The R&S VSE-K18 is a firmware application that adds functionality to measure the efficiency of amplifiers with the R&S VSE signal analyzer. You extend the amplifier application with the R&S VSE-K18D, which adds direct DPD functionality.
This user manual contains a description of the functionality that the application provides, including remote control operation.
Functions that are not discussed in this manual are the same as in the base unit and
are described in the R&S VSE user manual. The latest versions of the manuals are
available for download at the product homepage.
Installation
Find detailed installing instructions in the getting started or the release notes of the
R&S VSE.
●Starting the application..............................................................................................9
●Understanding the display information....................................................................10
1.1Starting the application
The amplifier measurement application adds a new type of measurement to the
R&S VSE.
To activate the amplifier application
1.
Select the "Add Channel" function in the Sequence tool window.
A dialog box opens that contains all operating modes and applications currently
available in your R&S VSE.
2. Select the "Amplifier" item.
The R&S VSE opens a new measurement channel for the Amplifier measurement
application.
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1.2Understanding the display information
Welcome to the amplifier measurement application
Understanding the display information
The following figure shows the display as it looks for amplifier measurements. All different information areas are labeled. They are explained in more detail in the following
sections.
142356
Figure 1-1: Screen layout of the amplifier measurement application
1 = Toolbar
2 = Channel bar
3 = Diagram header
4 = Result display
5 = Status bar
6 = Softkey bar
For a description of the elements not described below, refer to the getting started of the
R&S VSE.
Channel bar information
The channel bar contains information about the current measurement setup, progress
and results.
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Welcome to the amplifier measurement application
Understanding the display information
Figure 1-2: Channel bar of the amplifier application
Ref LevelCurrent reference level of the analyzer.
AttCurrent attenuation of the analyzer.
FreqFrequency the signal is transmitted on.
Meas TimeLength of the signal capture.
Meas BWBandwidth with which the signal is recorded.
TTFTime difference between the trigger event and the first sample of the reference
signal (= beginning of a frame).
SRateSample rate with which the signal is recorded.
SGLIndicates that single sweep mode is active.
CountThe current signal count for measurement tasks that involve a specific number
of subsequent sweeps (for example the parameter sweep).
X AxisX-axis value that is currently measured.
Y AxisY-axis value that is currently measured.
Window title bar information
For each diagram, the header provides the following information:
1
Figure 1-3: Window title bar information of the amplifier application
1= Window number
2= Window type
3= Trace color and number
4= Trace mode
Blue color = Window is selected
234
Status bar information
Global instrument settings, the instrument status and any irregularities are indicated in
the status bar beneath the diagram. Furthermore, the progress of the current operation
is displayed in the status bar.
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2Measurements and result displays
Measurements and result displays
Note that you can use the R&S VSE-K18 with the sequencer that is available with the
R&S VSE. The functionality is the same as in the spectrum application. Refer to the
R&S VSE user manual for more information.
The "ACLR" result display shows the power characteristics of the transmission (Tx)
channel and its neighboring channel(s).
The ACLR measurement in the R&S VSE-K18 is a measurement based on I/Q data.
Thus, its results are calculated by the same I/Q data as the rest of the results (like the
EVM). Note that the supported channel bandwidth is limited by the I/Q bandwidth of the
analyzer you are using.
The results are provided in numerical form in a table. The table is made up out of two
parts, one part containing the characteristics of the Tx channel, the other containing
those of the neighboring channels.
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The table contains the following information.
●
Channel
Shows the type of channel.
●
Bandwidth
Shows the channel's bandwidth.
●
Offset (neighboring channels only)
Shows the frequency offset between the center frequency of the adjacent (or alternate) channel and the center frequency of the transmission channel.
●
Power
Shows the power of the transmission channel, or the power of the upper / lower
neighboring channel.
The result is calculated over the complete capture buffer, not just the evaluation
range.
●
Balanced
Shows the difference between the lower and upper adjacent channel power
("Lower Channel" - "Upper Channel").
For more information on configuring the ACP measurement, see Chapter 3.15, "Con-
figuring adjacent channel leakage error (ACLR) measurements", on page 110.
Remote command:
Selection: LAY:ADD? '1',LEFT,ACP
Result query: CALCulate<n>:MARKer<m>:FUNCtion:POWer:RESult?
on page 330
AM/AM
The "AM/AM" result display shows nonlinear effects of the DUT. It shows the amplitude
at the DUT input against the amplitude at the DUT output.
The ideal "AM/AM" curve would be a straight line at 45°. However, nonlinear effects
result in a measurement curve that does not follow the ideal curve. When you drive the
amplifier into saturation, the curve typically flattens at high input levels.
The width of the "AM/AM" trace is an indicator of memory effects: the larger the width
of the trace, the more memory effects occur. The "AM/AM" Curve Width is shown in the
numerical Result Summary.
Both axes show the power of the signal in dBm.
You can analyze the "AM/AM" characteristics of the measured signal and the modeled
signal.
●
Measured signal
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Shows the "AM/AM" characteristics of the DUT.
The software uses the reference signal in combination with the synchronized measurement signal to calculate a software model that describes the characteristics of
the device under test.
The measured signal is represented by a colored cloud of values. The cloud is
based on the recorded samples. If samples have the same values (and would thus
be superimposed), colors represent the statistical frequency with which a certain
input / output level combination occurs. Blue pixels represent low statistical frequencies, red pixels high statistical frequencies. A color map is provided within the
result display.
●
Modeled signal
Shows the "AM/AM" characteristics of the model that has been calculated. The
modeled signal is calculated by applying the DUT model to the reference signal.
When the model matches the characteristics of the DUT, the characteristics of the
model signal are the same as those of the measured signal (minus noise).
The modeled signal is represented by a line trace.
When system modeling has been turned off, this trace is not displayed.
All traces include the digital predistortion, when you have turned on that feature.
Remote command:
Selection: LAY:ADD? '1',LEFT,AMAM
Result query: TRACe<n>[:DATA]?on page 143
AM/PM
The "AM/PM" result display shows nonlinear effects of the DUT. It shows the phase difference between DUT input and output for each sample of the synchronized measurement signal.
The ideal "AM/PM" curve would be a straight line at 0°. However, nonlinear effects
result in a measurement curve that does not follow the ideal curve. Typically, the curve
drifts from a zero phase shift, especially at high power levels when you drive the amplifier into saturation.
The width of the "AM/PM" trace is an indicator of memory effects: the larger the width
of the trace, the more memory effects occur. The "AM/PM" curve width is shown in the
numerical Result Summary.
The x-axis shows the levels of all samples of the reference signal (input power) or the
measurement signal (output power) in dBm. You can select the reference of the x-axis
(input or output power) in the "Result Configuration" dialog box.
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Measurements and result displays
The y-axis shows the phase of the signal for the corresponding power level. The unit is
either rad or degree, depending on your phase unit selection in the "Result Configuration" dialog box.
You can analyze the "AM/PM" characteristics of the real DUT or of the modeled DUT.
●
Measured signal
Shows the "AM/PM" characteristics of the DUT.
The software uses the reference signal together with the synchronized measurement signal to calculate a software model that describes the characteristics of the
device under test.
The measured signal is represented by a colored cloud of values. The cloud is
based on the recorded samples. If samples have the same values (and would thus
be superimposed), colors represent the statistical frequency with which a certain
input / output level combination occurs. A color map is provided within the result
display.
●
Modeled signal
Shows the "AM/PM" characteristics of the model that has been calculated. The
modeled signal is calculated by applying the DUT model to the reference signal.
When the model matches the characteristics of the DUT, the characteristics of the
modeled signal are the same as those of the measured signal (minus noise).
The modeled signal is represented by a line trace.
When system modeling has been turned off, this trace is not displayed.
All traces include the digital predistortion, when you have turned on that feature.
Remote command:
Selection: LAY:ADD? '1',LEFT,AMPM
Result query: TRACe<n>[:DATA]?on page 143
DDPD Results (R&S VSE-K18D)
The "DDPD Results" result display shows a selectable result (such as EVM or ACLR)
over all iterations of the direct DPD. This allows verification of the direct DPD's convergence as well as picking the ideal iteration step for further processing (e.g. in
R&S VSE-K18M). It is only available with application R&S VSE-K18D installed.
The display must be placed on screen before starting the direct DPD. The result type is
configurable in the "Result Configuration" dialog box.
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Remote command:
Selection: LAY:ADD? '1',LEFT,DDPD
Configure result type: CONFigure:DDPD:WINDow<n>:RESulton page 316
Result query: TRACe<n>[:DATA]?on page 143
EVM vs Power
The "EVM vs Power" result display shows the EVM against the measured power values.
The ideal EVM vs power curve would be a straight line at 0 %. However, among other
effects such as noise, nonlinear effects of the DUT cause an increase of the EVM.
Nonlinear effects usually occur on high power levels that drive the power amplifier into
saturation.
The x-axis shows the levels of all samples of the reference signal (input power) or the
measurement signal (output power) in dBm. You can select the reference of the x-axis
(input or output power) in the "Result Configuration" dialog box.
The y-axis shows the EVM of the signal for the corresponding power level in %.
All traces include the digital predistortion, when you have turned on that feature.
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Measurements and result displays
Remote command:
Selection: LAY:ADD? '1',LEFT,AMEV
Result query: TRACe<n>[:DATA]?on page 143
Error Vector Spectrum
The "Error Vector Spectrum" result display shows the error vector (EV) signal in the
spectrum around the center frequency.
The EV is a measure of the modulation accuracy. It compares two signals and shows
the distance of the measured constellation points and the ideal constellation points.
The unit is dB.
You can compare the measured signal against the reference signal and against the
modeled signal.
●
Measured signal against reference signal
Trace 1 compares measured signal and the reference signal.
To get useful results, the calculated linear gain is compensated to match both signals.
Depending on the DUT, noise and nonlinear effects may have been added to the
measurement signal. These effects are visualized by this trace.
●
Measured signal against modeled signal
Trace 2 compares measured signal and the modeled signal.
The EVM between the measured and modeled signal indicates the quality of the
DUT modeling. If the model matches the DUT behavior, the modeling error is zero
(or is merely influenced by noise).
This result display shows changes in the model and its parameters and thus allows
you to optimize the modeling.
When system modeling has been turned off, this trace is not displayed.
Remote command:
Selection: LAY:ADD? '1',LEFT,SEVM
Result query: TRACe<n>[:DATA]?on page 143
Gain Compression
The "Gain Compression" result display shows the gain and error effects of the DUT
against the DUT input or output power.
The gain is the ratio of the input and output power of the DUT.
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Measurements and result displays
The x-axis shows the levels of all samples of the reference signal (input power) or the
measurement signal (output power) in dBm. You can select the reference of the x-axis
(input or output power) in the "Result Configuration" dialog box.
The y-axis shows the gain in dB.
The ideal gain compression curve would be a straight horizontal line. However, nonlin-
ear effects result in a measurement curve that does not follow the ideal curve. In addition, the curve widens at very low input levels due to noise influence.
The width of the gain compression trace is an indicator of memory effects: the larger
the width of the trace, the more memory effects occur.
You can analyze the gain characteristics of the measured signal and the modeled signal.
●
Measured signal
Shows the gain characteristics of the DUT.
The software uses the reference signal in combination with the synchronized measurement signal to calculate a software model that describes the characteristics of
the device under test.
The measured gain is represented by a colored cloud of values. The cloud is
based on the recorded samples. If samples have the same values (and would thus
be superimposed), colors represent the statistical frequency with which a certain
input / output level combination occurs. Blue pixels represent low statistical frequencies, red pixels high statistical frequencies. A color map is provided within the
result display.
●
Modeled signal
Shows the gain characteristics of the model that has been calculated. The modeled
signal is calculated by applying the DUT model to the reference signal.
When the model matches the characteristics of the DUT, the characteristics of the
model signal are the same as those of the measured signal (minus noise).
The modeled signal is represented by a line trace.
When system modeling has been turned off, this trace is not displayed.
In addition, one or more horizontal lines can appear in the result display.
●
One line to indicate each compression point (1dB, 2dB and 3dB).
●
One line to indicate the reference point (0 dB compression) that the compression
points refer to.
Remote command:
Selection: LAY:ADD? '1',LEFT,GC
Result query: TRACe<n>[:DATA]?on page 143
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Gain Deviation vs Time
The "Gain Deviation vs Time" result display shows the deviation of each measured signal sample from the average gain of the measured signal.
The x-axis shows the time in seconds. The y-axis shows the gain deviation in dB.
The displayed results are based on the synchronized measurement data (represented
by the green bar in the capture buffer).
Note that the result query and trace export only work for unencrypted reference signal
waveform files.
Remote command:
Selection: LAY:ADD? '1',LEFT,GDVT
Result query: TRACe<n>[:DATA]?on page 143
Magnitude Capture
The "Magnitude Capture" result display contains the raw data that has been recorded
and thus represents the characteristics of the DUT.
The raw data is source for all further evaluations. You can also use the data in the capture buffer to identify the causes for possible unexpected results.
When you synchronize the reference signal and the measured signal, the synchronized
area is indicated by a horizontal green bar on the bottom of the diagram.
The current reference level is indicated by a red horizontal line.
The green bar at the bottom shows the current frame. In I/Q averaging mode, the aver-
age value is shown. In trace statistics mode, multiple values are possible. The currently
selected value is symbolized by a blue bar.
The "Memory DPD Coefficients" result table shows basically complex filter coefficients
for each polynomial degree. The two lines "1(Real)" and "1(Imag)" describe the complex impulse response for polynomial degree 1 (linear) of a filter from left to right. It is
only available with application R&S VSE-K18M installed.
Remote command:
Selection: LAY:ADD? '1',LEFT,MDPD
Result query: FETCh:MDPD:COEFficients?on page 326
Parameter Sweep
The "Parameter Sweep" result display is a result display that shows a result of the DUT
(for example the EVM) against two (custom) measurement parameters. The results of
this measurement are displayed in graphical and numerical form.
The parameter sweep is a good way, for example, to find the location of the ideal delay
time of the RF signal and the envelope signal if you are measuring an amplifier that
supports envelope tracking. You can also use the parameter sweep to determine the
characteristics and behavior of an amplifier over different frequencies and levels.
For more information about supported parameters and how to set them up see "Select-
ing the data to be evaluated during the parameter sweep"on page 115.
Parameter Sweep: Diagram ← Parameter Sweep
The parameter sweep diagram is a graphical representation of the parameter sweep
results. The results are either represented as a two-dimensional trace or as a threedimensional trace, depending on whether you are performing a parameter sweep with
one or two parameters.
In a two-dimensional diagram, the y-axis always shows the result. The displayed result
depends on the result type you have selected. The information displayed on the x-axis
depends on the parameter you have selected for evaluation (for example the EVM over
a given frequency range). Values between measurement point are interpolated. Basically, you can interpret the two-dimensional diagram as follows (example): "at a frequency of x Hz, the EVM has a value of y."
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Measurements and result displays
In a three-dimensional diagram, the z-axis always shows the result. The information on
the other two axes is arbitrary and depends on the parameters you have selected for
evaluation. For a better readability, the result values in the three-dimensional diagram
are represented by a colored trace: low values have a blue color, while high values
have a red color. Values between measurement point are interpolated. Basically, you
can interpret the three-dimensional diagram as follows (example): "at a frequency of
x Hz and a level of y, the EVM has a value of z."
Parameter Sweep: Table ← Parameter Sweep
The parameter sweep table shows the minimum and maximum results for all available
result types in numerical form. For each result type, the location where the minimum
and maximum result has occurred is displayed.
Example:
A minimum EVM of 0.244 % and a maximum EVM of 0.246 % has been measured
(first and second row). The minimum EVM has been measured at a frequency of
30 MHz and an output power of 0 dBm. The maximum EVM has been measured at a
frequency of 10 MHz and an output power of 0 dBm.
The following result types are evaluated in the parameter sweep.
ResultDescription
EVMError vector magnitude between synchronized reference and mea-
surement signal.
ACLRPower of the transmission channel.
ACLR Adj Upper / LowerPower of the adjacent channels (upper and lower).
ACLR Balanced (Adj, Alt1 and
Alt2)
RMS PowerRMS signal power at the DUT output.
GainGain of the DUT.
Crest Factor OutCrest factor of the signal at the DUT output. The crest factor is the
Curve Width ("AM/AM", "AM/PM") Spread of the samples in the "AM/AM" (or "AM/PM") result display
Power OutSignal power at the DUT output.
Difference between the lower and upper adjacent channel power
ratio of the RMS and peak power.
compared to the ideal "AM/AM" (or "AM/PM") curve.
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ResultDescription
Compression Point (1 dB / 2 dB /
3 dB)
Bal ACLR MagnitudeShows the difference between the lower and upper adjacent channel
Input power where the gain deviates by 1 dB, 2 dB or 3 dB from a reference gain (see "Configuring compression point calculation"
on page 110).
power.
Remote command:
Chapter 5.4.3.3, "Retrieving results of the parameter sweep table", on page 160
Phase Deviation vs Time
The "Phase Deviation vs Time" result display shows the phase deviation of the measured signal compared to the reference signal over time.
The x-axis shows the time in seconds. The y-axis shows the phase deviation in
degree.
The displayed results are based on the synchronized measurement data (represented
by the green bar in the capture buffer).
Note that the result query and trace export only work for unencrypted reference signal
waveform files.
Remote command:
Selection: LAY:ADD? '1',LEFT,PDVT
Result query: TRACe<n>[:DATA]?on page 143
Raw EVM
The "Raw EVM" result display shows the error vector magnitude of the signal over
time.
The EVM is a measure of the modulation accuracy. It compares two signals and shows
the distance of the measured constellation points and the ideal constellation points.
You can compare the measured signal against the reference signal and against the
modeled signal.
●
Measured signal against reference signal
Trace 1 compares the measured signal and the reference signal.
To get useful results, the calculated linear gain is compensated to match both signals.
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Measurements and result displays
Depending on the DUT, noise and nonlinear effects may have been added to the
measurement signal. These effects are visualized by this trace.
●
Measured signal against modeled signal
Trace 2 compares the measured signal and the modeled signal.
The EVM between the measured and modeled signal indicates the quality of the
DUT modeling. If the model matches the DUT behavior, the modeling error is zero
(or is merely influenced by noise).
This result display shows changes in the model and its parameters and thus allows
you to optimize the modeling.
When system modeling has been turned off, this trace is not displayed.
Note that the raw EVM is calculated for each sample that has been recorded. Thus, the
raw EVM can differ from EVM values that are calculated according to a specific mobile
communication standard that apply special rules to calculate the EVM, for example
LTE.
Remote command:
Selection: LAY:ADD? '1',LEFT,REVM
Result query: TRACe<n>[:DATA]?on page 143
Numeric Result Summary
The "Result Summary" shows various measurement results in numerical form, combined in one table.
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Measurements and result displays
For each result type, several values are displayed.
●
Current
Value measured during the last sweep.
For measurements that evaluate each captured sample, this value represents the
average value over all samples captured in the last sweep.
●
Min
For measurements that evaluate each captured sample, this value represents the
sample with lowest value captured in the last sweep.
●
Max
For measurements that evaluate each captured sample, this value represents the
sample with the highest value captured in the last sweep.
●
Unit
Unit of the result.
Results that evaluate each captured sample
●
"Raw EVM" and Raw Model EVM
●
Power In and Power Out
Note: When synchronization has failed or has been turned off, some results may be
unavailable.
Remote command:
Selecting the result display: LAY:ADD? '1',LEFT,RTAB
Querying results: see Chapter 5.4.3, "Retrieving numeric results", on page 145
Results to check modulation accuracy ← Numeric Result Summary
Raw EVMError vector magnitude between synchronized reference and measured sig-
nal.
FETCh:MACCuracy:REVM:CURRent[:RESult]? on page 149
Raw Model EVMError vector magnitude between synchronized measured and model signal.
FETCh:MACCuracy:RMEV:CURRent[:RESult]? on page 150
Frequency ErrorDifference of the RF frequency of the reference signal compared to the mea-
sured signal.
Note that a frequency error is not available if the frequency error estimation is
switched off. See also Chapter 3.9, "Estimating and compensating signal
errors", on page 90.
FETCh:MACCuracy:FERRor:CURRent[:RESult]? on page 147
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Measurements and result displays
Sample Rate ErrorSample rate difference between reference and measured signal.
Note that a sample rate error is not available if the sample rate error estimation is switched off. See also Chapter 3.9, "Estimating and compensating sig-
nal errors", on page 90.
FETCh:MACCuracy:SRERror:CURRent[:RESult]? on page 150
Magnitude ErrorDifference in magnitude between the reference signal and the measured sig-
nal.
FETCh:MACCuracy:MERRor:CURRent[:RESult]? on page 148
Phase ErrorPhase difference between reference and measured signal.
FETCh:MACCuracy:PERRor:CURRent[:RESult]? on page 149
Quadrature ErrorPhase deviation of the 90° phase difference between the real (I) and imagi-
nary (Q) part of the signal.
Within an ideal transmitter, the I and Q signal parts are mixed with an angle of
90° by the I/Q output mixer. Due to hardware imperfections, the signal delay of
I and Q can be different and thus lead to an angle non-equal to 90°.
Note that quadrature rate error is not available if the I/Q Imbalance estimation
is switched off. See also Chapter 3.9, "Estimating and compensating signal
errors", on page 90.
FETCh:MACCuracy:QERRor:CURRent[:RESult]? on page 149
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Measurements and result displays
Gain ImbalanceGain difference between the real (I) and imaginary (Q) part of the signal.
This effect is typically generated by two separate amplifiers with a different
gain in the I and Q path of the analog baseband signal generation.
Note that gain imbalance is not available if the I/Q Imbalance estimation is
switched off. See also Chapter 3.9, "Estimating and compensating signal
errors", on page 90.
FETCh:MACCuracy:GIMBalance:CURRent[:RESult]? on page 147
I/Q ImbalanceCombination of Quadrature error and Gain imbalance.
The I/Q imbalance parameter is a representation of the combination of Quadrature error and gain imbalance.
Note that I/Q imbalance is not available if the I/Q imbalance estimation is
switched off. See also Chapter 3.9, "Estimating and compensating signal
errors", on page 90.
FETCh:MACCuracy:IQIMbalance:CURRent[:RESult]? on page 148
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I/Q OffsetShift of the measured signal compared to the ideal I/Q constellation in the I/Q
plane.
Note that I/Q offset is not available if the I/Q Offset estimation is switched off.
See also Chapter 3.9, "Estimating and compensating signal errors",
on page 90.
FETCh:MACCuracy:IQOFfset:CURRent[:RESult]? on page 148
Amplitude DroopAmplitude droop is a measure of the change in magnitude of the signal over
the frame (reference signal) being measured in dB.
Note that amplitude droop is not available if the amplitude droop estimation is
switched off. See also Chapter 3.9, "Estimating and compensating signal
errors", on page 90.
Results to check power characteristics ← Numeric Result Summary
Power InSignal power at the DUT input when reference signal is active. The signal
generator level may change during direct DPD, but this result summary value
will always refer to the reference signal – not the DPD signal.
FETCh:POWer:INPut:CURRent[:RESult]? on page 153
Power In (Sensor)Signal power at the input power sensor.
FETCh:POWer:SENSor:IN:CURRent[:RESult]? on page 156
Power OutSignal power at the DUT output.
Power Out (Sensor)Signal power at the output power sensor.
It is the RMS power of:
●
The currently selected frame, if R&S VSE-K18 has successfully
synchronized.
●
The current capture buffer, if R&SVSE-K18 has not synchronized.
FETCh:POWer:OUTPut:CURRent[:RESult]? on page 153
FETCh:POWer:SENSor:OUT:CURRent[:RESult]? on page 157
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GainAverage gain calculated over all samples of the "Gain Compression" trace.
noise in
output signal
gain
Note that gain is not necessarily equal to the ratio "Power Out" / "Power In".
Gain only describes the ratio of the correlated signal in "Power Out" to "Power
In".
Gain is always referenced to the reference signal power, i.e. when DPD
changes the generator level, the gain is still referenced to the input power of
the reference signal - not the DPD signal.
Example: If the output signal contains the same amount of noise as the correlated signal (e.g. signal is 0 dBm and noise power is also 0 dBm), "Power Out"
will show the sum (3 dBm). However, assuming an input signal power of
-10 dBm, gain will only show 10 dB, not 13 dB.
FETCh:POWer:GAIN:CURRent[:RESult]? on page 152
total output
signal
correlated
output signal
input signal
Crest Factor InCrest factor of the signal at the DUT input. The crest factor is the ratio of the
RMS and peak power.
FETCh:POWer:CFACtor:IN:CURRent[:RESult]? on page 152
Crest Factor OutCrest factor of the signal at the DUT output. The crest factor is the ratio of the
RMS and peak power.
FETCh:POWer:CFACtor:OUT:CURRent[:RESult]? on page 152
AM/AM Curve WidthVertical spread of the samples in the "AM/AM" result display.
The "AM/AM" curve width shows the standard deviation of the output voltage
or the output phase deviation within a +/- 1% range around the mean amplitude in volt.
Output
amplitude
+/- 1%
σ of output
amplitude
in this range
10,5
Input amplitude
linear normalized
FETCh:AMAM:CWIDth:CURRent[:RESult]? on page 151
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AM/PM Curve WidthVertical spread of the samples in the "AM/PM" result display.
The "AM/PM" curve width shows the standard deviation of the output voltage
or the output phase deviation within a +/- 1% range around the mean amplitude in volt.
Output
amplitude
+/- 1%
σ of output
amplitude
in this range
FETCh:AMPM:CWIDth:CURRent[:RESult]? on page 151
10,5
Input amplitude
linear normalized
Compression Point (1 dB / 2
dB / 3 dB)
Input power where the gain deviates by 1 dB, 2 dB or 3 dB from a reference
gain (see "Configuring compression point calculation"on page 110).
In the graphical result, the compression points are indicated by horizontal red
lines.
FETCh:POWer:P1DB:CURRent[:RESult]? on page 153
FETCh:POWer:P2DB:CURRent[:RESult]? on page 154
FETCh:POWer:P3DB:CURRent[:RESult]? on page 154
Output Compression Point
(1 dB / 2 dB / 3 dB)
Output power where the gain deviates by 1 dB, 2 dB or 3 dB from a reference
gain.
Uses identical operating points as "Compression Point (1 dB / 2 dB / 3 dB)",
but is identified by output power at compression point rather than input power.
FETCh:POWer:P1DB:OUT:CURRent[:RESult]? on page 155
FETCh:POWer:P2DB:OUT:CURRent[:RESult]? on page 155
FETCh:POWer:P3DB:OUT:CURRent[:RESult]? on page 156
Occupied BandwidthOccupied bandwidth calculated for the defined evaluation range.
Spectrum FFT
The "Spectrum FFT" result display shows the frequency spectrum of the signal.
The spectrum FFT result shows the signal level in the spectrum around the center fre-
quency. The unit is dBm.
You can display the spectrum of the measured signal and the reference signal. In the
best case, the measured signal has the same shape as the reference signal.
The "Time Domain" result display shows the signal characteristics over time.
It is similar to the "Power vs Time" and "Magnitude Capture" result displays in that it
shows the signal characteristics over time. However, it deliberately shows only a very
short period of the signal. You can thus use it to compare various aspects of the signal,
especially the timing of the displayed signals, in a single result display.
●
Measured signal
Trace 1 shows the characteristics of the measured signal over time. The data
should be the same as the results shown in the "Magnitude Capture" RF result display.
In the best case, the measured signal is the same as the reference signal.
●
Modeled signal
Trace 2 shows the characteristics of the modeled signal. When system modeling
has been turned off, this trace is not displayed.
If the model matches the behavior of the DUT, the characteristics of the signal are
the same as those of the measured signal (minus the noise).
●
Reference signal
Trace 3 shows the characteristics of the reference signal. The reference signal
present at the DUT input represents the ideal signal.
Remote command:
Selection: LAY:ADD? '1',LEFT,TDOM
Result query: TRACe<n>[:DATA]?on page 143
Scale of the x-axis (display settings for the time domain) ← Time Domain
The scale of the x-axis depends on your configuration in the "Display Settings" dialog
box.
The logic is as follows:
●
When you select automatic scaling (➙ "Position: Auto") and synchronization has
failed, the application searches for the peak level in the capture buffer and shows
the signal around the peak for the "Duration" that has been defined.
●
When you select automatic scaling (➙ "Position: Auto") and synchronization is OK,
the application searches for the peak level in the synchronized area of the capture
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buffer and shows the signal around the peak for the "Duration" that has been
defined.
●
When you select manual scaling (➙ "Position: Manual") and synchronization has
failed, the x-axis starts at an "Offset" relative to the first sample in the capture buffer. The end of the x-axis depends on the "Duration" you have defined.
●
When you select manual scaling (➙ "Position: Manual") and synchronization is OK,
the x-axis starts at an "Offset" relative to the first sample in the synchronized area
of the capture buffer. The end of the x-axis depends on the "Duration" you have
defined.
Note: The "Display Settings" for the time domain are only available after you have
selected the "Specifics for: Time Domain" item from the corresponding dropdown menu
at the bottom of the dialog box.
Scale of the y-axis (display settings for the time domain) ← Time Domain
The scale of the y-axis also depends on your configuration.
The signal characteristics displayed in the time domain result display all have a differ-
ent unit. Therefore, the application provides a feature that normalizes all results to 1
(see "Configuring the time domain result display"on page 130). Normalization makes it
easier to compare the timing between the traces. By default, normalization is on. Note
that you can normalize each "Time Domain" window individually.
Unnormalized results are displayed in their respective unit.
Statistics Table
The results for the statistics table are available only after the statistics mode has been
activated using [SENSe:]SWEep:STATistics[:STATe]on page 297. If statistics
mode is switched off, the statistics table stays empty.
Each value in the statistics table has different rows describing a single frame: Average,
Std. Dev, Maximum and Minimum. This is similar to the Numeric Result Summary.
The different color codes represent different result values:
●
Blue
Result of the current result range. The selected values are updated when the user
sweeps through the result range selection.
●
Green
In I/Q averaging mode, the values in the green area are identical to the ones in the
black background area.
In trace statistics mode, the green area refers to all frames of the current capture
buffer, whereas the black area refers to all measured frames (including previous
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capture buffers). Statistics is always done over sweep “Count” frames and then is
being reset, unless the "Continuous Statistics" switch is activated. In this case,
infinite statistics is executed.
●
Black / No selection
Statistical results that can also be based on result ranges that were captured in
previous measurement sweeps.
Remote command:
Adding statistics table: LAY:ADD? '1',LEFT,STAB
Querying results: Chapter 5.4.3.4, "Retrieving results of the statistics table",
on page 174
Configuring statistics table: Chapter 5.6.4, "Configuring the statistics table",
on page 363
Navigating through results ranges found in a capture: CONFigure:RESult:RANGe[:
●Configuring the parameter sweep......................................................................... 113
●Configuring power servoing...................................................................................117
3.1Configuration overview
Throughout the measurement channel configuration, an overview of the most important
currently defined settings is provided in the "Overview". The "Overview" is displayed
when you select the "Overview" icon, which is available at the bottom of all softkey
menus.
In addition to the main measurement settings, the "Overview" provides quick access to
the main settings dialog boxes. The individual configuration steps are displayed in the
order of the data flow. Thus, you can easily configure an entire measurement channel
from input over processing to output and analysis by stepping through the dialog boxes
as indicated in the "Overview".
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Configuration overview
In particular, the "Overview" provides quick access to the following configuration dialog
boxes (listed in the recommended order of processing):
1. Reference Signal
See Chapter 3.2, "Designing a reference signal", on page 35.
2. Input and output
See Chapter 3.3, "Configuring inputs and outputs", on page 45.
3. Trigger
See Chapter 3.4, "Triggering measurements", on page 80.
4. Data Acquisition
See Chapter 3.5, "Configuring the data capture", on page 81.
5. Synchronization, error estimation and compensation
See Chapter 3.7, "Synchronizing measurement data", on page 86.
See Chapter 3.9, "Estimating and compensating signal errors", on page 90.
6. Measurement
Modeling: see Chapter 3.11, "Applying system models", on page 92.
DPD: see Chapter 3.12, "Applying digital predistortion", on page 95.
7. Result configuration
See Chapter 4, "Analysis", on page 119.
8. Display configuration
See Chapter 2, "Measurements and result displays", on page 12.
To configure settings
► Select any button in the "Overview" to open the corresponding dialog box.
Select a setting in the channel bar (at the top of the measurement channel tab) to
change a specific setting.
Preset Channel
Select the "Preset Channel" button in the lower left-hand corner of the "Overview" to
restore all measurement settings in the current channel to their default values.
Remote command:
SYSTem:PRESet:CHANnel[:EXEC] on page 141
Specifics for
The channel can contain several windows for different results. Thus, the settings indicated in the "Overview" and configured in the dialog boxes vary depending on the
selected window.
Select an active window from the "Specifics for" selection list that is displayed in the
"Overview" and in all window-specific configuration dialog boxes.
The "Overview" and dialog boxes are updated to indicate the settings for the selected
window.
Many of the results available in the application require a reference signal that
describes the characteristics of the signal you feed into the amplifier.
The reference signal describes the characteristics of the signal that you feed into the
amplifier and whose amplified version is measured by the application. You can define
any signal you want as a reference signal.
The application provides several methods to design a reference signal:
●
Designing the signal on a generator
(Having a Rohde & Schwarz generator is mandatory for this method.)
●
Designing the signal in a waveform file
●
Designing the signal in the amplifier application
(Having a Rohde & Schwarz generator is mandatory for this method.)
For a list of supported signal generators, refer to the datasheet of the amplifier application.
The remote commands required to configure the reference signal are described in
Chapter 5.5.1, "Designing a reference signal", on page 228.
Reference signal information........................................................................................ 36
Using multi-segment waveform files............................................................................. 36
Transferring the reference signal.................................................................................. 37
Designing a reference signal on a signal generator......................................................38
Designing a reference signal in a waveform file............................................................39
Designing a reference signal within the R&S VSE-K18................................................ 40
└ Signal Bandwidth............................................................................................ 41
└ Maximum Filter Order..................................................................................... 45
Reference signal information
Each tab of the "Reference Signal" dialog box contains some basic information about
the reference signal currently in use.
The information is only displayed when a reference signal has been successfully loaded. When you load a different waveform, the reference signal information is updated
accordingly.
●
Waveform file
Name and path of the waveform file currently in use.
●
Sample rate
The sample rate in the header of the currently used reference signal waveform file
in Hz.
●
Number of samples
Length of the currently used reference signal waveform file in samples.
●
Crest Factor (File)
Crest factor of the whole file currently in use. The crest factor of waveform files is
read from their header. The crest factor of iq.tar files is calculated.
●
Bandwidth (OBW)
The occupied bandwidth of the reference signal currently in use. A calculated
bandwidth that contains 99% of signal power is displayed.
Modern chip technologies implement several communication standards within one chip
and thus increase the requirements in spatial design and test systems. To fulfill the
requirements in the test systems, and to enable a rapid change between different
waveforms containing different test signals, the R&S SMW provides the functionality to
generate multi-segment waveform files. Multi-segment waveform files are files that
contain several different waveforms.
(For more information about creating and using multi-segment waveform files (including examples) refer to the documentation of the R&S SMW.)
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Configuration
Designing a reference signal
When you are testing amplifiers with the amplifier measurement application, you can
use a multi-segment waveform file to create the reference signal. If you use one of
these files, you have to select the segment that you want to use as a reference signal
in the corresponding input field.
Note that the content of the segment you are using for the reference signal must match
the content of the segment used by the ARB of the signal generator. You can select the
segment for the used by the generator in the generator setup.
Remote command:
CONFigure:REFSignal:SEGMent on page 234
Transferring the reference signal
Both the signal generator and analyzer used in the test setup need to know the characteristics of the reference signal.
●
The signal generator needs that information to generate the signal.
●
The analyzer needs that information for the evaluation of the results.
This is why you have to transfer the signal information to both instruments. The transmission is done through a LAN connection that you have to establish when setting up
the measurement. For more information on that see Chapter 3.3.6, "Controlling a sig-
nal generator", on page 61.
●
When you design the reference signal on the signal generator, transfer the signal
information from the generator to the analyzer with the ➙"Read and Load Current
Signal from R&S SMW" button.
You can either design a reference signal with one of the available firmware options
(for example an LTE signal with the R&S SMW-K55) or design a signal in a custom
waveform file. Note that the R&S VSE-K18 does not support all firmware options of
the signal generator.
●
When you load the reference signal from a waveform file or design the signal within
the R&S VSE-K18, transfer the signal information from the analyzer to the generator. Depending on the signal source, you can do this either with the "Load and
Export Selected Waveform File to Generator" or the "Generate and Load Signal
and Export it to Generator" buttons.
When you send the signal information to the generator, the application automatically
configures the generator accordingly.
Transmission state
The LED displayed with the transmission button shows the state of the reference signal
transmission.
The LED is either gray, green or red:
●
Grey LED
Transmission state unknown (for example when you have not yet started the transmission).
●
Green LED
Transmission has been successful.
●
Red LED
Transmission has not been successful.
Check if the generator IP address / computer name are correct and if the connection has been established.
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Designing a reference signal
Designing a reference signal on a signal generator
One way to design a reference signal is to design the signal on the signal generator
itself.
You can design any signal you like, as long as it is storable as an arbitrary waveform
(ARB) file. When you are done, you have to transfer the signal information from the
signal generator to the signal analyzer with the "Read from Generator, Load" button.
The "Force ARB Mode" switch forces the signal generator to use its ARB mode (arbitrary waveform) rather than its real-time mode, whenever possible. As a result, switching between DPD on and off state is significantly faster. When the "Force ARB Mode"
function is used, the peak power of the generator is read out and used within the process but as a result of this function the RMS power of the generator is modified. Also
the waveform header of the file is recalculated to make sure that the peak input level
stays constant or lower than the gain expansion during DPD calculation.
The parameters of the currently active reference signal are described in "Reference
signal information"on page 36.
The "Open Generator Control" button provides functionality to change the generator
settings as described in Chapter 3.3.6, "Controlling a signal generator", on page 61.
Most of the options available for the connected generator are supported by the automatic signal import functionality of the R&S VSE-K18. If the signal import was not successful (indicated by a red LED), you have to transfer the reference signal in another
way (for example with a memory stick).
For a comprehensive description of all features available on the signal generator and
information on how to generate signals, refer to the documentation of the signal generator.
Remote command:
See signal generator documentation.
CONFigure:REFSignal:CGW:AMODe[:STATe] on page 229
CONFigure:REFSignal:CGW:READ on page 229
CONFigure:REFSignal:CGW:LEDState? on page 229
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Configuration
Designing a reference signal
Designing a reference signal in a waveform file
One way to design a reference signal is to define its characteristics in a waveform file
(*.wv or *.iq.tar).
You can create a waveform file, for example:
●
With the R&S®WinIQSIM2 software package
●
By exporting a signal designed on the signal generator
Basically, this file contains the characteristics of the reference signal. The generator
then generates the reference signal based on the information in the file.
There are two ways to generate the reference signal through a custom waveform file.
●
The generator is connected to the R&S VSE in a LAN, and can be recognized by
the R&S VSE-K18 (Rohde & Schwarz generators only, for example the R&S SMW)
In that case, you can simply transfer the reference signal information to the generator with the features integrated into the R&S VSE-K18. The generator then generates the corresponding signal with the appropriate signal level, and the R&S VSEK18 is able to compare the measured signal to the ideal reference signal.
●
The generator is not connected to the R&S VSE
In that case, you have to load the reference signal information onto the generator
manually and turn off the "Export to Generator" function. Because no exchange of
information is possible between generator and analyzer, it is required to specify the
input level of the signal in the "DUT Peak Input Power" input field.
The parameters of the currently active reference signal are described in "Reference
signal information"on page 36.
The "Open Generator Control" button provides functionality to change the generator
settings as described in Chapter 3.3.6, "Controlling a signal generator", on page 61.
For a comprehensive description of all features available on the signal generator and
information on how to generate and export signals to a file, refer to the documentation
of the signal generator.
To transfer a waveform file from the analyzer to the generator and process it with the
ARB generator of the R&S SMW, for example, proceed as follows:
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Configuration
Designing a reference signal
▶ In the "Custom Waveform" tab, select a file via the "Load, Play on Generator" button.
▶ Transfer the file to the generator with the "Select" button.
If a waveform is only used as a reference without transferring it to the signal generator,
make sure that the generator control state "Off" is selected in the generator setup dialog.
Designing a reference signal within the R&S VSE-K18
One way to design a reference signal is to design the signal within the R&S VSE-K18.
The application provides functionality to design a basic reference signal and saves the
signal characteristics in a waveform file which you have to transfer to the signal generator with the "Generate and Load Signal and Export it to Generator" button.
When the data has been transferred, the signal generator (for example the R&S SMW)
generates the corresponding signal.
The generated signal is a pseudo-noise signal, whose basic properties, like crest factor
and bandwidth, you can specify as required.
The parameters of the currently active reference signal are described in "Reference
signal information"on page 36.
The "Open Generator Control" button provides functionality to change the generator
settings as described in Chapter 3.3.6, "Controlling a signal generator", on page 61.
Table 3-1: Parameter dependencies
ParameterMin ValueMax Value
Target Crest Factor213
Signal Length((N+2*RampLength)*100)/Pulse-
DutyCycle
N=1000 for Target Crest Factor
< 12.5 dB
N=25000 for Target Crest Factor
≥ 12.5 dB
Notch WidthSignal Bandwidth/100Signal Bandwidth
Ramp Length
0 if Pulse Duty Cycle is 100 %
Otherwise (Signal Length*Pulse-
DutyCycle/100-N)/2
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Configuration
Designing a reference signal
To generate a reference signal within the application, proceed as follows:
▶ In the "Generate Own Signal" tab, design the reference signal as required.
The application stores the current signal properties as an ARB signal in a waveform
file.
▶ Upload the data to the generator with the "Generate, Play on Generator" button.
You can define the following signal characteristics.
●
"Signal Bandwidth"on page 41
●
"Pulse Duty Cycle"on page 41
●
"Signal Length"on page 42
●
"Ramp Length"on page 42
●
"Target Crest Factor"on page 42
●
"Waveform File Name"on page 42
●
"Notch Width"on page 42
●
"Notch Position"on page 43
Remote command:
CONFigure:REFSignal:GOS:WRITe on page 234
CONFigure:REFSignal:GOS:LEDState? on page 232
Signal Bandwidth ← Designing a reference signal within the R&S VSE-K18
Defines the bandwidth of the reference signal.
The bandwidth should not be larger than maximum I/Q bandwidth supported by your
signal analyzer (which depends on the analyzer configuration).
Remote command:
CONFigure:REFSignal:GOS:BWIDth on page 231
Pulse Duty Cycle ← Designing a reference signal within the R&S VSE-K18
Defines the duty cycle of a pulsed reference signal.
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Configuration
Designing a reference signal
The duty cycle of a pulse is the ratio of the pulse duration and the actual length of the
pulse. A duty cycle of 100 % corresponds to a continuous signal.
Example:
The pulse duration is 2 μs. The actual length of the pulse is 1 μs. The duty cycle is
1 μs : 2 μs = 0.5 or 50 %.
Remote command:
CONFigure:REFSignal:GOS:DCYCle on page 232
Signal Length ← Designing a reference signal within the R&S VSE-K18
Defines the number of samples that the reference signal consists of.
A number that is a power of 2 speeds up the internal signal processing. Thus, such a
number should be specified if no other requirements limit the choice of the sample
count.
For more information, see "Pulse Duty Cycle"on page 41.
Remote command:
CONFigure:REFSignal:GOS:SLENgth on page 233
Ramp Length ← Designing a reference signal within the R&S VSE-K18
Defines the number of samples used to ramp up the pulse to its full power and vice
versa.
Remote command:
CONFigure:REFSignal:GOS:RLENgth on page 233
Target Crest Factor ← Designing a reference signal within the R&S VSE-K18
Defines the crest factor of the reference signal.
The crest factor shows the RMS power in relation to the peak power.
The crest factor is defined for a signal with 100 % pulse duty cycle and 0 Hz notch.
Changes to the pulse duty cycle and notch parameters will change the crest factor.
Remote command:
CONFigure:REFSignal:GOS:CRESt on page 231
Waveform File Name ← Designing a reference signal within the R&S VSE-K18
Defines the name of the waveform file that the reference ARB signal configuration is
stored in.
Remote command:
CONFigure:REFSignal:GOS:WNAMe on page 234
Notch Width ← Designing a reference signal within the R&S VSE-K18
Defines the width of a notch that you can add to the reference signal.
Within the notch, all carriers of the reference signal have zero amplitude. You can use
the noise notch to, for example, determine the noise power ratio (NPR) before and
after the DPD.
Remote command:
CONFigure:REFSignal:GOS:NWIDth on page 233
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Designing a reference signal
Notch Position ← Designing a reference signal within the R&S VSE-K18
Defines an offset for the noise notch relative to the center frequency.
The offset moves the notch to a position outside the center of the signal. You can use
the offset to, for example, generate a one-sided noise signal or to examine asymmetric
distortion effects.
Remote command:
CONFigure:REFSignal:GOS:NPOSition on page 232
Crest Factor Reduction (Generator Option K548)
The Crest Factor Reduction dialog provides functionality to control the main parameters of a Rohde & Schwarz signal generator equipped with option K548.
Enables the crest factor reduction calculation.
If "On" is selected and all input fields are editable, crest factor reduction is active on the
generator but the R&S VSE-K18 application has no CFR reference yet.
If "On" is selected and "Read CFR from Generator, Load" is selected, all input fields
are grayed out. The CFR reference can now be used by the R&S VSE-K18 application.
Remote command:
CONFigure:CFReduction[:STATe] on page 236
CONFigure:CFReduction[:STATe]:LEDState? on page 236
EVM Ref. Signal ← Crest Factor Reduction (Generator Option K548)
Loads a new ARB file as reference if "CFR" is selected. The original ARB file is stored.
Remote command:
Sets the value difference by which you want to change your crest factor.
Remote command:
CONFigure:CFReduction:CFDelta on page 239
CONFigure:CFReduction:CFDelta:LEDState? on page 239
Current Crest Factor ← Crest Factor Reduction (Generator Option K548)
Displays the current crest factor of the waveform after the calculation of the resulting
crest factor is completed.
Remote command:
CONFigure:CFReduction:CCFactor? on page 239
Max Iterations ← Crest Factor Reduction (Generator Option K548)
Sets the number of iterations that are used for calculating the resulting crest factor. The
iteration process is stopped when the desired crest factor delta is achieved by 0.1 dB.
Remote command:
CONFigure:CFReduction:ITERations on page 237
CONFigure:CFReduction:ITERations:LEDState? on page 237
Selects which filter mode is used for the filtering. In "Simple" mode, you can specify the
RF bandwidth and channel spacing of the signal. The lowpass filter is designed to pass
through frequency components inside the signal bandwidth and suppress components
in the adjacent channel. In "Enhanced" mode, you can specify the passband and stopband frequencies of the lowpass filter.
Remote command:
CONFigure:CFReduction:FILTer on page 238
CONFigure:CFReduction:FILTer:LEDState? on page 238
Signal Bandwidth ← Crest Factor Reduction (Generator Option K548)
Sets the signal bandwidth. The value of the "Signal Bandwidth" should not be higher
than the "Channel Spacing".
When in automatic mode, "Signal Bandwidth" shall be set to the OBW value of the reference file (shown in reference signal overview).
"Channel Spacing" shall be set to 1.15 times this value.
Remote command:
CONFigure:CFReduction:SBANdwidth on page 236
CONFigure:CFReduction:SBANdwidth:AUTO on page 237
CONFigure:CFReduction:SBANdwidth:LEDState? on page 237
The default input source for the connected instrument is "Radio Frequency". Depending on the connected instrument, different input parameters are available.
Figure 3-1: RF input source settings for an R&S FSW with B2000 option
If the Frequency Response Correction option (R&S VSE-K544) is installed, the Amplifier measurement application also supports frequency response correction using
Touchstone (.snp) files or .fres files.
Input Type (Instrument / File)........................................................................................46
10 dB Minimum Attenuation..........................................................................................50
Input Type (Instrument / File)
Selects an instrument or a file as the type of input provided to the channel.
Note: External mixers are only available for input from a connected instrument.
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Configuration
Configuring inputs and outputs
Note: If the R&S VSE software is installed directly on an instrument, or integrated in
Cadence®AWR®VSS, some restrictions apply on the available input type.
Remote command:
INSTrument:BLOCk:CHANnel[:SETTings]:SOURce<si> on page 261
INPut<ip>:SELect on page 260
Instrument
Specifies a configured instrument to be used for input.
Input 1 / Input 2
For instruments with two input connectors, you must define which input source is used
for each measurement channel.
Note that you cannot use both RF inputs simultaneously.
"Input 1"
R&S FSW85: 1.00 mm RF input connector for frequencies up to
85 GHz (90 GHz with option R&S FSW-B90G)
"Input2"
Remote command:
INPut<ip>:TYPE on page 261
Input Coupling
The RF input of the R&S VSE can be coupled by alternating current (AC) or direct current (DC).
The RF input of the connected instrument can be coupled by alternating current (AC)
or direct current (DC).
For an active external frontend, input coupling is always DC.
AC coupling blocks any DC voltage from the input signal. AC coupling is activated by
default to prevent damage to the instrument. Very low frequencies in the input signal
can be distorted.
However, some specifications require DC coupling. In this case, you must protect the
instrument from damaging DC input voltages manually. For details, refer to the data
sheet.
Remote command:
INPut<ip>:COUPling<ant> on page 256
Impedance
For some measurements, the reference impedance for the measured levels of the connected instrument can be set to 50 Ω or 75 Ω.
R&S FSW85: 1.85 mm RF input connector for frequencies up to
67 GHz
Select 75 Ω if the 50 Ω input impedance is transformed to a higher impedance using a
75 Ω adapter of the RAZ type. (That corresponds to 25Ω in series to the input impedance of the instrument.) The correction value in this case is 1.76 dB = 10 log (75Ω/
50Ω).
Remote command:
INPut<ip>:IMPedance<ant> on page 258
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Configuration
Configuring inputs and outputs
Direct Path
Enables or disables the use of the direct path for small frequencies.
In spectrum analyzers, passive analog mixers are used for the first conversion of the
input signal. In such mixers, the LO signal is coupled into the IF path due to its limited
isolation. The coupled LO signal becomes visible at the RF frequency 0 Hz. This effect
is referred to as LO feedthrough.
To avoid the LO feedthrough the spectrum analyzer provides an alternative signal path
to the A/D converter, referred to as the direct path. By default, the direct path is
selected automatically for RF frequencies close to zero. However, this behavior can be
disabled. If "Direct Path" is set to "Off" , the spectrum analyzer always uses the analog
mixer path.
For an active external frontend, the direct path is always used automatically for frequencies close to zero.
"Auto"
"Off"
Remote command:
INPut<ip>:DPATh on page 256
(Default) The direct path is used automatically for frequencies close
to zero.
The analog mixer path is always used.
High Pass Filter 1 to 3 GHz
Activates an additional internal highpass filter for RF input signals from 1 GHz to
3 GHz. This filter is used to remove the harmonics of the analyzer to measure the harmonics for a DUT, for example.
For some connected instruments, this function requires an additional hardware option
on the instrument.
Note: For RF input signals outside the specified range, the high-pass filter has no
effect. For signals with a frequency of approximately 4 GHz upwards, the harmonics
are suppressed sufficiently by the YIG-preselector, if available.)
Remote command:
INPut<ip>:FILTer:HPASs[:STATe] on page 257
YIG-Preselector
Enables or disables the YIG-preselector.
This setting requires an additional option on the connected instrument.
An internal YIG-preselector at the input of the connected instrument ensures that
image frequencies are rejected. However, image rejection is only possible for a restricted bandwidth. To use the maximum bandwidth for signal analysis you can disable the
YIG-preselector at the input of the connected instrument, which can lead to image-frequency display.
Note: Note that the YIG-preselector is active only higher frequencies, depending on
the connected instrument. Therefore, switching the YIG-preselector on or off has no
effect if the frequency is below that value.
To use the optional 90 GHz frequency extension (R&S FSW-B90G), the YIG-preselector must be disabled.
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To use the optional 54 GHz frequency extension (R&S FSV3-B54G), the YIG-preselector must be disabled.
Remote command:
INPut<ip>:FILTer:YIG[:STATe] on page 257
B2000 State
Activates the optional 2 GHz bandwidth extension (R&S FSW-B2000).
Note: The R&S VSE software supports input from a connected R&SFSW with a
B2000 option installed. However, the R&S FSW interface to the oscilloscope must be
set up and aligned directly on the instrument before the R&S VSE software can start
analyzing the input.
The analysis bandwidth is defined in the data acquisition settings of the application as
usual. Note that the maximum bandwidth cannot be restricted manually as for other
bandwidth extension options.
Manual operation on the connected oscilloscope, or remote operation other than by the
R&S VSE, is not possible while the B2000 option is active.
Remote command:
SYSTem:COMMunicate:RDEVice:OSCilloscope[:STATe] on page 263
Oscilloscope Splitter Mode
Activates the use of the power splitter inserted between the [IF 2 GHZ OUT] connector
of the R&S FSW and the [CH1] and [CH3] input connectors of the oscilloscope. Note
that this mode requires an additional alignment with the power splitter.
For details see the R&S FSW I/Q Analyzer and I/Q Input User Manual.
Remote command:
SYSTem:COMMunicate:RDEVice:OSCilloscope:PSMode[:STATe] on page 264
Oscilloscope IP Address
When using the optional 2 GHz bandwidth extension (R&S FSW-B2000) with an R&S
FSW as the connected instrument, the entire measurement, as well as both instruments, are controlled by the R&S VSE software. Thus, the instruments must be connected via LAN, and the TCPIP address of the oscilloscope must be defined in the
R&S VSE software.
For tips on how to determine the computer name or TCPIP address, see the oscilloscope's user documentation.
Remote command:
SYSTem:COMMunicate:RDEVice:OSCilloscope:TCPip on page 263
Preselector State
Turns the preselector on and off.
When you turn on the preselector, you can configure the characteristics of the prese-
lector and add the preamplifier into the signal path.
When you turn off the preselector, the signal bypasses the preselector and the pream-
plifier, and is fed into the input mixer directly.
Remote command:
INPut<ip>:PRESelection[:STATe] on page 258
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Preselector Mode
Selects the preselection filters to be applied to the measurement.
"Auto"
"Auto Wide"
"Auto Narrow"
"Manual"
Remote command:
INPut<ip>:PRESelection:SET on page 258
Automatically applies all available bandpass filters in a measurement.
Available with the optional preamplifier.
Automatically applies the wideband filters consecutively:
●
Lowpass 40 MHz
●
Bandpass 30 MHz to 2250 MHz
●
Bandpass 2 GHz to 8 GHz
●
Bandpass 8 GHz to 26.5 GHz
Available with the optional preselector.
Automatically applies the most suitable narrowband preselection fil-
ters in a measurement, depending on the bandwidth you have
selected.
For measurement frequencies up to 30 MHz, the connected instrument uses combinations of lowpass and highpass filters. For higher
frequencies, the connected instrument uses bandpass filters.
Available with the optional preselector.
Applies the filter settings you have defined manually.
Configuration
10 dB Minimum Attenuation
Turns the availability of attenuation levels of less than 10 dB on and off.
When you turn on this feature, the attenuation is always at least 10 dB. This minimum
attenuation protects the input mixer and avoids accidental setting of 0 dB, especially if
you measure EUTs with high RFI voltage.
When you turn it off, you can also select attenuation levels of less than 10 dB.
The setting applies to a manual selection of the attenuation as well as the automatic
selection of the attenuation.
Remote command:
INPut<ip>:ATTenuation:PROTection:RESet on page 255
You can load a file simply by selecting it in a file explorer and dragging it to the
R&S VSE software. Drop it into the "Measurement Group Setup" window or the channel bar for any channel. The channel is automatically configured for file input, if necessary. If the file contains all essential information, the file input is immediately displayed
in the channel. Otherwise, the "Recall I/Q Recording" dialog box is opened for the
selected file so you can enter the missing information.
If the file contains data from multiple channels (e.g. from LTE measurements), it can be
loaded to individual input sources, if the application supports them.
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The "Input Source" settings defined in the "Input" dialog box are identical to those configured for a specific channel in the "Measurement Group Setup" window.
If the Frequency Response Correction option (R&S VSE-K544) is installed, the Amplifier measurement application also supports frequency response correction using
Touchstone (.snp) files or .fres files.
Encrypted .wv files can also be imported. Note, however, that traces resulting from
encrypted file input cannot be exported or stored in a saveset.
Input Type (Instrument / File)........................................................................................51
Zero Padding.................................................................................................................52
Input Type (Instrument / File)
Selects an instrument or a file as the type of input provided to the channel.
Note: External mixers are only available for input from a connected instrument.
Note: If the R&S VSE software is installed directly on an instrument, or integrated in
Cadence®AWR®VSS, some restrictions apply on the available input type.
Remote command:
INSTrument:BLOCk:CHANnel[:SETTings]:SOURce<si> on page 261
INPut<ip>:SELect on page 260
Input File
Specifies the I/Q data file to be used for input.
Select "Select File" to open the "Load I/Q File" dialog box.
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Zero Padding
Enables or disables zero padding for input from an I/Q data file that requires resampling. For resampling, a number of samples are required due to filter settling. These
samples can either be taken from the provided I/Q data, or the software can add the
required number of samples (zeros) at the beginning and end of the file.
If enabled, the required number of samples are inserted as zeros at the beginning and
end of the file. The entire input data is analyzed. However, the additional zeros can
effect the determined spectrum of the I/Q data. If zero padding is enabled, a status
message is displayed.
If disabled (default), no zeros are added. The required samples for filter settling are
taken from the provided I/Q data in the file. The start time in the R&S VSE Player is
adapted to the actual start (after filter settling).
Note: You can activate zero padding directly when you load the file, or afterwards in
the "Input Source" settings.
The "Frequency" tab of the "Input / Output" dialog box contains settings to configure
frequency characteristics.
The frequency settings are similar to those available in the spectrum application. For a
comprehensive description of these settings, refer to the R&S VSE user manual.
The remote commands required to configure the frequency are described in Chap-
ter 5.5.4, "Configuring the frequency", on page 275.
Center Frequency......................................................................................................... 52
Center Frequency Stepsize...........................................................................................53
Frequency Offset ..........................................................................................................53
Center Frequency
Defines the frequency of the measured signal.
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The possible value range depends on the R&S VSE model you have. See the data
sheet for more information about the supported frequency range.
Remote command:
[SENSe:]FREQuency:CENTer on page 275
Center Frequency Stepsize
Defines the step size by which the center frequency is increased or decreased when
the arrow keys are pressed.
When you use the rotary knob the center frequency changes in steps of only 1/10 of
the "Center Frequency Stepsize".
"= Center"
"Manual"
Remote command:
[SENSe:]FREQuency:CENTer:STEP on page 275
Sets the step size to the value of the center frequency and removes
the coupling of the step size to span or resolution bandwidth. The
used value is indicated in the "Value" field.
Defines a fixed step size for the center frequency. Enter the step size
in the "Value" field.
Frequency Offset
Shifts the displayed frequency range along the x-axis by the defined offset.
This parameter has no effect on the instrument's hardware, on the captured data, or on
data processing. It is simply a manipulation of the final results in which absolute frequency values are displayed. Thus, the x-axis of a spectrum display is shifted by a
constant offset if it shows absolute frequencies. However, if it shows frequencies relative to the signal's center frequency, it is not shifted.
A frequency offset can be used to correct the display of a signal that is slightly distorted
by the measurement setup, for example.
The allowed values range from -1 THz to 1 THz. The default setting is 0 Hz.
Remote command:
The "Amplitude" tab of the "Input / Output" dialog box contains settings to configure the
signal level characteristics.
The level settings are the same as those available in the spectrum application. For a
comprehensive description of these settings, refer to the R&S VSE user manual.
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The remote commands required to configure the amplitude are described in Chap-
ter 5.5.5, "Defining level characteristics", on page 276.
Functions available in the "Amplitude" dialog box described elsewhere:
Attenuation Mode / Value ............................................................................................. 56
Using Electronic Attenuation ........................................................................................56
Reference Level
Defines the expected maximum input signal level. Signal levels above this value are
possibly not measured correctly, which is indicated by the "IF Overload" status display.
Defines the expected maximum reference level. Signal levels above this value are possibly not measured correctly. Signals above the reference level are indicated by an "IF
Overload" status display.
The reference level can also be used to scale power diagrams; the reference level is
then used for the calculation of the maximum on the y-axis.
Since the hardware of the connected instrument is adapted according to this value, it is
recommended that you set the reference level close above the expected maximum signal level. Thus you ensure an optimum measurement (no compression, good signal-tonoise ratio).
Note: Note that for input from the External Mixer (R&S VSE-B21) the maximum refer-
ence level also depends on the conversion loss; see the R&S VSE base software user
manual for details.
For an active external frontend, the reference level refers to the RF input at the external frontend, not the levels at the RF input of the connected instrument.
Remote command:
DISPlay[:WINDow<n>][:SUBWindow<w>]:TRACe<t>:Y[:SCALe]:
RLEVel<ant> on page 276
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Shifting the Display ( Offset ) ← Reference Level
Defines an arithmetic level offset. This offset is added to the measured level. In some
result displays, the scaling of the y-axis is changed accordingly.
Define an offset if the signal is attenuated or amplified before it is fed into the R&S VSE
so the application shows correct power results. All displayed power level results are
shifted by this value.
The reference level offset takes level offsets into account that occur after the signal has
passed through the DUT (usually an amplifier). For level offsets occurring before the
DUT, you can define a level offset on the signal generator from within the R&S VSEK18 user interface.
The setting range is ±200 dB in 0.01 dB steps.
Note, however, that the internal reference level (used to adjust the hardware settings to
the expected signal) ignores any "Reference Level Offset" . Thus, it is important to
keep in mind the actual power level the R&S VSE must handle. Do not rely on the displayed reference level (internal reference level = displayed reference level - offset).
Remote command:
DISPlay[:WINDow<n>][:SUBWindow<w>]:TRACe<t>:Y[:SCALe]:
RLEVel<ant>:OFFSet on page 277
Input Coupling
The RF input of the R&S VSE can be coupled by alternating current (AC) or direct current (DC).
The RF input of the connected instrument can be coupled by alternating current (AC)
or direct current (DC).
For an active external frontend, input coupling is always DC.
AC coupling blocks any DC voltage from the input signal. AC coupling is activated by
default to prevent damage to the instrument. Very low frequencies in the input signal
can be distorted.
However, some specifications require DC coupling. In this case, you must protect the
instrument from damaging DC input voltages manually. For details, refer to the data
sheet.
Remote command:
INPut<ip>:COUPling<ant> on page 256
Impedance
For some measurements, the reference impedance for the measured levels of the connected instrument can be set to 50 Ω or 75 Ω.
Select 75 Ω if the 50 Ω input impedance is transformed to a higher impedance using a
75 Ω adapter of the RAZ type. (That corresponds to 25Ω in series to the input impedance of the instrument.) The correction value in this case is 1.76 dB = 10 log (75Ω/
50Ω).
Remote command:
INPut<ip>:IMPedance<ant> on page 258
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Attenuation Mode / Value
The RF attenuation can be set automatically as a function of the selected reference
level (Auto mode). Automatic attenuation ensures that no overload occurs at the RF
Input connector for the current reference level. It is the default setting.
In "Manual" mode, you can set the RF attenuation in 1 dB steps (down to 0 dB). Other
entries are rounded to the next integer value. The range is specified in the data sheet.
If the defined reference level cannot be set for the defined RF attenuation, the reference level is adjusted accordingly and the warning "limit reached" is displayed.
NOTICE! Risk of hardware damage due to high power levels. When decreasing the
attenuation manually, ensure that the power level does not exceed the maximum level
allowed at the RF input, as an overload can lead to hardware damage.
Remote command:
INPut<ip>:ATTenuation on page 277
INPut<ip>:ATTenuation:AUTO on page 278
Using Electronic Attenuation
If the (optional) Electronic Attenuation hardware is installed on the connected instrument, you can also activate an electronic attenuator.
In "Auto" mode, the settings are defined automatically; in "Manual" mode, you can
define the mechanical and electronic attenuation separately.
For an active external frontend, electronic attenuation is not available.
Note: Note that restrictions can apply concerning which frequencies electronic attenua-
tion is available for, depending on which instrument is connected to the R&S VSE software. Check your instrument documentation for details.
In "Auto" mode, RF attenuation is provided by the electronic attenuator as much as
possible to reduce the amount of mechanical switching required. Mechanical attenuation can provide a better signal-to-noise ratio, however.
When you switch off electronic attenuation, the RF attenuation is automatically set to
the same mode (auto/manual) as the electronic attenuation was set to. Thus, the RF
attenuation can be set to automatic mode, and the full attenuation is provided by the
mechanical attenuator, if possible.
If the defined reference level cannot be set for the given attenuation, the reference
level is adjusted accordingly and the warning "limit reached" is displayed in the status
bar.
Remote command:
INPut<ip>:EATT:STATe on page 279
INPut<ip>:EATT:AUTO on page 279
INPut<ip>:EATT on page 279
3.3.4Power sensors
Access: "Overview" > "Input" > "Power Sensor" tab
A typical measurement using power sensors in the R&S VSE-K18 application is set up
as shown below:
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For details on working with power sensors, see the R&S VSE User Manual.
Input and output sensors are configured individually on a separate tab.
Switches the power measurement for all power sensors on or off. Note that in addition
to this general setting, each power sensor can be activated or deactivated individually
by the Select setting on each tab. However, the general setting overrides the individual
settings.
Apply Auto Level Correction
This function can be activated after "Auto Set Level Correction" has been used.
If the input sensor is selected, the input power used to calculate the measurement
results is corrected so that it corresponds to the value measured by the input power
sensor.
If the output sensor is selected, the power measured on the analyzer is corrected so
that it corresponds to the value measured by the output power sensor.
Remote command:
CALCulate:PMETer:LEVel:CORRection on page 250
[SENSe:]PMETer:LEVel:CORRection:APPLy on page 249
Select
Selects the individual power sensor for usage if power measurement is generally activated ( State function).
The detected serial numbers of the power sensors connected to the instrument are
provided in a selection list. For each of the four available power sensor indexes
( "Power Sensor 1" ... "Power Sensor 4" ), which correspond to the tabs in the configuration dialog, one of the detected serial numbers can be assigned. The physical sensor
is thus assigned to the configuration setting for the selected power sensor index.
By default, serial numbers not yet assigned are automatically assigned to the next free
power sensor index for which "Auto Assignment" is selected.
Alternatively, you can assign the sensors manually by deactivating the "Auto" option
and selecting a serial number from the list.
Remote command:
[SENSe:]PMETer<p>[:STATe] on page 249
SYSTem:COMMunicate:RDEVice:PMETer<p>:DEFine on page 243
SYSTem:COMMunicate:RDEVice:PMETer<p>:CONFigure:AUTO[:STATe]
on page 242
SYSTem:COMMunicate:RDEVice:PMETer<p>:COUNt? on page 243
Zeroing Power Sensor
Starts zeroing of the power sensor.
For details on the zeroing process refer to the R&S VSE User Manual.
Remote command:
CALibration:PMETer<p>:ZERO:AUTO ONCE on page 244
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Frequency Manual
Defines the frequency of the signal to be measured. The power sensor has a memory
with frequency-dependent correction factors. This allows extreme accuracy for signals
of a known frequency.
Remote command:
[SENSe:]PMETer<p>:FREQuency on page 246
Frequency Coupling
Selects the coupling option. The frequency can be coupled automatically to the center
frequency of the instrument or to the frequency of marker 1.
Remote command:
[SENSe:]PMETer<p>:FREQuency:LINK on page 247
Unit/Scale
Selects the unit with which the measured power is to be displayed. Available units are
dBm, dB, W and %.
If dB or % is selected, the display is relative to the reference value that is defined with
either the "Meas -> Ref" setting or the "Reference Value" setting.
Remote command:
UNIT<n>:PMETer<p>:POWer on page 251
UNIT<n>:PMETer<p>:POWer:RATio on page 251
Meas Time/Average
Selects the measurement time or switches to manual averaging mode. In general,
results are more precise with longer measurement times. The following settings are
recommended for different signal types to obtain stable and precise results:
"Short"
"Normal"
"Long"
"Manual"
Remote command:
[SENSe:]PMETer<p>:MTIMe on page 247
[SENSe:]PMETer<p>:MTIMe:AVERage[:STATe] on page 248
Setting the Reference Level from the Measurement Meas -> Ref
Sets the currently measured power as a reference value for the relative display. The
reference value can also be set manually via the Reference Value setting.
Remote command:
CALCulate<n>:PMETer<p>:RELative[:MAGNitude]:AUTO ONCE on page 245
Stationary signals with high power (> -40dBm), because they require
only a short measurement time and short measurement time provides
the highest repetition rates.
Signals with lower power or modulated signals
Signals at the lower end of the measurement range (<-50 dBm) or
Signals with lower power to minimize the influence of noise
Manual averaging mode. The average count is set with the Average
Count ( Number of Readings ) setting.
Reference Value
Defines the reference value in dBm used for relative power meter measurements.
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Remote command:
CALCulate<n>:PMETer<p>:RELative[:MAGNitude] on page 244
Use Ref Level Offset
If deactivated, takes the Sensor Level Offset into account.
Remote command:
[SENSe:]PMETer<p>:ROFFset[:STATe] on page 248
Sensor Level Offset
Takes the specified offset into account for the measured power. Only available if Use
Ref Level Offset is disabled.
Remote command:
[SENSe:]PMETer<p>:SOFFset on page 249
Average Count ( Number of Readings )
Defines the number of readings (averages) to be performed after a single sweep has
been started. This setting is only available if manual averaging is selected ( Meas
Time/Average setting).
The values for the average count range from 0 to 256 in binary steps (1, 2, 4, 8, …).
For average count = 0 or 1, one reading is performed. The general averaging and
sweep count for the trace are independent from this setting.
Results become more stable with extended average, particularly if signals with low
power are measured. This setting can be used to minimize the influence of noise in the
power sensor measurement.
Remote command:
[SENSe:]PMETer<p>:MTIMe:AVERage:COUNt on page 248
Duty Cycle
Sets the duty cycle to a percent value for the correction of pulse-modulated signals and
activates the duty cycle correction. With the correction activated, the sensor calculates
the signal pulse power from this value and the mean power.
Remote command:
[SENSe:]PMETer<p>:DCYCle[:STATe] on page 246
[SENSe:]PMETer<p>:DCYCle:VALue on page 246
Using the power sensor as an external trigger
If activated, the power sensor creates a trigger signal when a power higher than the
defined "External Trigger Level" is measured. This trigger signal can be used as an
external power trigger by the connected instrument.
This setting is only available in conjunction with a compatible power sensor.
Remote command:
[SENSe:]PMETer<p>:TRIGger[:STATe] on page 253
TRIG:SOUR PSE, see TRIGger[:SEQuence]:SOURce on page 250
External Trigger Level ← Using the power sensor as an external trigger
Defines the trigger level for the power sensor trigger.
For details on supported trigger levels, see the data sheet.
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Remote command:
[SENSe:]PMETer<p>:TRIGger:LEVel on page 253
Hysteresis ← Using the power sensor as an external trigger
Defines the distance in dB to the trigger level that the trigger source must exceed
before a trigger event occurs. Setting a hysteresis avoids unwanted trigger events
caused by noise oscillation around the trigger level.
Remote command:
[SENSe:]PMETer<p>:TRIGger:HYSTeresis on page 252
Trigger Holdoff ← Using the power sensor as an external trigger
Defines the minimum time (in seconds) that must pass between two trigger events.
Trigger events that occur during the holdoff time are ignored.
Remote command:
[SENSe:]PMETer<p>:TRIGger:HOLDoff on page 252
Drop-Out Time ← Using the power sensor as an external trigger
Defines the time the input signal must stay below the trigger level before triggering
again.
Slope ← Using the power sensor as an external trigger
Defines whether triggering occurs when the signal rises to the trigger level or falls
down to it.
Remote command:
[SENSe:]PMETer<p>:TRIGger:SLOPe on page 253
3.3.5Configuring outputs
Access: "Overview" > "Input / Output" > "Output"
The "Output" tab of the "Input / Output" dialog box contains settings to configure the
various signal outputs available on the R&S VSE.
The functionality is the same as in the spectrum application. For more information
about the output functions, refer to the R&S VSE user manual.
The "Generator Setup" tab of the "Input / Output" dialog box contains settings to control the signal generator from within the R&S VSE-K18. A remote control connection
between the R&S VSE and the signal generator has to be established to be able to do
so.
Because a signal generator is (mostly) mandatory in the test setup, these features
make measurement configuration as easy as possible. This way, you can control both
analyzer and generator from within the application without having to operate the two
instruments to configure the measurement.
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While generator control is active, you cannot change the connection information.
When you switch on generator control while it is still active in another channel, the con-
trol is disabled in the other channel. Only one channel can control a generator at any
time.
The remote commands required to configure the generator are described in Chap-
ter 5.5.6, "Controlling a signal generator", on page 282.
State of operation
Most settings have an LED that shows the state of the corresponding setting on the
signal generator.
The LED is either gray, green or red:
●
Grey LED
Configuration state unknown (for example when you have not yet started the transmission).
●
Green LED
Configuration has been successful. Generator has been configured correctly.
●
Red LED
Configuration has not been successful.
Check if the connection between analyzer and generator has been established or if
the IP address has been stated correctly.
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The "Generator Control" functions are activated, when a signal generator is selected in
the RF generator selection box:
If no signal generator is selected ("NONE"), the "Generator Control" functions are
turned off.
Generator details
The "Generator Details" contain information about the connected signal generator, like
the software version or the serial number of the generator.
Updating generator settings
When you change the generator level or frequency in this dialog, the application automatically updates those settings on the generator.
When you use the "Upload All Settings To Generator" button, you can force an update
of all generator settings available in this dialog box. Useful when you change the level
or frequency on the generator itself. In that case, those settings remain the same in the
R&S VSE-K18. To restore the original settings defined within the R&S VSE-K18, use
that button to restore the generator settings.
Remote command:
CONFigure:GENerator:SETTings:UPDate on page 290
Querying generator settings
Similarly, you can transfer the current generator configuration into the amplifier application with the "Query All Settings From Generator" button.
Note that the center frequency is not updated when you attach the generator frequency
to that of the R&S VSE.
Remote command:
CONFigure:SETTings on page 290
IP Address.....................................................................................................................64
Opens a dialog box to configure the network properties of the signal generator.
You can connect to the generator either by entering its IP address ("123" button), or its
computer name ("ABC" button).
If you are not sure about the IP address or computer name of your generator, check its
user interface or kindly ask your IT administrator to provide them.
After you have entered IP address or computer name, use "Connect" to establish the
connection. The R&S VSE shows if the connection state, and, if the connection was
successful, the connected generator type.
Remote command:
CONFigure:GENerator:CONNection:CSTate? on page 286
RMS Level
Defines the RMS level of the signal that is generated.
When you define the RMS level here, the signal generator is automatically configured
to that level.
In addition, you can define a level offset (for example to take external attenuation into
account). Note that the level offset is a purely mathematical value and does not change
the actual level of the signal at the RF output.
The level offset takes level offsets into account that occur before the signal has passed
through the DUT (usually an amplifier). For level offsets occurring after the DUT, define
a level offset in the "Amplitude" menu of the signal analyzer.
You can also define a Digital Attenuation that you can use for fast output level
changes.
NOTICE! Risk of damage to the DUT.
RMS levels that are too high can damage or destroy the DUT.
Make sure to keep an eye on the RMS level, especially when defining a level offset. A
level offset changes the displayed value of the RMS level, but not the real RMS level.
Displayed RMS level = real RMS level + level offset
Thus, the actual RMS level can be higher than the displayed level.
Note: Always change the generator level from within the R&S VSE-K18 user interface
and thus synchronize the levels of both instruments.
If you change the generator level on the signal generator, the R&S VSE-K18 does not
synchronize the levels and measurement results are going to be invalid.
CONFigure:GENerator:POWer:LEVel:OFFSet:LEDState? on page 288
Maximum DUT Input Level
Defines the maximum level that the generated signal can have. Selecting a higher level
is not possible.
Defining a maximum output level is useful if you are measuring sensitive DUTs.
Remote command:
CONFigure:GENerator:DUT:INPut:MAXimum:POWer on page 283
CONFigure:GENerator:DUT:INPut:MAXimum:POWer:LEDState? on page 284
Attach to Analyzer Frequency
Turns synchronization of the analyzer and generator frequency on and off.
When you turn on this feature, changing the frequency on the analyzer automatically
adjusts the frequency on the generator.
Remote command:
CONFigure:GENerator:FREQuency:CENTer:SYNC[:STATe] on page 285
Center Frequency
Defines the frequency of the signal that the generator transmits.
When you turn on Attach to Analyzer Frequency, any changes you make to the gener-
ator frequency are also adjusted on the analyzer.
Remote command:
CONFigure:GENerator:FREQuency:CENTer on page 285
CONFigure:GENerator:FREQuency:CENTer:LEDState? on page 285
Reference Frequency
Selects the source of the generator reference frequency.
The internal reference is that of the signal generator itself. When you select an external
reference, you can use another frequency reference, for example that of the R&S VSE.
Remote command:
CONFigure:GENerator:EXTernal:ROSCillator on page 284
CONFigure:GENerator:EXTernal:ROSCillator:LEDState? on page 284
Path RF / BB
Selects the RF signal path of the generator that is used for signal generation.
Remote command:
If you are using a waveform file that contains several different waveforms, you have to
select the segment to transfer to the signal generator.
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Note that the segment that you have selected in the "Generator Setup" has to match
the segment selected for the reference signal, regarding the signal characteristics.
Remote command:
CONFigure:GENerator:SEGMent on page 289
CONFigure:GENerator:SEGMent:LEDState? on page 289
Digital Attenuation
Attenuates or amplifies the internal, digitally modulated I/Q signal on the signal generator. The level of the RF signal is thus adjusted accordingly.
Digital attenuation allows very fast level changes of the internal I/Q signals.
Note that digital attenuation only has an effect on the RF output level if the internal I/Q
modulator of the generator is active.
Remote command:
CONFigure:GENerator:POWer:LEVel:ATTenuation on page 286
RF Output
Turns the RF output on the connected signal generator on and off.
When you turn off the RF output, the generator does not feed a signal into the connec-
ted DUT.
Remote command:
CONFigure:GENerator:RFOutput[:STATe] on page 288
CONFigure:GENerator:RFOutput:LEDState? on page 288
Settling Delay
The "Settling Delay" defines a time period between the time a parameter changes on
the generator and the start of the next measurement. The R&S VSE automatically
waits for the defined time period whenever one of the relevant generator settings has
been changed.
Defining a delay time is especially useful for measurements that automatically change
generator settings (for example the parameter sweep). The delay time considers the
settling time of the generator's hardware components between individual measurements.
Remote command:
CONFigure:DUT:STIMe on page 283
3.3.7Reference: I/Q file input
●Basics on input from I/Q data files.......................................................................... 66
●I/Q data file format (iq-tar).......................................................................................67
3.3.7.1Basics on input from I/Q data files
The I/Q data to be evaluated in a particular R&S VSE application cannot only be captured by the application itself, it can also be loaded from a file, provided it has the correct format. The file is then used as the input source for the application.
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For example, you can capture I/Q data using the I/Q Analyzer application, store it to a
file, and then analyze the signal parameters for that data later using the Pulse application (if available).
An application note on converting Rohde & Schwarz I/Q data files is available from the
Rohde & Schwarz website:
1EF85: Converting R&S I/Q data files
When importing data from an I/Q data file using the import functions provided by some
R&S VSE applications, the data is only stored temporarily in the capture buffer. It overwrites the current measurement data and is in turn overwritten by a new measurement.
If you use an I/Q data file as input, the stored I/Q data remains available for any number of subsequent measurements. Furthermore, the (temporary) data import requires
the current measurement settings in the current application to match the settings that
were applied when the measurement results were stored (possibly in a different application). When the data is used as an input source, however, the data acquisition settings in the current application (attenuation, center frequency, measurement bandwidth, sample rate) can be ignored. As a result, these settings cannot be changed in
the current application. Only the measurement time can be decreased, to perform
measurements on an extract of the available data (from the beginning of the file) only.
For input files that contain multiple data streams from different channels, you can
define which data stream to be used for the currently selected channel in the input settings.
You can define whether the data stream is used only once, or repeatedly, to create a
larger amount of input data.
When using input from an I/Q data file, the [RUN SINGLE] function starts a single measurement (i.e. analysis) of the stored I/Q data, while the [RUN CONT] function repeatedly analyzes the same data from the file.
Pre-trigger and post-trigger samples
In applications that use pre-triggers or post-triggers, if no pre-trigger or post-trigger
samples are specified in the I/Q data file, or too few trigger samples are provided to
satisfy the requirements of the application, the missing pre- or post-trigger values are
filled up with zeros. Superfluous samples in the file are dropped, if necessary. For pretrigger samples, values are filled up or omitted at the beginning of the capture buffer.
For post-trigger samples, values are filled up or omitted at the end of the capture buffer.
3.3.7.2I/Q data file format (iq-tar)
I/Q data is packed in a file with the extension .iq.tar. An iq-tar file contains I/Q
data in binary format together with meta information that describes the nature and the
source of data, e.g. the sample rate. The objective of the iq-tar file format is to separate I/Q data from the meta information while still having both inside one file. In addition, the file format allows you to include user-specific data and to preview the I/Q data
in a web browser (not supported by all web browsers).
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The iq-tar container packs several files into a single .tar archive file. Files in .tar
format can be unpacked using standard archive tools (see http://en.wikipedia.org/wiki/
Comparison_of_file_archivers) available for most operating systems. The advantage
of .tar files is that the archived files inside the .tar file are not changed (not compressed) and thus it is possible to read the I/Q data directly within the archive without
the need to unpack (untar) the .tar file first.
Sample iq-tar files
Some sample iq-tar files are provided in the
C:\ProgramData\Rohde-Schwarz\VSE\<version_no>\user/Demo/ directory
on the R&S VSE.
These files are also available in the demo mode of the R&S VSE software.
An application note on converting Rohde & Schwarz I/Q data files is available from the
Rohde & Schwarz website:
1EF85: Converting R&S I/Q data files
Contained files
An iq-tar file must contain the following files:
●
I/Q parameter XML file, e.g. xyz.xml
Contains meta information about the I/Q data (e.g. sample rate). The filename can
be defined freely, but there must be only one single I/Q parameter XML file inside
an iq-tar file.
●
I/Q data binary file, e.g. xyz.complex.float32
Contains the binary I/Q data of all channels. There must be only one single I/Q
data binary file inside an iq-tar file.
Optionally, an iq-tar file can contain the following file:
●
I/Q preview XSLT file, e.g. open_IqTar_xml_file_in_web_browser.xslt
Contains a stylesheet to display the I/Q parameter XML file and a preview of the
I/Q data in a web browser (not supported by all web browsers).
A sample stylesheet is available at http://www.rohde-schwarz.com/file/
open_IqTar_xml_file_in_web_browser.xslt.
●I/Q parameter XML file specification....................................................................... 69
●I/Q data binary file...................................................................................................78
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I/Q parameter XML file specification
The content of the I/Q parameter XML file must comply with the XML schema
RsIqTar.xsd available at: http://www.rohde-schwarz.com/file/RsIqTar.xsd.
In particular, the order of the XML elements must be respected, i.e. iq-tar uses an
"ordered XML schema". For your own implementation of the iq-tar file format make
sure to validate your XML file against the given schema.
The following example shows an I/Q parameter XML file. The XML elements and attributes are explained in the following sections.
The following data elements are the minimum required for a valid iq-tar file. They
are always provided by an iq-tar file export from a Rohde & Schwarz product. If not
specified otherwise, it must be available in all iq-tar files used to import data to a
Rohde & Schwarz product.
ElementPossible ValuesDescription
<RS_IQ_TAR_FileFormat>
<Name>
<Comment>
-The root element of the XML file. It must contain the attribute
fileFormatVersion that contains the number of the file format
definition.
stringOptional: describes the device or application that created the file.
stringOptional: contains text that further describes the contents of the
file.
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<DateTime>
<Samples>
<Clock>
<Format>
<DataType>
yyyy-mm-ddThh:mm:ssContains the date and time of the creation of the file. Its type is
xs:dateTime (see RsIqTar.xsd).
integerContains the number of samples of the I/Q data. For multi-chan-
nel signals all channels have the same number of samples. One
sample can be:
●
A complex number represented as a pair of I and Q values
●
A complex number represented as a pair of magnitude and
phase values
●
A real number represented as a single real value
See also <Format> element.
doubleContains the clock frequency in Hz, i.e. the sample rate of the I/Q
data. A signal generator typically outputs the I/Q data at a rate
that equals the clock frequency. If the I/Q data was captured with
a signal analyzer, the signal analyzer used the clock frequency as
the sample rate. The attribute unit must be set to "Hz".
complex | real | polar
int8 | int16 | int32 | float32 |
float64
Specifies how the binary data is saved in the I/Q data binary file
(see <DataFilename> element). Every sample must be in the
same format. The format can be one of the following:
●
complex: Complex number in cartesian format, i.e. I and Q
values interleaved. I and Q are unitless
●
real: Real number (unitless)
●
polar: Complex number in polar format, i.e. magnitude
(unitless) and phase (rad) values interleaved. Requires
DataType = float32 or float64
Specifies the binary format used for samples in the I/Q data
binary file (see <DataFilename> element and "I/Q data binary
file"on page 78). The following data types are allowed:
●
int8: 8 bit signed integer data
●
int16: 16 bit signed integer data
●
int32: 32 bit signed integer data
●
float32: 32 bit floating point data (IEEE 754)
●
float64: 64 bit floating point data (IEEE 754)
<ScalingFactor>
<NumberOfChannels>
doubleOptional: describes how the binary data can be transformed into
values in the unit Volt. The binary I/Q data itself has no unit. To
get an I/Q sample in the unit Volt the saved samples have to be
multiplied by the value of the <ScalingFactor>. For polar data
only the magnitude value has to be multiplied. For multi-channel
signals the <ScalingFactor> must be applied to all channels.
The attribute unit must be set to "V".
The <ScalingFactor> must be > 0. If the <ScalingFactor>
element is not defined, a value of 1 V is assumed.
integerOptional: specifies the number of channels, e.g. of a MIMO sig-
nal, contained in the I/Q data binary file. For multi-channels, the
I/Q samples of the channels are expected to be interleaved within
the I/Q data file (see "I/Q data binary file"on page 78). If the
<NumberOfChannels> element is not defined, one channel is
assumed.
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<DataFilename>
<UserData>
<PreviewData>
xmlOptional: contains user, application or device-specific XML data
xmlOptional: contains further XML elements that provide a preview of
Contains the filename of the I/Q data binary file that is part of the
iq-tar file.
It is recommended that the filename uses the following convention:
<xyz>.<Format>.<Channels>ch.<Type>
●
<xyz> = a valid Windows file name
●
<Format> = complex, polar or real (see Format element)
●
<Channels> = Number of channels (see
NumberOfChannels element)
●
<Type> = float32, float64, int8, int16, int32 or int64 (see
DataType element)
Examples:
●
xyz.complex.1ch.float32
●
xyz.polar.1ch.float64
●
xyz.real.1ch.int16
●
xyz.complex.16ch.int8
which is not part of the iq-tar specification. This element can
be used to store additional information, e.g. the hardware configuration. User data must be valid XML content.
the I/Q data. The preview data is determined by the routine that
saves an iq-tar file (e.g. R&S VSE). For the definition of this
element refer to the RsIqTar.xsd schema. Note that the preview can be only displayed by current web browsers that have
JavaScript enabled and if the XSLT stylesheet
open_IqTar_xml_file_in_web_browser.xslt is available.
User-defined data elements
You can insert additional user, application or device-specific XML data that is not part
of the iq-tar specification in the <UserData> element. User data must be valid XML
content.
Rohde & Schwarz products use this element to import and export application-specific
data. While some elements are mandatory in order to import the iq-tar file to the product, others are optional.
The subelements within the <UserData> element provided by the Rohde & Schwarz
products are <DataImportExport_MandatoryData> and
<DataImportExport_OptionalData>. To import an iq-tar file to the R&SVSE
software, either both of these elements or none of them must be provided.
Mandatory data elements
The following information is always provided by an iq-tar file export from
Rohde & Schwarz products. It is contained in the
<DataImportExport_MandatoryData> element. It must be available in all iq-tar
files used to import data to the R&S VSE software if optional data is included (see
"Optional data elements"on page 72).
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Table 3-2: Subelements of <DataImportExport_MandatoryData>
Element NamePossible ValuesDescription
<ChannelNames><ChannelName>
<ChannelName>
<CenterFrequency>
StringChannel name in R&S VSE software
DoubleCenter frequency of captured I/Q data
Mapping of channels in iq-tar file to
channel names in R&S VSE software.
CH_1 = first <ChannelName>
CH_2 = second <ChannelName>
...
CH_n = last <ChannelName>
Optional data elements
Optionally, the following information can be provided in iq-tar files used to import
data to Rohde & Schwarz products. This information can also be provided by an
iq-tar file export from the R&S VSE software, if selected. Note that the available
information during data export depends on the connected instrument.
Optional information is contained in the <DataImportExport_OptionalData> element. If this element is included in the <UserData> element, the
<DataImportExport_MandatoryData> element must also be included (see "Man-
datory data elements"on page 71).
Optional data is included in <Key> subelements with a specific name attribute. Keys for
an individual channel are provided together, i.e. first all keys for CH_1, then all keys for
CH_2 etc. The channel index is provided as a prefix for the key name attribute and corresponds to the mapping defined in the <ChannelNames> in
<DataImportExport_MandatoryData> (see "Mandatory data elements"
on page 71).
Table 3-3: Possible information in <DataImportExport_OptionalData>
<Key> element name attributePossible Values
Ch<n>_RefLevel[dBm]Double
Ch<n>_RefLevelOffset[dB]Double
Ch<n>_AttenuMech[dB]Integer
Ch<n>_AttenuElecStateON | OFF
Ch<n>_AttenuElecValue[dB]Integer
Ch<n>_PreampStateON | OFF
Ch<n>_PreampGain[dB]Integer
Ch<n>_PreSelectorStateON | OFF
(R&S FSWT only)
Ch<n>_PreSelectorTypeNARROW | WIDE
(R&S FSWT only)
Ch<n>_Impedance[Ohm]50 | 75
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<Key> element name attributePossible Values
Ch<n>_InputCouplingAC | DC
Ch<n>_DeviceIdString
Ch<n>_DeviceOptionsString
Ch<n>_DeviceHwInfoString
Ch<n>_DeviceVersionsString
Ch<n>_CalibrationStateON | OFF
Ch<n>_RefOscillatorInputOFF | ON
Ch<n>_RefOscillatorFreq[Hz]Double
Ch<n>_InputPathRF
Ch<n>_InputSelectionINPUT1 | INPUT2
(R&S FSWT only)
Ch<n>_HighPassFilterStateON | OFF
Ch<n>_YigPreSelectorStateON | OFF
Ch<n>_ExtMixerStateON | OFF
Ch<n>_MeasBandwidth[Hz]Double
Ch<n>_FilterSettingsFLAT | GAUSS | OFF
Ch<n>_TrgSourceExtern <1 ..4> | I/Q Power | IF Power | RF Power |
Power Sensor | Time
Ch<n>_TrgLevel[dB]Double
Ch<n>_TrgHysteresis[dB]Double
Ch<n>_TrgTpis[s]Double
Ch<n>_TrgOffset[s]Double
Ch<n>_TrgSlopeRising | Falling | Rising/Falling
Ch<n>_TrgHoldoff[s]Double
Ch<n>_TrgDropOut[s]Double
Ch<n>_NumberOfPostSamplesInteger
Ch<n>_NumberOfPreSamplesInteger
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Example: Example for <DataImportExport_OptionalData>
The following example demonstrates the XML description inside the iq-tar file. Note
that this preview is not supported by all web browsers.
Open the xml file in a web browser, e.g. Microsoft Internet Explorer. If the stylesheet
open_IqTar_xml_file_in_web_browser.xslt is in the same directory, the web
browser displays the xml file in a readable format.
Data stored as int16 and a desired full scale voltage of 1 V
ScalingFactor = 1 V / maximum int16 value = 1 V / 215 = 3.0517578125e-5 V
Scaling FactorNumerical valueNumerical value x ScalingFac-
tor
Minimum (negative) int16 value
Maximum (positive) int16 value
- 215 = - 32768
215-1= 32767
-1 V
0.999969482421875 V
I/Q data binary file
The I/Q data is saved in binary format according to the format and data type specified
in the XML file (see <Format> element and <DataType> element). To allow reading
and writing of streamed I/Q data, all data is interleaved, i.e. complex values are interleaved pairs of I and Q values and multi-channel signals contain interleaved (complex)
samples for channel 0, channel 1, channel 2 etc. If the <NumberOfChannels> element is not defined, one channel is presumed.
Example: Element order for real data (1 channel)
I[0], // Real sample 0
I[1], // Real sample 1
I[2], // Real sample 2
...
Example: Element order for complex cartesian data (1 channel)
I[0], Q[0], // Real and imaginary part of complex sample 0
I[1], Q[1], // Real and imaginary part of complex sample 1
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I[2], Q[2], // Real and imaginary part of complex sample 2
...
Example: Element order for complex polar data (1 channel)
Mag[0], Phi[0], // Magnitude and phase part of complex sample 0
Mag[1], Phi[1], // Magnitude and phase part of complex sample 1
Mag[2], Phi[2], // Magnitude and phase part of complex sample 2
...
Example: Element order for complex cartesian data (3 channels)
The R&S VSE-K18 provides functionality to trigger measurements.
The "Trigger" dialog box contains settings to configure triggered measurements.
The following trigger sources are supported:
●
Free Run
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Configuration
Configuring the data capture
●
External
●
I/Q Power
●
IF Power
●
RF Power
●
Time
If the time trigger is used, the R&S VSE automatically sets the repetition interval to
match the length of the reference file. "Auto Time Trigger" sets the trigger offset to
the current trigger to sync (TTS) value.
The trigger settings are similar to those in the spectrum application. For a comprehensive description of the trigger functionality, refer to the R&S VSE user manual.
Access: "Overview" > "Data Acquisition"
The "Data Acquisition" dialog box contains settings to configure the process of how the
application records the signal.
The remote commands required to configure the data capture are described in Chap-
ter 5.5.7, "Configuring the data capture", on page 291.
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Configuring the measurement bandwidth..................................................................... 82
Inverting the I/Q branches.............................................................................................84
Defining the resolution bandwidth for spectrum measurements................................... 84
Configuring the measurement bandwidth
The sample rate defined for data acquisition is the sample rate with which the analyzer
samples the amplified signal.
The measurement bandwidth defines the flat, usable bandwidth of the final I/Q data.
The application allows you to adjust both values automatically or manually.
Automatic adjustment ← Configuring the measurement bandwidth
When you select automatic adjustment of sample rate and measurement bandwidth,
the application selects a bandwidth that is appropriate for the characteristics of the reference signal and adjusts the sample rate accordingly.
For more information about the reference signal, see Chapter 3.2, "Designing a refer-
Manual definition ← Configuring the measurement bandwidth
When you define the sample rate and measurement bandwidth manually, you can
select values that you are comfortable with. Because the bandwidth is a function of the
sample rate (and vice versa), the application adjusts the values when you change
either setting.
The following dependencies apply:
●
When you change the sample rate, the application updates the bandwidth accordingly (and vice versa). It also adjusts the capture length to the new values. The
capture time remains the same.
●
When you change the capture time or capture length, the sample rate and bandwidth remain the same.
Maximum bandwidth ← Configuring the measurement bandwidth
The maximum bandwidth you can use depends on your hardware configuration.
For an overview of available bandwidth extensions, refer to the datasheet.
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By default, the application automatically determines the maximum bandwidth. When
you select a maximum bandwidth other than "Auto", the bandwidth is restricted to that
value. When you select the maximum bandwidth manually, make sure that this bandwidth is suited for the signal you are testing. Otherwise, the signal can be distorted and
results are no longer valid.
If you have no bandwidth extension this setting is not available.
For more information about the maximum bandwidth, refer to the user manual of the
R&S VSE I/Q Analyzer.
Remote command:
TRACe:IQ:WBANd[:STATe] on page 295
TRACe:IQ:WBANd:MBWidth on page 295
Configuring the measurement time
The measurement time (or capture time) defines the duration of a measurement in
which the required number of samples is collected.
The capture length is the number of samples that are captured during the selected
measurement time. The capture length is a function of the sample rate and the capture
time.
Automatic adjustment ← Configuring the measurement time
When you select automatic adjustment of capture time, the application selects a capture time that is appropriate for the characteristics of the reference signal.
As orientation, the application shows the length of the reference signal in the corresponding field in the dialog box (➙ "Ref Signal Duration").
For more information about the reference signal, see Chapter 3.2, "Designing a refer-
Manual definition ← Configuring the measurement time
When you define the capture length and time manually, you can select values that you
are comfortable with.
However, make sure to define a capture time that is greater than the length of the reference signal - otherwise the application is not able to analyze the signal correctly.
The following dependencies apply:
●
When you change the capture time, the application updates the capture length
accordingly (and vice versa). Sample rate and bandwidth remain the same.
●
When you change the sample rate or bandwidth, the application updates the cap-
ture length accordingly. The capture time remains the same.
Note that the maximum capture time depends on the current measurement bandwidth.
Remote command:
The application allows you to swap the I and Q branches of the signal.
Swapping the branches is useful, for example, when the DUT inverts the real (I) and
imaginary (Q) parts of the signal and transfers the signal that way.
Note that the sideband is also inverted when you turn on this feature.
Remote command:
[SENSe:]SWAPiq on page 292
Defining the resolution bandwidth for spectrum measurements
The resolution bandwidth (RBW) defines the bandwidth of the resolution filter applied
to spectrum measurements (like the "Spectrum FFT" result).
The "RBW Mode" selects whether the application automatically selects a suitable resolution bandwidth based on the signal you are measuring, or if you define the resolution
bandwidth manually. When you select manual definition of the RBW (for example when
you want to do a measurement according to a certain telecommunications standard),
you can enter the bandwidth in the "RBW" field.
The amplifier measurement application supports any bandwidth between 1 Hz and
10 MHz.
Remote command:
[SENSe:]BANDwidth[:RESolution]:AUTO on page 292
[SENSe:]BANDwidth[:RESolution] on page 292
3.6Sweep configuration
Access: "Overview" > "Data Acquisition" > "Sweep"
The "Sweep" dialog box contains settings to configure the characteristics of a single
data recording (a sweep).
The remote commands required to configure the sweep are described in Chap-
Select Result Rng......................................................................................................... 85
Statistics State
Turns the sweep statistics calculation on and off.
Remote command:
[SENSe:]SWEep:STATistics[:STATe] on page 297
Statistics Mode
Sets the statistics mode.
If I/Q averaging is selected, the IQ data is averaged over several data captures after
synchronization to the reference file. This leads to a significant noise reduction. Be
aware that I/Q averaging is only possible for synchronized parts of the captured signal,
because it only makes sense if the same samples in the I/Q data stream are averaged.
Therefore, make sure that the measurement is synchronized. Otherwise, the results
would be invalid.
If trace statistics is selected, multiple frames are measured to create a graphical or
scalar statistics result.
Remote command:
[SENSe:]SWEep:STATistics:MODE on page 298
Continuous Statistics
If continuous statistics is enabled, it does not reset the results when the average count
is through. Instead, it continues to average the data. The continuous statistics setting
only has an effect in continuous sweep mode.
If continuous statistics is turned off, averaging starts again from "0" after the defined
statistics count is reached.
Remote command:
[SENSe:]SWEep:STATistics:CONTinuous[:STATe] on page 297
Statistics Count
Defines the number of single data captures the application uses to average the data.
Remote command:
[SENSe:]SWEep:STATistics:COUNt on page 297
Select Result Rng
Sets the result range.
Remote command:
CONFigure:RESult:RANGe[:SELected] on page 298
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3.7Synchronizing measurement data
Configuration
Synchronizing measurement data
Access: "Overview" > "Sync / Error Est / Comp" > "Sync and Eval Range" > "Synchronization"
The application allows you to synchronize the measured signal with the reference signal and provides various features to control synchronization.
Synchronization consists of signal estimation and compensation. After the application
has detected the position of the reference signal in the capture buffer, it estimates possible errors in the measured signal (for example the sample error rate or the amplitude
droop) by comparing it to the reference signal. The estimated errors can optionally be
compensated for.
The remote commands required to configure signal synchronization are described in
Chapter 5.5.9, "Synchronizing measurement data", on page 298.
Turning synchronization of reference and measured signal on and off.........................86
Selecting the synchronization method.......................................................................... 87
Defining a synchronization confidence level................................................................. 87
Defining the estimation range....................................................................................... 88
Turning synchronization of reference and measured signal on and off
During measurements, the application tries to synchronize the measured signal with
the reference signal. When no significant correlation between the measured and reference signal can be found, synchronization fails.
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Configuration
Synchronizing measurement data
However, you can turn off synchronization if you would like to run unsynchronized
measurements. Note however, that the calculation of some results in the result summary requires synchronization. These results cannot be calculated when you turn off
synchronization.
When you turn off synchronization, the results are always calculated over the complete
capture buffer. When synchronization is on, the results are always calculated over the
synchronized data range of the capture buffer. Therefore, the result values can be different for unsynchronized measurements, even if you measure the same signal (the
result is still valid and correct, though).
Failed synchronization
When you turn on "Stop on Sync Failed", the application automatically aborts the measurement, in case synchronization fails.
Remote command:
CONFigure:SYNC:STAT on page 301
CONFigure:SYNC:SOFail on page 300
Selecting the synchronization method
The application allows you to select the method with which the application synchronizes the signals with the "Synchronization Mode" parameter. The following methods are
available.
●
I/Q Direct
The I/Q data for the reference signal is directly correlated with the reference and
measured signal. The performance of this method degrades in the presence of a
frequency offset between the measured and reference signals.
●
I/Q Phase Difference
Correlation on the phase differentiated I/Q data. This method retains phase change
information and can handle a frequency offset , but is more sensitive to noise than
the "I/Q Direct" method.
●
I/Q Magnitude
Correlation on the magnitude of the I/Q data with no regard for phase information.
This method can handle a frequency offset and is less sensitive to noise that the
"I/Q Phase Difference" method, but is only useful with amplitude modulated sig-
nals.
●
Trigger
It is assumed that the capture is triggered at the start of the reference waveform.
Only minimal correlation is performed to account for trigger jitter. This method is the
fastest synchronization method.
Remote command:
CONFigure:SYNC:DOMain on page 300
Defining a synchronization confidence level
The synchronization confidence level ("Sync Confidence") is a percentage that
describes how similar (or correlated) reference and measured signal need to be in
order for synchronization to be successful.
A value of 0 % means that synchronization is always successful even if the signals are
not correlated at all. However, results that rely on a good synchronization (like the
EVM) do contain reasonable values in that case. A value of 100 % means that the signals are identical (in that they are linearly dependent).
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Configuration
Evaluating measurement data
The cross-correlation is calculated over all samples in the capture buffer (or the estimation range, if you have defined one).
When the cross-correlation coefficient falls below the confidence level you have
defined, synchronization is no longer successful.
Remote command:
CONFigure:SYNC:CONFidence on page 300
Defining the estimation range
The estimation range has several effects on the synchronization process.
●
It defines which part of the reference signal is used for cross-correlation within the
capture buffer in order to align the reference and measured signals.
●
It defines which part of the reference signal is used for error estimation.
By default, the application estimates over the complete reference signal. However, you
can also estimate over a given range in the capture buffer only. In that case, turn off
the "Use Full Ref Signal" feature. When you are not using the full reference signal, the
"Eval Start" and "Eval Stop" fields become available. The allowed values are offsets
relative to the beginning of the capture buffer (0 s). The highest offset possible
depends on the size of the capture buffer.
Defining an estimation range is useful in the following cases.
●
If you want to limit the estimation to a specific part of the signal, for example if the
signal contains a preamble or midamble.
●
If you want to limit the estimation to the ON part of a TDD signal.
●
If you want to increase the measurement speed for relatively long signals, for
example an LTE signal.
On the downside, limiting the estimation range leads to a higher empirical variance of
the results.
In the preview pane displayed in the dialog box, the currently defined estimation range
is represented by two red vertical lines.
Tip: You can also use the touchscreen to move the lines to a new position in the pre-
view pane. However, this way is not as accurate as entering a number into the input
field.
Remote command:
CONFigure:ESTimation:FULL on page 298
CONFigure:ESTimation:STARt on page 299
CONFigure:ESTimation:STOP on page 299
3.8Evaluating measurement data
Access: "Overview" > "Sync / Error Est / Comp" > "Sync and Eval Range" > "Eval
Range"
The application allows you to define the time frame in the reference signal used to
evaluate and calculate the measurement results.
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Configuration
Evaluating measurement data
The remote commands required to configure signal evaluation are described in Chap-
ter 5.5.10, "Defining the evaluation range", on page 301.
Defining the evaluation range....................................................................................... 89
Defining the evaluation range
The evaluation range defines the data range in the capture buffer over which the application calculates the measurement results.
By default, the application calculates the results over the complete capture buffer. If
synchronization has been successful, the application calculates the results over the
capture buffer range in which the reference signal has been found. If you have turned
off synchronization or if it has not been successful, the complete capture buffer is used
to calculate the remaining results.
Example:
The capture buffer is 30 ms long, the reference signal starts at 9 ms and is 10 ms long.
When synchronization is successful, the evaluation range starts at 9 ms and ends at
19 ms. If synchronization has been turned off, the evaluation range is the full capture
buffer.
However, you can also select a particular data range within the reference signal. In that
case, turn off the "Use Full Ref Signal" feature. When it is off, the "Eval Start" and "Eval
Stop" fields become available. The allowed values are offsets relative to the beginning
of the reference signal (0 s). The highest offset possible depends on the length of the
reference signal.
Example:
The situation is as described above (30 ms capture buffer, 10 ms reference signal).
Let's say you want to evaluate milliseconds 2 to 6 of the reference signal. In that case,
you would have to define a start offset of 11 ms (the reference signal starts at 9 ms,
plus the first 2 ms you are not interested in = 11 ms) and a stop offset of 15 ms (9 ms +
6 ms).
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3.9Estimating and compensating signal errors
Configuration
Estimating and compensating signal errors
In the preview pane displayed in the dialog box, the currently defined evaluation range
is represented by two blue vertical lines.
Tip: You can also use the touchscreen to move the lines to a new position in the preview pane. However, this way is not as accurate as entering a number into the input
field.
Remote command:
CONFigure:EVALuation:FULL on page 301
CONFigure:EVALuation:STARt on page 302
CONFigure:EVALuation:STOP on page 303
Access: "Overview" > "Sync / Error Est / Comp" > "Error Est / Compensation"
The application allows you to estimate possible undesired effects in the signal, and, if
there are any, also compensate these effects.
The remote commands required to configure error compensation and equalization are
described in Chapter 5.5.11, "Estimating and compensating signal errors",
on page 303.
Estimation and compensation
When you turn on error estimation only, the results are not compensated for the corresponding errors.
When you turn on error compensation, the displayed results are also corrected by the
estimated errors. Note that in that case, the signal might look better than it actually is.
Compensation without estimation is not possible.
Generally, it is recommended to switch off the estimation of a certain parameter if it is
not existent. E.g., if generator and analyzer are frequency locked, it is recommended to
switch off the frequency error estimation. Furthermore sample rate error estimation can
be switched off if the frequency locked generator is a vector signal generator, i.e.
includes the DAC.
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3.10Equalizer
Configuration
Equalizer
You can estimate and compensate the following effects:
●
I/Q Imbalance: combined effect of amplitude and phase error.
●
I/Q Offset: shift of the constellation points in a particular direction.
●
Frequency Error: difference between measured and reference center frequency.
●
Amplitude Droop: decrease of the signal power over time in the transmitter.
●
Sample Error Rate: difference between the sample rate of the reference signal
and the measured signal.
In addition, the amplifier application provides equalizer functionality. The equalizer corrects distortions in the frequency characteristics during the transmission of the signal. It
can thus help to faithfully reproduce the input signal at the amplifier output.
Using the equalizer
Using the equalizer requires a description of the equalizer filter. You can either train
(and save) such a filter automatically with the R&S VSE, or use one that you already
have.
Training (or creating) the equalizer filter is a process in which the R&S VSE compares
the frequency response of the input and output signal and equalizes potential distortion. The goal is to match the frequency response of the output signal and the input
signal. The R&S VSE is able to train the filter based on all samples in the evaluation
range.
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Configuration
Applying system models
The "Equalizer Filter Length For Training" property defines the number of FIR filter
coefficients to be calculated. A larger number of samples generally yields better
results, but takes longer to calculate. After you have defined the filter length (coefficients), you can start the training sequence with the "Train Equalizer Filter on Current
I/Q Data" feature. To apply the filter, turn on the equalizer with the "Equalizer State"
toggle.
Note that the reference and measured signal need to be synchronized for a successful
filter training. Make sure to turn on signal synchronization before you train a filter.
When the filter training is done, you can save the filter in a csv or a fres file (➙ "Save
Equalizer").
For more information about the fres file format, refer to the R&S VSE user manual.
If you want to use an equalizer filter that you already have from a previous measure-
ment, you can restore that filter (➙ "Load Equalizer Filter") and apply it without a training sequence.
The dialog box also shows the information about the filter file that is currently in use.
This information includes the file name, the date it was modified last and the length of
the filter (in samples).
Note: Any equalizer filter is only valid for the sample rate it has been trained for.
If you change the sample rate when an equalizer filter is active, the R&S VSE automatically turns off the equalizer filter. If you still want to use an equalizer filter with the new
sample rate, you have to train and apply the equalizer filter again.
Note: An I/Q data export always exports the unequalized (raw) data.
If you want to export the equalized data, you can do so with the following SCPI command.
A polynomial model describes the characteristics of the DUT based on the input signal
and the output signal of the amplifier.
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Configuration
Applying system models
The remote commands required to configure system models are described in Chap-
ter 5.5.12, "Applying a system model", on page 308.
Turning system modeling on and off.............................................................................93
Selecting the degree of the polynomial.........................................................................94
Defining the modeling range......................................................................................... 94
Selecting the modeling scale........................................................................................ 95
Turning system modeling on and off
You can use the system modeling functionality to calculate a mathematical model that
describes the properties of the DUT.
Using a model is useful to observe and estimate the behavior of the amplifier and, if
necessary, adjust the DUT behavior. The application supports memory-free polynomial
models to the 18th degree.
The following diagrams contain traces that show the model. These traces are calculated by using the model function on the reference signal.
●
"AM/AM"
●
"AM/PM"
Note that the model traces are also the basis for the DPD functionality available in the
R&S VSE-K18.
When the characteristics of the modeled signal match those of the measured signal,
the model describes the DUT behavior well. If not, you can try to get a better result by
adjusting the model properties.
When you turn on modeling, the application shows an additional trace in the graphical
result displays. This trace corresponds to the signal characteristics after the model has
been applied to the reference signal.
Selecting the modeling sequence
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Configuration
Applying system models
The modeling sequence selects the sequence in which the models are calculated. The
application then either calculates the "AM/AM" model before calculating the "AM/PM"
model (default), or vice versa.
Remote command:
CONFigure:MODeling[:STATe] on page 310
CONFigure:MODeling:SEQuence on page 310
Selecting the degree of the polynomial
In addition to the type of curve, you can also select the order of the polynomial model.
The order of the model defines the degree, complexity and number of terms in the pol-
ynomial model. In general, a polynomial of the Nth degree looks like this:
y = a0 + a1x + a2x2 + … + aNx
N
The degree of the model is defined by N (as an index or exponent). The higher the
order, the more complex the calculation and the longer it takes to calculate the model.
Higher models do not necessarily lead to better fitting model curves.
Note that the nonlinear effects consume an additional bandwidth proportional to 2
times the number of odd factors in the polynomial, excluding the linear one.
Example:
If the signal bandwidth is 1 MHz and the highest degree is 5, the bandwidth of the
resulting signal is increased by 2 times 2 (because there are the variables a3 and a5)
times 1 MHz which are 4 MHz. This leads to a total signal bandwidth of 5 MHz (1 MHz
+ 4 MHz). The configured recording bandwidth must be at least 5 MHz to record all
nonlinear effects generated by the DUT.
Tip: To select a specific subset of polynomial degrees you want to apply, you can
either:
●
Define a range of degrees (e.g. "0 - 5", in that case the application applies all
degrees in that range).
●
Define a set of individual degrees only (e.g. "1;3;5;7", in that case the application
applies those degrees only). Note that the "." key on the front panel draws the ";"
character.
●
Define a combination of the methods mentioned above (e.g. "1;3;5-7")
The modeling range defines the part of the signal that the model is applied to.
When you limit the level range that the model is applied to, only samples with levels
between peak level and "peak level minus modeling level range value" are used during
the model calculation. Note that the modeling range is also the range the DPD is
applied to.
You can also define a smaller or larger modeling level range. Make sure, however, that
the range is large enough not to distort the model.
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Configuration
Applying digital predistortion
In addition, you can define the number of points on the curve that the application uses
to calculate the model. The selected points are spaced equidistant on a logarithmic
scale (an equidistant spacing on a linear scale is also possible if you prefer that). Using
fewer modeling points further speeds up measurement times (but can reduce the quality of the model if set too low).
The input power range is split into several equally spaced subranges (= modeling
points) for the calculation of the amplifier model.
With the "Modeling Scale", you can select whether the split is done on a logarithmic or
linear basis.
Remote command:
CONFigure:MODeling:SCALe on page 310
3.12Applying digital predistortion
Access: "Overview" > "Measurement" > "DPD"
Digital predistortion (DPD) is a method to improve the linearity of an RF power amplifier. Basically, DPD is a set of correction values that is added to the input signal to
compensate the non-linearities that occur in the amplifier. The output signal measured
by the R&S VSE then shows the corrected amplifier characteristics.
You can compensate non-linearities with the functionality of the amplifier application.
The application provides two compensation methods: polynomial DPD and direct DPD.
Note that you can only use one of the two DPD types at any time. When you turn on
the polynomial DPD, the R&S VSE automatically turns off the direct DPD and vice
versa.
Using the DPD functionality requires a connection to a signal generator. For more information about configuring generators, see Chapter 3.3.6, "Controlling a signal genera-
●Hammerstein model (R&S VSE-K18M)................................................................ 105
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3.12.1Polynomial DPD
Configuration
Applying digital predistortion
For polynomial DPD, the application calculates the correction values based on a polynomial function, whose characteristics you can define with the settings available for the
system models. The polynomial DPD approach used by the R&S VSE compensates
for "AM/AM" (amplitude-to-amplitude) distortion and "AM/PM" (amplitude-to-phase) distortion.
When you apply the DPD, the correction values are applied to the input signal to
improve the linearity of the amplifier.
The remote commands required to configure the polynomial DPD are described in
Chapter 5.5.13, "Applying digital predistortion", on page 311.
Selecting the DPD method............................................................................................96
Selecting the DPD shaping method.............................................................................. 97
Polynomial DPD Power / Linearity Tradeoff..................................................................97
Selecting the order of model calculation....................................................................... 98
Selecting the DPD method
The amplifier application provides a couple of DPD calculation methods.
●
"Use Generator DPD Option K541"
The signal generator corrects the input signal in real time.
This method requires a Rohde & Schwarz signal generator equipped with option
R&S SMx-K541.
The source of the predistortion values is either a table or a polynomial function.
After a successful measurement, you can apply the predistortion values that were
calculated by the R&S VSE with the "Update" button. (The button is only available
when data has been captured on the R&S VSE and synchronization was success-
ful).
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Configuration
Applying digital predistortion
Note that you have to turn on the DPD model in order to make the DPD work.
As long as you use the same amplifier, the polynomial DPD calculated with this
method is valid for all signals that use a similar bandwidth and frequency as the
signal it was calculated for.
●
"Generate Pre-Distorted Waveform File"
The R&S VSE applies the correction values taken from the table or polynomial
function to each measured sample and generates a waveform file that contains the
corrected input signal. For TDD and FDD signals, we recommend that you use the
full reference signal to generate the DPD.
You can start the DPD calculation and transfer the resulting waveform file to the
connected generator with the "Generate and Load" button. Successful calculation
and transfer are indicated by a green LED. Note that you have to turn on the DPD
model in order to make the DPD work.
Note:
When you use this method, the predistortion information only applies to the cur-
rently selected reference signal and generator level. When you change the refer-
ence signal or generator level, you have to create a file that applies to the new ref-
erence signal.
You can also save the predistorted waveform into a waveform file with the "Store
Pre-Distorted Waveform File" feature for later reference.
Remote command:
CONFigure:DPD:METHod on page 319
Selecting the DPD shaping method
The application provides several ways for DPD calculation (or shaping).
●
"From Table"
Shapes the DPD function based on a table that contains the correction values
required to predistort the signal.
The calculation of the table is based on the "AM/AM" and "AM/PM" polynomial
models.
For more information about the contents and usage of the shaping table, refer to
the documentation of the R&S SMW-K541.
You can define a file name for the DPD table in the corresponding field.
●
"From Polynomial"
Shapes the DPD function based on a correction polynomial that is calculated out of
the model polynomial.
Compared to DPD based on a shaping table, this method does not transfer a list
with correction values. Instead, the application transfers the polynomial coefficients
of the correction polynomial.
For more information, see Chapter 3.11, "Applying system models", on page 92.
You can update the DPD shaping on the signal generator comfortably with the
The "DPD Power / Linearity Tradeoff" describes the effects of the DPD on the amplifier
characteristics.
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Configuration
Applying digital predistortion
When you define a tradeoff of 0 %, the DPD aims for the best linearity (green line in
the illustration below). When you increase the tradeoff value, the DPD aims for an optimization of the output power at the expense of linearity. In the ideal case (red line), the
DPD affects the amplifier characteristics in a way that the best output power is achieved.
Output Power [dBm]
100 %
Original AM/AM Curve
0 %
Input Power [dBm]
Remote command:
CONFigure:DPD:TRADeoff on page 321
Selecting the order of model calculation
The application allows you to compensate for "AM/AM" distortion, "AM/PM" distortion
or both simultaneously. You can turn correction of the distortion models on and off in
the corresponding fields.
If you want to predistort both the "AM/AM" distortion and the "AM/PM" distortion simultaneously, you can select the order in which the curves are calculated and applied to
the I/Q signal on the R&S SMW.
●
"AM/AM" First
Calculates the "AM/AM" first, then calculates the "AM/PM" based on the signal that
has already been corrected by its "AM/AM" distortions.
●
"AM/PM" First
Calculates the "AM/PM" first, then calculates the "AM/AM" based on the signal that
has already been corrected by its "AM/PM" distortions.
Note: the DPD sequence is displayed by the diagram that is part of the dialog box.
Remote command:
The direct DPD is an iterative process in which the correction values are determined
for each sample of the input signal. Compared to the polynomial DPD, the direct DPD
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Configuration
Applying digital predistortion
is not based on a model. It rather calculates the correction values for each sample
directly.
Determining the DPD directly is based on a sequence of individual measurements (iterations). When one iteration is done, the R&S VSE applies the correction values, measures the improved input signal again, applies the correction values etc. This process
goes on until the number of iterations that you have defined is done. Usually, the predistortion gets better with an increasing number of iterations. On the other hand,
increasing the number of iterations also increases the measurement time.
Note that if synchronization is not possible during direct DPD, R&S VSE-K18 continues
with a new measurement (including capture) until synchronization was successful.
Reducing the synchronization confidence level can help in that case.
The result of the direct DPD is an I/Q file that contains a predistorted waveform. When
you save the I/Q file, you can later play it back on a signal generator.
For TDD and FDD signals, we recommend that you use the full reference signal to
generate the DPD.
Further improvement of predistortion
In addition to increasing the number of iterations, it is recommended to apply signal
averaging during each iteration. Averaging helps to remove noise from the signal,
which in turn improves the quality of the predistortion values.
Without averaging, each iteration consists of a single measurement. When you apply
averaging, the number of measurements during each iteration increases, depending on
the number of averages you have defined.
The advantage of the direct DPD compared to the polynomial DPD is, that it takes
memory effects into account. This, and the fact that it is not based on a model, but corrects each sample individually, makes the direct DPD the superior method to predistort
the input signal and determine the ideal DPD effect for your DUT. Note however, that
the correction values that have been determined are only applicable to the signal and
amplifier you have used. If the signal characteristics change in any way, you have to
predistort the signal again.
The direct DPD is especially useful for the following test cases:
●
Determining the best performance of a DUT.
●
Removing external effects from the measurement results, for example a preampli-
fier that should not be considered in the final measurement results.
Continuous statistics during direct DPD calculation
Continuous statistics is automatically disabled during the direct DPD calculation.
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Configuration
Applying digital predistortion
Generator control during direct DPD calculation
When direct DPD is activated, the generator is prevented from changing its attenuator
setting automatically, i.e. it is being set into mode "Fixed" if it was in "Auto" mode so
far. The attenuator mode is switched back to "Auto" when direct DPD is turned off. If
the generator was in "Fixed" or "Manual" mode, the mode is not changed.
Also, the I/Q modulator of the signal generator is set to high quality table mode.
The remote commands required to configure the direct DPD are described in Chap-
ter 5.5.13, "Applying digital predistortion", on page 311.
Automated direct DPD sequence................................................................................100
Manual direct DPD sequence..................................................................................... 101
Direct DPD Power / Linearity Tradeoff........................................................................102
Automated direct DPD sequence
The direct DPD method requires one or more measurements (or iterations) to determine the correction values.
When you select the "Start Direct DPD Sequence" button, the R&S VSE initiates a
sequence of measurements during which the DPD is calculated. The number of measurements performed during the sequence depends on the number of "Iterations" you
have defined. It is also recommended to average each iteration for further improvement of the quality of the input signal. The "Gain Expansion" defines the increase of
input power relative to the peak power value of the reference signal.
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