Noise — Friend and Foe of Engineers
By Wolfgang Damm,
Product Management Director, Wireless Telecom Group
Foe — agreed, but friend? How can noise be appreciated by engineers who labor at the edge of
technology when trying to move signals and information as fast as possible from A to B? Isn’t
noise something we all want to avoid and eliminate? This column addresses engineers who are
interested in exploring the concept of utilizing noise for test and measurement purposes. It dis-
cusses how white Gaussian noise can be employed as a versatile signal source. A short introduc-
tion discusses causes, sources, and quantities relevant to noise, followed by two application ex-
amples that utilize noise: noise as a broadband reference and noise load to determine optimal
system operation levels.
What Is Noise?
Noise is omnipresent in the universe. With the exception of absolute zero temperature point at
0 Kelvin (0 K), all materials produce noise with a power level proportional to the physical tem-
perature of the material. Noise is generated by random vibrations of conducting electrons and
holes in the material. It is often referred to as thermal noise. A variety of other effects generate
noise as well, but it would exceed the scope of this document to discuss them all. Noise energy
emitted by one single element is rather minuscule, but the almost infinite count of vibrating ele-
ments sum up to a significant power level — large enough to challenge us when developing
sensitive receivers, or operating with ADCs and DACs that have a high bit resolution, just to
name two applications.
White Noise
Thermal noise is “white” and has a Gaussian amplitude distribution. The term “white” specifies
constant output power over a linear frequency spectrum, as opposed to “pink” noise that
provides constant power over a logarithmic frequency spectrum. Because of this evenly distrib-
uted power, certain frequency segments of equal bandwidth provide the same power level with
white noise, which can be very helpful when analyzing filters, amplifiers, and system responses.
Overall output power of white noise sources is dependent on the specified bandwidth. Output
characteristics can be described in different ways:
Power: dBm, dBm/Hz, dBm/frequency band
Voltage: V/Hz
Ratios: ENR (excess noise ratio), noise temperature (K)
The fact that power spectral density is constant over frequency implies that noise power is pro-
portional to bandwidth. If the measurement bandwidth is doubled, the detected noise power is
doubled as well and increases by 3 dB. Total power (P) in dBm and spectral power (PS) in
dBm/Hz of white noise sources are related by the following equation:
Wireless Telecom Group Whitepaper: Noise - Friend and Foe of Engineers
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P = PS + 10log(BW).
BW is the measured bandwidth, and PS is a characteristic quantity of a particular noise source,
usually provided on datasheets. Specific noise sources are built for optimal flatness over the fre-
quency band.
Gaussian Distribution And Crest Factor
Statistical evaluations of related occurring events present always certain kinds of distribution
curves. Gaussian distribution, also known as normal distribution, is the most common way
events take place. Most white noise sources provide Gaussian distribution of their spectral
power.
Why is Gaussian distribution of such importance? The randomness of noise sources requires a
mathematical model that allows calculating the probability density of events. Gaussian distribu-
tion right and left of the mean probability is of equal size. Crest factor, the peak-to-average ra-
tio, is also an important quantity for noise sources. It allows calculating the likelihood of un-
wanted events relative to the mean probability. Such renegade events may cause an overload of
an amplifier input, distortion of a signal, or a bit error. Obviously, the fewer of those natural but
unwanted events happen, the better. High quality white Gaussian noise sources offer crest
Wireless Telecom Group Whitepaper: Noise - Friend and Foe of Engineers
www.wtcom.com, Phone: +1-973-386-9696
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Figure 1 shows two white noise sources. Spectrum A has a large variance in power distribution,
and thus provides a low crest factor. Spectrum B has a high crest factor, so unwanted signal levels
are less frequent.
Gaussian Distribution
with high crest factor
Gaussian Distribution
with low crest factor
Noise spectrum A
Noise spectrum B
Frequency
Frequency
factors of up to 18 dB, placing the probability of unwanted events far beyond reasonable meas-
urement capabilities.
Application 1: Noise as a Broadband Reference
We discussed two key characteristics of white noise: It offers all frequencies in a specified fre-
quency band simultaneously, and that with a constant power level. These features make noise
sources desirable elements whenever analyzing frequency bands of filters, circuits, instruments,
or systems, as, for example, filter analysis or spectrum analyzer calibration.
A simple way to calibrate spectrum analyzers is to use a broadband white noise source to monit-
or the analyzer's frequency response. Noise sources are available with spectral flatness that far
exceeds typical spectrum analyzer accuracy; hence, this flat frequency distribution makes white
noise sources ideal for calibration purposes. A spectrum analyzer's flatness is influenced by the
effects of its internal RF attenuator, preselector, and mixing mode gain variations. Injecting
noise into a spectrum analyzer as a reference source can therefore provide an accurate meas-
urement of the amplitude variations versus frequency.
Another way to normalize the errors associated with spectrum analyzer measurement is to em-
ploy a signal generator that sweeps the required frequency while the analyzer stores the re-
sponse. A noise source has several advantages over this approach:
Cost: The cost of a noise source is insignificant compared to the cost of a broadband signal
generator with similar output-versus-frequency characteristics.
Size: A noise source can be made much smaller than a signal generator.
Speed: When performing broadband measurements, the oscillator must be set, responses
stored, next frequency set, next responses stored, and so on. Even with fast signal
generators, this can take quite a long time, depending on the number of samples
taken. White noise sources generate all the frequencies simultaneously, so the limit-
ing factor is only the measurement speed of the spectrum analyzer. The procedure
requires less time, which dramatically reduces cost.
Accuracy: Noise sources can be accurately measured to within tenths of a dB by NIST-traceable
methods.
Application 2: Noise Load to Determine System Behavior —
Noise-Power-Ratio (NPR) Measurements
Serious dynamic range problems can occur in systems loaded with multi-channel signals. Any
nonlinearity in the system (e.g. an amplifier) causes intermodulation products among the input
frequencies. This produces new frequencies that may fall within the bandwidth of other chan-
nels, therefore creating distortions. The amount of distortion increases with the number of
channels and the degree of amplifier saturation. For example, two uncorrelated tones may, at
times, add in-phase to create peak voltages that are about 6 dB higher than the RMS voltage.
Wireless Telecom Group Whitepaper: Noise - Friend and Foe of Engineers
www.wtcom.com, Phone: +1-973-386-9696
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The peak-to-RMS voltage ratio increases by 10 log(2n) dB, where n is equal to the number of un-
correlated signals of the same amplitude. Many uncorrelated load signals can be simulated by
white Gaussian noise for noise power ratio (NPR) testing. The NPR method is an accurate means
of reproducing multi-carrier intermodulation effects
and determining the amplifier's performance under
worst-case loading conditions.
Intermodulation testing of amplifiers with only two
tones has many shortcomings if the life system is ac-
tually loaded with numerous signals. First, the dis-
tortion product amplitude may be dependent on the
frequency spacing of the input signals. Second, the
amplifier will perform differently when loaded with
many signals. The peak-to-average ratio of multiple
modulated signals is much greater than two or sev-
eral tones. These large peaks stress the amplifier or
device under test (DUT) to a greater degree. The
NPR method emulates many signals by loading the
amplifier with white Gaussian noise.
Intermodulation distortion manifests it-
self in two primary ways. In a receiver
LNA, adjacent channel signals cause in-
band distortion products. For a transmit-
ter power amplifier, distortion of the
primary signal will cause interference in
adjacent channels. Both cases are
closely related and can be accounted for
with the noise power ratio (NPR) test.
NPR is a measure of distortion produced
in a particular band by a device that is
loaded with just white noise. Measure-
ment of NPR versus output power, or
loading, is used to define the optimum
operating point for maximum signal-to-
noise ratio (SNR). The NPR of a DUT is
degraded primarily by two factors. The
first is the distortion products that are
produced under high loading conditions.
The second is the noise floor of the amp-
lifier that will become dominant under
very low loading conditions. By making
numerous measurements with different
loading levels, a curve will be generated,
as shown in Figure 2. NPR is poor at low
loading levels because the amplifier is being operated near its own noise floor. The NPR is also
poor at very high loading levels. But the slope on this side of the curve is steeper since the dis-
Wireless Telecom Group Whitepaper: Noise - Friend and Foe of Engineers
www.wtcom.com, Phone: +1-973-386-9696
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Figure 2: Plot of NPR vs. loading
condition to determine the optimum op-
erating point for maximum SNR.
Figure 3: Output noise spectrum during NPR Meas-
urement. Noise is injected over the whole operating
bandwidth (a). Now, a notch filter is applied to sup-
press a known amount of power in a specific band-
width (b). The excess of measured power is generated
by the DUT.
tortion products are dominant in this case. If distortions are caused by nth-order harmonics, in-
termodulation products increase by (n-1) dB for every 1 dB increase of the loading level. For ex-
ample, for third-order distortions, intermodulation products increase 2 dB for every 1 dB in-
crease of the loading level. Systems are often operated at signals a few dB below the point of
maximum NPR. To perform an NPR test, an accurate level of white Gaussian noise is applied to
the amplifier. A bandstop (notch) filter is then inserted to create a "quiet" channel. The NPR is
the ratio between the noise power measured with and without the notch filter (Figure 3).
Conclusion
Noise can indeed help to solve test and measurement challenges for engineers. The applications
discussed above — noise as a broadband reference and noise to measure system load behavior
— are just two of many. A wide variety of noise sources available for specific applications. They
are affordable, and offer a flat response over a wide frequency band.
Wireless Telecom Group Whitepaper: Noise - Friend and Foe of Engineers
www.wtcom.com, Phone: +1-973-386-9696
Page 5 of 5

# Noise — Friend and Foe of Engineers

Foe — agreed, but friend? How can noise be appreciated by engineers who labor at the edge of technology when trying to move signals and information as fast as possible from A to B? Isn’t noise something we all want to avoid and eliminate? This column addresses engineers who are interested in exploring the concept of utilizing noise for test and measurement purposes.

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