Systems Video Gaming Accessories ES370 User Manual

ELAN DIGITAL SYSTEMS LTD.  
LITTLE PARK FARM ROAD,  
SEGENSWORTH WEST,  
FAREHAM,  
HANTS. PO15 5SJ.  
TEL: (44) (0)1489 579799  
FAX: (44) (0)1489 577516  
USBscope50  
USER’S GUIDE  
ES370  
All Trademarks are duly acknowledged.  
The USBscope50 is Patent Pending.  
REVISION HISTORY  
ISSUE PAGES  
DATE  
04.07.2005  
08.07.2005  
15.07.2005  
NOTES  
1
2
3
30  
30  
31  
FIRST ISSUE  
Various additional info & spec amendments  
Add support for Win98 & DBCS Language’s in  
2K/XP  
4
5
31  
39  
20.07.2005  
27.09.2005  
Various additional info & amendments  
General update. Explain trigger modes, Math,  
FFTs etc  
Elan Digital Systems Ltd.  
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Disclaimer  
This document has been carefully prepared and checked. No responsibility can be  
assumed for inaccuracies. Elan reserves the right to make changes without prior notice  
to any products herein to improve functionality, reliability or other design aspects. Elan  
does not assume any liability for loses arising out of the use of any product described  
herein; neither does its use convey any license under its patent rights or the rights of  
others. Elan does not guarantee the compatibility or fitness for purpose of any product  
listed herein. Elan products are not authorized for use as components in life support  
services or systems. Elan should be informed of any such intended use to determine  
suitability of the products.  
Software supplied with Elan PC-Cards, Compact Flash cards or USB devices is  
provided “as-is” with no warranty, express or implied, as to its quality or fitness for a  
particular purpose. Elan assumes no liability for any direct or indirect losses arising  
from use of the supplied code.  
Copyright © 2005 Elan Digital Systems Ltd.  
Federal Communications Commission (FCC) Statement  
This equipment has been tested and found to comply with the limits for a Class A digital device,  
pursuant to Part 15 of the FCC Rules. These limits are designed to provide reasonable protection  
against harmful interference in a residential installation. This equipment generates, uses, and can  
radiate radio frequency energy and, if not installed and used in accordance with the instructions, may  
cause harmful interference to radio communications. However, there is no guarantee that interference  
will not occur in a particular installation. If this equipment does cause harmful interference to radio or  
television reception, which can be determined by turning the equipment off and on, the user is  
encouraged to try to correct the interference by one or more of the following measures:  
- Reorient or relocate the receiving antenna  
- Increase the separation between the equipment and receiver  
- Connect the equipment into an outlet on a circuit different from that to which the receiver is  
connected.  
- Consult an Elan authorized dealer or service representative for help.  
Elan is not responsible for any radio or television interference caused by using other than  
recommended cables and connectors or by unauthorized changes or modifications to this equipment.  
Unauthorized changes or modifications could void the user's authority to operate the equipment.  
This device complies with Part 15 of the FCC Rules. Operation is subject to the following two  
conditions (1) this device may not cause harmful interference, and (2) this device must accept any  
interference received, including interference that may cause undesired operation.  
Listed Products  
The models covered by this installation guide are intended only for installation in Listed computers for  
use in business or home.  
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1 OVERVIEW  
The USBscope50 is a digital storage oscilloscope that has the  
following features:  
Single channel scope with BNC input and USB PC interface  
Each USBscope50 can be stacked to increase channel count (each  
requires its own USB connection)1  
300V Cat II isolation between BNC ground and USB ground2  
50MSample/sec single shot sample rate  
1GSample/sec equivalent sample rate3  
Timebase from 4ns/div to 4s/div in 1,2,4 steps  
75MHz 3dB analogue bandwidth4  
3000 sample points, 8-bits per sample  
Pre and post triggering, and trigger delay5  
AC and DC coupling  
Input sensitivities with x1 probe are 30mV/div, 300mV/div,  
3V/div and with x10 probe are 300mV/div, 3V/div, 30V/div  
1Meg input impedance, 16pF  
Channel offset control  
Auto and Normal hardware triggering with >, <, +, – modes  
Host powered from USB (200mA typ)  
Stacked configurations of 2,3 and 4 channels are supported  
Stacked configurations allow any channel to be trigger channel  
Stacked configurations have tight phase locking between channels  
Probe compensation output, 3V 1KHz  
Power/activity LED  
1 A stacking connector kit is required  
2 In stacked configurations the channels share a common ground at the BNC terminals  
3 Suitable to measure repetitive signals that are not phase locked with the internal acquisition clock  
4 Hardware trigger bandwidth is approximately 60MHz  
5 Only in single-shot mode  
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2 ABOUT THE USBscope50  
2.1 General  
The USBscope50 uses a 50MSample/sec 8-bit A-to-D converter.  
The A-to-D and front-end circuits that process the input waveform,  
and the digital stages that acquire and store the waveform are all  
powered from the USB host interface via an isolated supply. This  
means that there is no galvanic connection between the BNC ground  
(or BNC centre terminal), and the USB interface. When you  
measure a circuit and connect the scope ground clip to a voltage that  
is not at the same ground potential as the host computer, no current  
can flow and the host computer is therefore not forced to be at the  
same potential as the circuit under test. This clearly has major safety  
advantages. The USBscope50 has been designed so that up to 300V  
CAT II6, or 500V CAT I can exist between the scope ground clip  
and the host computer ground.  
Each USBscope50 can be used as an independent single channel  
scope but to enhance flexibility several USBscope50s can be stacked  
together to make a combined 2,3 or 4-channel device. In this case,  
each scope is synchronised with the others so that the compound  
device acts like a single multi-channel instrument.  
Each  
USBscope50 still needs its own USB connection and the combined  
device shares a common ground between all the BNC connectors i.e.  
the channels are isolated from the USB but not from each other.  
6 The CAT rating refers to how large a transient over-voltage may be when connected to the circuit in  
question. The USBscope50 is designed to handle a certain transient over-voltage between the BNC  
and the USB host i.e. across the internal isolation circuits. The CAT II UL rating defines a more  
severe environment than CAT I and hence larger transients are possible. This is why the isolation  
rating for CAT II is lower than the rating for CAT I. For further information on CAT ratings please  
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2.2 USBscope50 Architecture  
The figure below shows a simplified diagram of the USBscope50.  
STACK  
CONN  
AC/DC  
CONTROLLER  
BNC  
USB  
CONTROLLER  
USB  
COMP  
Trigger  
DATA  
PSU  
ATTENUATOR  
1Meg  
AMP  
8-BIT ADC  
ISOLATION BARRIER  
Figure 2.2-1 USBscope50 Architecture Diagram  
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2.3 Using More Than One USBscope50  
A unique feature of the USBscope50 architecture is that up to 4  
devices7 can be stacked to make a multi-channel instrument.  
In order to use a stacked configuration, you must purchase the  
stacking connector kit. This kit comprises 3 long lead connectors  
and 1 short lead connector as shown:  
2.3.1 Assembling The Stack  
To stack the USBscope50 devices, first be sure that none of them are  
connected to a USB port.  
Before you begin, put the short lead connector to one-side…you’ll  
use that one last.  
Now, insert one of the long connectors from the top of one of the  
scopes (it doesn’t really matter which one). Push the pins of the  
connector into the top of the stacking connector from the side where  
you can see the top of the black connector down inside the scope.  
Be careful when doing this, don’t use too much force or you may  
damage the connector pins. Push the long connector all the way in  
until it seats down on the scope’s internal connector. You should be  
able to see the gold pins about 2-3mm beyond the bottom surface of  
the scope. The connectors have no pin orientation…they can go in 2  
possible ways round…both are OK.  
7 Don’t stack more than 4, the software will reject this.  
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Repeat this for all except the last scope to be stacked.  
For the last scope in the stack, do the same as above but use the short  
length connector. This time, the pins are shorter so they stop well  
inside the scope’s case. This scope MUST be the bottom scope in  
the stack. The reason for this is that if you use the long connector,  
the pins could be shorted out accidentally, or you may touch the pins  
when the scope is connected to a high voltage and you could get an  
electric shock! Similarly, if you plan to use only one scope, make  
sure there is no stack connector fitted or the shorter connector type is  
fitted.  
This is a safety critical point so please note it carefully.  
Now you can assemble the stack.  
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Start with the bottom scope. Hold it in one hand, and put the next  
scope on top of the 1st, the same way around. Align the stacking  
connectors and when the stacking connectors are partly mated  
engage the front “P” shaped clip (BNC end) on the 2nd scope into the  
“P” shaped slot on the 1st scope.  
Now, bring the back edge “P” clip (USB end) of the 2nd scope down  
until it clicks into the 1st scope’s slot. These two scopes are now  
mated.  
Check that as you pushed the 2nd scope down, the stack connector  
has not been forced upward…if it has simply press it down until it  
seats correctly (see picture above for a guide as to the normal  
exposed connector depth after stacking). Repeat this for each  
remaining scope, adding each one on top of the previous one.  
The scopes are now stacked.  
2.3.2 Disassembling The Stack  
Start with the top scope in the stack. Grasp the stack in one hand  
and with the other hand’s thumb and forefinger, pinch between the  
interface between the top two scopes, near the back “P” clip (USB  
end). With moderate force, the top scope will pop up and come free.  
Remove the stacking connector from the free scope.  
Repeat this for all scopes in the stack.  
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2.3.3 USB Connections For Stacked Configurations  
All stacked scopes need a USB connection. A standard hub may  
be useful for multi-channel stacks to get enough USB ports.  
Each scope needs about 200mA. Plugging more than 2 scopes into a  
hub will mean that the hub may need to be powered externally.  
Please refer to the hub’s documentation for more details about the  
power available per port.  
2.3.4 Software For Stacked Configurations  
When you run USBscope50, it will automatically detect the scopes  
connected via USB and will also check to see if the scopes are  
electrically connected together via the stack. It will then initialise all  
connected scopes, one at a time. This may take a few seconds.  
If you stack several scopes but forget to connect say one of the  
scopes to a USB port, the software will warn you and will not run.  
The software will display a channel “tab” for each scope in use.  
The channel number allocated to each scope depends on its serial  
number, so the order you stacked them will almost certainly NOT be  
the same as the channel order allocated by software.  
To find out which scope is Channel 1, use the CH1 tab and click the  
“id” button.  
The LED on that scope will blink rapidly for about 4 seconds, or  
until you click the button again.  
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Repeat this for each channel in the stack to identify them.  
If you like, you can stop the software, and unplug all the scopes from  
their USB connections, and then re-stack them in their channel order.  
The “about” tab lists all the scopes that have been found. Click on  
any of the scopes in the list to see more information and an  
explanation of items in the list.  
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2.3.5 Stacking Do’s And Don’ts  
Do power off all scopes (remove USB lead) before connecting  
and disconnecting scopes from the stack  
Don’t remove any scopes from the stack while the software is  
running  
Don’t remove any scopes from the stack while any of them are  
powered  
Don’t stack several scopes and leave one or more scopes un-  
stacked…this configuration will ignore the un-stacked scopes  
Don’t short circuit any of the stack connector pins, or bend the  
pins or use excessive force trying to mate the connectors  
Don’t probe or drive any of the stack connector signals  
Avoid touching the stack connector pins/signals during  
stacking  
Do make sure that each stack connector is properly seated in  
place before trying to stack another channel on top  
Don’t allow water or dirt etc to enter the scope via the stack  
connector access hole  
Do remember that scopes in the stack are NOT isolated from  
each other, they are only isolated from the USB ports. To  
re-iterate, stacked scopes have their BNC connector bodies  
connected together through the stack connector.  
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2.4 Input Ranges  
The USBscope50 supports 3 settings on its input attenuator.  
The ranges at the BNC input depend on the type of scope probe  
used:  
A “x1” probe causes no signal attenuation and will result in nominal  
full-scale input ranges of +/-0.3V, +/-3V and +/-30V. The  
bandwidth of x1 scope probes is generally quite low (10’s of MHz)  
and the circuit being measured will see a 1MegOhm load.  
A “x10” probe causes a factor of ten signal attenuation and will  
result in nominal full-scale input ranges of +/-3V, +/-30V and +/-  
300V. The bandwidth of x10 scope probes is generally high (100’s  
of MHz) and the circuit being measured will see a 10MegOhm load.  
The USBscope50 also supports AC and DC coupling:  
In AC coupling mode, the input signal is passed through a capacitor  
prior to attenuation. The input bandwidth is around 3.4Hz up to  
75MHz.  
In DC coupling mode, the capacitor is bypassed and the bandwidth  
is DC up to 75MHz.  
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2.5 Probe Compensation  
Before taking measurements with the USBscope50, the attached x10  
scope probe must be compensated to ensure that it is matched to the  
scope input stage8.  
This ensures that the probe+scope act together to keep the input  
frequency response as flat as possible. Using a scope probe that has  
not been adjusted to match the USBscope50 can lead to inaccurate  
readings for higher frequency signals.  
The USBscope50 includes a probe compensation output9.  
This must be turned on using the USBscope50 software. Once  
enabled, the compensation output is a 0 to 3V (approx) square wave  
with 50% duty cycle and 1KHz frequency. Note that the  
compensation output will switch off automatically when you close  
the channel’s tab10.  
The USBscope50 can work with scope probes that list an adjustment  
range that includes 16pF. It is best to use probes that have a range  
that puts the 16pF point near the middle of the range, for example  
the HP10071A type probe lists an adjustment range of 9-17pF and  
our tests show that whilst it is easy to compensate this probe against  
the USBscope50, the trimmer in the probe body is certainly quite  
close to the top end of its range. There are many probe choices on  
the market, and lots of them list ranges that span 16pF.11  
To compensate your probe follow these steps:  
1. Connect your x10 probe to the USBscope50 software and run  
the USBscope50 software  
8 This does not apply to x1 scope probes  
9 Later models have a dual pad compensation point that includes a GND pad  
10 This is to avoid the fast edges of the square wave possibly coupling into your measurement  
11 Some very high frequency low capacitance probes may not be suitable for use with the USBscope50  
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2. Set the input range to 0.3V/div, x10 probe and coupling to  
AC  
3. Use the channel tab and click on the “cmp” button to turn on  
the compensation output  
4. Set the timebase to 100us/div, and set “auto” triggering, with  
the trigger level set to about 0%.  
5. Now connect your probe tip to the compensation output on  
the scope. You should see a square wave something like this  
or it may look more like this  
6. You may find you need to connect the ground clip to either  
the BNC ground or use the GND pad near the compensation  
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output12 to achieve a clean waveform with minimal mains  
“hum”  
7. Now, slowly adjust the trimmer in the probe body until you  
achieve the best square wave shape that you can. By this we  
mean nice square corners and minimum over and under shoot  
near the edges. A small amount of over shoot is preferable to  
an adjustment with “curved” square wave corners: this would  
mean that the scope will attenuate high frequency signal  
components whereas a small amount of overshoot will mean  
that the scope will tend to slightly amplify high frequency  
signal components. A typical trace, after compensation will  
look  
like  
this.  
Some deviation from this is normal due to variations in probe  
performance. It is possible that on lower cost, lower  
bandwidth probes that you may see a larger amount of  
overshoot near the edges. This overshoot may be very  
narrow and seem to come and go…this is normal. Better  
quality scope probes have better transient response and so  
have smaller overshoot.  
12 Be careful not to short-circuit the GND pad to the COMP output with the ground clip. A momentary  
short circuit is not harmful but leaving a sustained short may damage the scope’s output  
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2.6 Acquisition Modes  
The USBscope50 can acquire waveforms in two different ways. The  
mode and sample interval (i.e. the time between each data point) is  
displayed on the main panel  
2.6.1 Single Shot  
In this mode, the ADC is clocked at up to 50MegaSamples/sec.  
Each sample is placed into the buffer and then the buffer is painted  
on the screen.  
This mode is the one to use for non-repetitive signals i.e. single  
pulses, irregular bus events etc. It can also be used for repetitive  
waveforms.  
For practical purposes the maximum frequency sine wave you can  
resolve is about 10MHz in this mode, giving just 5 sample points per  
cycle: expect to see a very “jagged” and “triangular” looking  
waveform when observing a 10MHz input! Drop the input  
frequency down to say 1MHz and you will see a nice smooth  
waveform.  
In single shot mode the timebase can be set from 200ns/div all the  
way up to 4s/div. The time to acquire the waveform gets noticeably  
slower when rates above 40ms/div are selected: the total acquisition  
time is approximately “30 x timebase” so at 4s/div, the display will  
update once every 120s, or 2 minutes !  
As with all digital storage scopes, be careful not to view a high  
frequency waveform on too low a timebase. You may see a  
waveform that looks correct but drifts or fluctuates over time, and  
that has the wrong frequency…this is called aliasing and is quite  
normal. To avoid this effect, always pick the fastest single shot  
timebase consistent with being able to view the waveform in  
question.  
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2.6.2 Random Interleaved Sampling  
This mode is a little more complex and is suited only to observing  
certain types of waveform.  
The USBscope50 includes special circuitry that allows it to trigger  
off the input waveform and also to be able to measure the time  
between the trigger instant and the first ADC sample that is taken.  
In this way, several single shot acquisitions are taken and the data  
points for each “sweep” are ordered based on the relative time as  
measured. For this to work of course, the relationship between the  
trigger instant and the waveform must remain constant i.e. a  
repetitive waveform is required like a continuous sine wave or  
square wave for example. It also needs the scope to be in normal  
trigger mode…the software automatically switches to this mode on  
entering RIS mode.  
The software automatically sweeps the input several times before  
updating the display. Because each sweep happens at a random time  
with respect to the input waveform, the relative times measured for  
each sweep are also random. So it can take a few seconds for the  
“picture” of the waveform to update fully. While this acquisition  
process is happening, you may see some waveform displays that are  
not related to the actual input waveform…this is because the random  
nature of the sweeps means that the software may not have  
completely built up the picture of the signal, leaving some data from  
previous sweeps on the screen. This is normal. Wait a while and the  
waveform will update completely.  
Another side-effect of the RIS mode is that because the relative  
sweep time measurement is “quantized” i.e. the time value is  
rounded up or down to place it into one of 20 possible values, or  
“bins”, a fast changing input signal can show small anomalies13 on  
the screen as a result…the software forces the sweep data into one or  
other of the bins even though the data may have been at one end of  
the “bin” or the other.  
13 This may show up as small spikes that come and go, particularly near to fast changing edges. In  
essence the data for a particular sweep is forced to a particular place on the time axis and these data  
points may therefore appear to be in slightly the “wrong” place in time…showing as an error in voltage  
i.e. a spike. This is normal.  
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RIS mode is not well suited to very slow input signals or signals that  
have jitter. This will lead to an uncertainty in the trigger instant and  
hence the sweep data will appear in the wrong “bins” and so the  
displayed waveform will not “lock” on the screen over time.  
Please note that in RIS mode it is not possible to observe the  
probe compensation output. This is because it is precisely phase-  
locked to the ADC’s clock hence there is no way to take random  
sweeps to build up the picture...every sweep comes out in the same  
bin due to the phase lock. This is normal.  
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2.7 Trigger Modes  
The USBscope50 can use three main types of triggering. These  
modes are used when the “run” button or the “once14” button has  
been pressed causing the scope to enter the run state.  
2.7.1 Auto Triggering  
In this mode the acquisition begins just after the software has set up  
the scope. The scope will effectively free run, but it will try  
periodically to trigger from the input waveform. If a trigger is  
detected the scope will stay in a mode to enable it run as though it is  
in Normal mode (see below). This means the scope will lock to the  
waveform. If no trigger is detected the scope will carry in in a Free  
Run mode. Note that when you adjust the trigger threshold or the  
timebase, the scope will shorten the time until the next trigger test so  
that it can lock to the waveform more rapidly as you adjust these  
settings. If the scope looses lock on the waveform, you will observe  
a brief delay (1 to 2 seconds) before the Free Run mode is resumed.  
In Auto mode, when triggering is detected, the trigger status panel  
will illuminate red.  
14 The once button does a single acquisition and so does not perform any trigger test when in Auto  
mode. Effectively, using the once button in Auto mode is the same as using it in Free mode. In Norm  
mode, the scope will wait for the trigger event during a “once” acquisition.  
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It is normal for the scope to take several seconds to move from free  
run to triggered mode when a signal is first applied to the scope  
input or is changed significantly.  
2.7.2 Normal Triggering  
In this mode, the acquisition is primed, but will not start until the  
input waveform meets some criteria. This mode will cause the  
waveform on the screen to “lock” to an edge and so appear fixed in  
time. It is useful for observing regular waveforms or for doing a  
single triggered acquisition. If no suitable waveform is present, the  
scope will wait indefinitely with no display update in the meantime.  
2.7.3 Free Triggering  
This mode is a simple Free Run (like Auto Mode) with no attempt to  
lock to the input waveform. It is good for checking DC levels etc.  
Note there are no options for edge selection as these have no effect  
in Free Mode.  
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2.8 Trigger Position  
The total sample buffer is 3000 points long. The acquisition can be  
triggered in Auto and Norm mode from the input waveform.  
By adjusting the trigger position slider, you can make the trigger  
position in the buffer earlier or later in time. This is known as pre  
and post triggering.  
Trigger position is adjustable in single-shot mode only15.  
2.9 Trigger Delay  
Like the trigger position setting, the trigger delay allows an amount  
of time to pass after the trigger instant, before the acquisition stores  
the sample data into the buffer. This allows you to see events that  
happen some time after the trigger.  
The delay is adjustable in steps of the sample interval, from 0 to  
65535 steps. Adding trigger delay when using slow timebase  
settings further slows the time between successive sweeps.  
When delayed trigger is used, the trigger mark on the plot shows a  
“<” symbol.  
15 By definition, RIS mode needs repetitive waveforms so pre or post trigger has no relevance.  
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Trigger delay is effective in single-shot mode only.  
Note that setting a large delay will noticeably slow the overall  
acquisition rate.  
Also note that if you forget that you have set up a delayed trigger, it  
can appear that you can’t find the trigger event on your waveform.  
Please keep note of whether there is a “<” symbol on the trigger  
indicator.  
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2.10Trigger Threshold  
You can adjust the trigger voltage that is used for Auto and Norm  
Modes, either by turning the trigger knob or by clicking on the main  
plot.  
After the trigger threshold has been moved, a guide line appears on  
the screen for a few seconds.  
2.11Full Screen Plot  
To aid viewing the time plot, a full screen mode is available. Note  
that when viewing the waveform at such a large scale, you will be  
able to see the small steps in the waveform introduced by the  
digitisation process. This is normal.  
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The full screen plot can be placed on top by simply left clicking it.  
To pop the scope back on top, click the plot with the right mouse  
key.  
The full screen plot can be stretched to any size, and can be  
maximised by double clicking it.  
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2.12FFT Plot (Spectrum Analyser)  
Each scope channel can be analysed using a 2048 point Fast Fourier  
Transform. The plot will be shown in a scalable window and will  
include all channels selected for analysis, in their respective colours.  
The lower limit for the dB plot is limited to –54dB. An on-screen  
cross-hair type cursor allows you to measure points on the spectrum.  
The FFT time data can be “pre-shaped” using various window  
functions, available under the MATH tab. There is also a selection  
for dB or Linear plot types on the same tab. These settings are  
global for all FFTs.  
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2.13Math Functions  
The USBscope50 includes two virtual math channels. These  
channels are generated using the data from two scope channels  
called A and B and a mathematical function, like +, - etc.  
The math functions are accessed under the MATH tab.  
Note that the voltage range selector knobs may adjust or limit  
automatically. This is so that the computed math data cannot be  
shown in higher effective resolution than either of the two  
constituent channels used in the math. The practical effect of this is  
that if you try and turn the voltage selector for a math channel to a  
setting that is lower than one or both of the selected channels, the  
knob will jump back to the lowest setting allowed. Equally, if you  
adjust either of the channels involved in the maths, then the math  
channel selector knob will auto adjust to match the lowest setting of  
either channel.  
The math data computed can also be FFT’d just like the regular  
scope channels.  
IMPORTANT NOTE: The math functions use the true channel data.  
If you invert a channel using the “inv” button, this will have no  
effect on the math result. So to get ch1 minus ch2, select “A” as  
“1”, select “B” as “2” and select the “fn” as “-“.  
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2.14Data Export  
The channel data and FFT data can be saved using the DATA tab.  
Simply select the channels you wish to save and click the save  
button. You will be prompted for a file name. The final files will be  
stored as:  
YourSelectedName.chNdata.txt  
and  
YourSelectedName.chNfft.txt  
where N is the channel number. FFT data will only be stored if that  
channel’s FFT is enabled.  
Remember to stop the scope before saving the data otherwise the  
most recent data will be saved.  
Data is saved in ASCII text format and will import directly to Excel  
or MathCAD.  
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2.14.1Example Data File  
There are 3000 sets of numbers, followed by a footer that defined the  
acquisition mode used.  
-5.0079  
-4.7575  
-5.0079  
-5.0079  
-4.7575  
-4.7575  
-5.0079  
-4.7575  
-4.7575  
-4.7575  
-4.7575  
-4.7575  
DATA FOR CH: 1  
VERTICAL FULL SCALE (+/-v): 30  
SAMPLE PERIOD (s): 0.0004  
BANDWIDTH LIMIT: False  
DATE: 21/09/2005 11:32:31  
SOFTWARE: USBscope50 Ver1.0.8  
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2.14.2Example FFT File  
There are 1024 sets of numbers, followed by a footer that defined the  
acquisition mode used.  
-54.0  
-54.0  
-54.0  
-54.0  
-54.0  
-54.0  
-54.0  
-54.0  
-54.0  
-54.0  
-54.0  
-54.0  
FFT FOR CH: 1  
VERTICAL FULL SCALE (+/-v): 30  
FREQ STEP (Hz): 2.44140625  
SPECTRAL WINDOW: Rectangular  
PLOT TYPE: dB(V) Plot  
DATE: 27/09/2005 18:48:39  
SOFTWARE: USBscope50 Ver1.0.8  
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3 SOFTWARE INSTALLATION  
3.1 Windows 98SE and Windows Me  
Before plugging in the hardware:  
Use the supplied install CD and run the setup program. This will  
copy all the required files and drivers to your PC.  
After running the setup program:  
Insert the USBscope50 into a free USB socket, or into a USB hub  
port. A USB extension cable can be used if needed.  
During installation, three new hardware devices are detected: The  
USBscope50 Composite Device” first, followed (twice) by the  
USBscope50 Controller” itself. The installation is automatic and  
requires no user input. After the drivers have started, you will not  
get any indication that everything went OK except by checking the  
device manager. After installation the device manager will look like  
this16:  
16 The COM port number will be platform specific, this is just an example  
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Once the hardware has installed, there is no need to make any  
settings for the allocated COM port…the software takes care of all  
this at run time.  
Start the USBscope50 software and you will see the following  
display:  
To find out what the various buttons and knobs do, simply hover  
over them for a brief explanation.  
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3.2 Windows 2K and XP17  
Before plugging in the hardware:  
Use the supplied install CD and run the setup program. This will  
copy all the required files and drivers to your PC.  
After running the setup program:  
Insert the USBscope50 into a free USB socket, or into a USB hub  
port. A USB extension cable can be used if needed.  
During installation, two hardware devices are detected: The  
USBscope50 Composite Device” first, followed by the  
USBscope50” itself. It is vital to complete the installation of  
both devices18. After installation the device manager will look like  
this19:  
17 Include Language variants using the DBCS character mappings e.g. Chinese, Japanese, Korean etc  
18  
If Windows prompts to search the Internet for a driver, select “Not  
this time”, and when it warns about Unsigned Drivers you MUST  
click on “Continue Anyway”  
19 The COM port number will be platform specific, this is just and example  
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Once the hardware has installed, there is no need to make any  
settings for the allocated COM port…the software takes care of all  
this at run time20.  
Start the USBscope50 software and you will see the following  
display:  
To find out what the various buttons and knobs do, simply hover  
over them for a brief explanation.  
20 You may be prompted to alter the COM port number…please follow the on-screen instructions.  
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4 HARDWARE SPECIFICATION  
All parameters typical @ 20°C unless otherwise stated  
4.1 Power Requirements  
Supply Voltage:  
5.0V  
±10% from host USB bus  
Total Supply Current:  
200mA avg  
4.2 Mechanical  
Mass:  
42g typ.  
Case Material Data:  
Size (typical in mm):  
Polycarbonate (UL94V rated)  
99.621 x 30.6 x 17.522  
4.3 Environmental  
Humidity:  
<80% non condensing  
-10°C to +45°C Ambient  
22°C ±3°C for rated accuracy  
10mins for rated accuracy  
-40°C to +80°C Ambient  
Indoor or under-cover use only  
Cat II  
General Operating Temperature:  
Specific Operating Temperature:  
Full Warm Up Time:  
Storage Temperature:  
Operating Location:  
Operational Category:  
Pollution Degree:  
2
21 From BNC end to USB end  
22 Not including “P” clips on base  
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4.4 Performance  
4.4.1 Safety Data and Maximum Ratings  
Important Safety Precautions  
Always observe these when using the USBscope50  
The USBscope50 contain no user serviceable parts inside.  
Do not open the plastic housing.  
There may be lethal voltages inside the plastic housing. Do  
not use the instrument if the housing is damaged or is poorly  
fitting. In such a case do not connect anything to the  
USBscope50 to avoid a hazard. The USBscope50 will have  
to be repaired or replaced in such a situation.  
Do not exceed the maximum ratings listed below.  
Never use the instrument if it becomes damp for any reason.  
This includes situations were condensation has formed on  
the unit due to sudden temperature or humidity changes.  
Never use test leads that are damaged or have insufficient or  
incomplete insulation.  
Never allow any conductive part of any test lead to contact  
the host computer ground. Doing so will bypass the safety  
isolation in the USBscope50 and could cause a lethal hazard.  
Remember that the isolation is between the BNC and the  
USB connectors. The BNC is, of course, at the same  
potential as the test lead ground clip to which it is connected.  
Be careful when measuring hazardous voltages not to touch  
the BNC connector ground for this reason23.  
Only use the shorter length stack connector in the bottom  
scope of the stack, and if using a single scope, don’t fit any  
stack connector at all. This is to avoid touching the contacts  
23 This is true of almost all scopes, except that most scopes have no isolation to safety earth…in fact  
normal scopes connect the BNC ground directly to safety earth. If you were to connect a probe  
ground clip to an earth referenced potential you would short it out on a normal scope!  
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Isolation rating:  
300V CAT II, 500V CAT I between BNC  
ground and USB ground  
BNC ground to USB ground +/-2.5KV  
1000pF typ between BNC ground and USB  
ground  
Transient isolation24:  
Isolation capacitance25:  
Maximum Measured Voltage:  
Between BNC center and BNC ground: +/-30V.  
Absolute Maximum Input Voltage26: Between BNC center and BNC ground: +/-50V.  
4.4.2 Static Performance  
Input DC resistance:  
Input capacitance:  
Range accuracy:  
1Meg Ohm ±2%  
16pF ±10% at 1MHz  
+/-0.3V range:  
+/-3.0V range:  
+/-30.0V range:  
AC, DC, GND  
8bit  
±4%  
±6%  
±6%  
Input coupling modes:  
ADC vertical resolution:  
Channel offset error:  
Channel offset control:  
Buffer depth:  
Pre-triggering:  
Post-triggering:  
Triggering:  
±2% of range  
±100% of range, approx 7bit resolution  
3000 points  
Up to 99% of buffer depth27  
Up to 100% of buffer depth27  
Auto, normal, rising edge, falling edge, greater,  
less  
Trigger delay:  
Trigger range:  
From 0 to 65535 sample periods27  
±100% of range, approx 7bit resolution  
24 This figure derives from the 300V CAT II isolation rating and defines the peak transient voltage that  
can be safely tolerated between the BNC ground and the USB ground.  
25 This capacitance causes the impedance across the isolation barrier will reduce with frequency. This  
is only significant if an AC component is impressed between the BNC ground and the USB ground that  
is referenced to the USB ground. At 50/60Hz this impedance is approximately 3MegOhms.  
26 This level will saturate the scope input, and is the maximum that can be applied without causing  
damage to the scope. It applies regardless of the input attenuator or coupling setting.  
27 Single shot mode only  
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4.4.3 Dynamic Performance  
Maximum ADC single shot rate:  
50MSPS  
Maximum effective sample rate28: 1GSPS  
Sample rates available:  
4ns/div to 4s/div in 1,2,4 sequence  
Sample rate accuracy:  
0.02% typ  
Stacked scope channel skew:  
Analogue 3dB bandwidth:  
AC coupling 3dB high pass freq:  
±2ns between any channel pair typ  
75MHz typ  
3.4Hz typ  
Analogue trigger 3dB bandwidth29: 60MHz typ  
SFDR:  
50dB typ  
Compensation output:  
0 to 3V nominal 1KHz square wave, absolute  
max source/sink current 1mA  
4.4.4 Miscelaneous  
USB transfer rate:  
USB device ID:  
USB 1.130 Full Speed 12MBits/sec  
10C4 F001  
28 Using RIS mode  
29 The circuit involved with triggering causes the maximum input frequency that can trigger the scope  
to be lower than the scopes measurement channel bandwidth.  
30 Works in USB 1.1 or USB 2.0 hosts using the 12MBits/sec full speed mode  
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