Spectrum analyzer
A spectrum analyzer circa 2005
The main PCB from a 20 GHz Agilent N9344C spectrum analyser. Showing thestripline PCB filters, and modular block
construction.
A spectrum analyzer measures the magnitude of an input signal versus frequency within the full frequency
range of the instrument. The primary use is to measure the power of the spectrum of known and unknown
signals. The input signal a spectrum analyzer measures is electrical, however, spectralcompositions of
other signals, such as acoustic pressure waves and optical light waves, can be considered through the use
of an appropriatetransducer. Optical spectrum analyzers also exist, which use direct optical techniques
such as a monochromator to make measurements.
By analyzing the spectra of electrical signals, dominant frequency, power, distortion, harmonics, bandwidth,
and other spectral components of a signal can be observed that are not easily detectable in time
domain waveforms. These parameters are useful in the characterization of electronic devices, such
as wireless transmitters.
The display of a spectrum analyzer has frequency on the horizontal axis and the amplitude displayed on
the vertical axis. To the casual observer, a spectrum analyzer looks like an oscilloscope and, in fact, some
lab instruments can function either as an oscilloscope or a spectrum analyzer.

History
This section
requires expansion.(December 2012)
A spectrum analyzer circa 1970
The first spectrum analyzers, in the 1960s, were swept-tuned instruments.[1]
Following the discovery of the Fast Fourier Transform in 1965, the first FFT-based analyzers were
introduced in 1967.[2]
Today, there are three basic types of analyzer: the swept-tuned spectrum analyzer, the vector signal
analyzer, and the real-time spectrum analyzer.[1]
Types[
A modern spectrum analyzer display
Spectrum analyzer types are dictated by the methods used to obtain the spectrum of a signal. There are
swept-tuned and FFT based spectrum analyzers:

A swept-tuned spectrum analyzer uses a superheterodyne receiver to down-convert a portion of the
input signal spectrum (using a voltage-controlled oscillator and a mixer) to the center frequency of
a band-pass filter. With a superheterodyne architecture, the voltage-controlled oscillator is swept
through a range of frequencies, enabling the consideration of the full frequency range of the
instrument.

A FFT spectrum analyzer computes the discrete Fourier transform (DFT), a mathematical process that
transforms a waveform into the components of its frequency spectrum, of the input signal.
Some spectrum analyzers, such as real-time spectrum analyzers, use a hybrid technique where the
incoming signal is first down-converted to a lower frequency using superheterodyne techniques and then
analyzed using fast fourier transformation (FFT) techniques.
Form factor[
Spectrum analyzers tend to fall into three form factors: benchtop, portable and handheld.
Benchtop[
This form factor is useful for applications where the spectrum analyzer can be plugged into AC power,
which generally means in a lab environment or production/manufacturing area. Bench top spectrum
analyzers have historically offered better performance and specifications than the portable or handheld
form factor. Bench top spectrum analyzers normally have multiple fans (with associated vents) to dissipate
heat produced by the processor. Due to their architecture, bench top spectrum analyzers typically weigh
more than 30 pounds (14 kg). Some bench top spectrum analyzers offer optional battery packs, allowing
them to be used away from AC power. This type of analyzer is often referred to as a "portable" spectrum
analyzer.
Portable[
This form factor is useful for any applications where the spectrum analyzer needs to be taken outside to
make measurements or simply carried while in use. Attributes that contribute to a useful portable spectrum
analyzer include:

Optional battery-powered operation to allow the user to move freely outside.

Clearly viewable display to allow the screen to be read in bright sunlight, darkness or dusty conditions..

Light weight (usually less than 15 pounds (6.8 kg)).
Handheld[
This form factor is useful for any application where the spectrum analyzer needs to be very light and small.
Handheld analyzers offer a limited capability relative to larger systems. Attributes that contribute to a useful
handheld spectrum analyzer include:

Very low power consumption.

Battery-powered operation while in the field to allow the user to move freely outside.

Very small size

Light weight (usually less than 2 pounds (0.91 kg)).
Theory of operation[
Swept-tuned[
As discussed above in types, a swept-tuned spectrum analyzer down-converts a portion of the input signal
spectrum to the center frequency of a band-pass filter by sweeping the voltage-controlled oscillator through
a range of frequencies, enabling the consideration of the full frequency range of the instrument.
The bandwidth of the band-pass filter dictates the resolution bandwidth, which is related to the minimum
bandwidth detectable by the instrument. As demonstrated by the animation to the right, the smaller the
bandwidth, the more spectral resolution. However, there is a trade-off between how quickly the display can
update the full frequency span under consideration and the frequency resolution, which is relevant for
distinguishing frequency components that are close together. For a swept-tuned architecture, this relation
for sweep time is useful:
Where ST is sweep time in seconds, k is proportionality constant, Span is the frequency range under
consideration in Hertz, and RBW is the resolution bandwidth in Hertz.[3] Sweeping too fast, however,
causes a drop in displayed amplitude and a shift in the displayed frequency.[4]
Also, the animation contains both up- and down-converted spectra, which is due to a frequency
mixer producing both sum and difference frequencies. The local oscillator feedthrough is due to the
imperfect isolation from the IF signal path in the mixer.
For very weak signals, a pre-amplifier is used, although harmonic and intermodulation distortion may lead
to the creation of new frequency components that were not present in the original signal.
FFT-based[
With a FFT based spectrum analyzer, the frequency resolution is
, the inverse of the
time T over which the waveform is measured and Fourier transformed.
With Fourier transform analysis in a digital spectrum analyzer, it is necessary to sample the input signal
with a sampling frequency
that is at least twice the bandwidth of the signal, due to theNyquist limit.[5] A
Fourier transform will then produce a spectrum containing all frequencies from zero to
. This can
place considerable demands on the required analog-to-digital converterand processing power for the
Fourier transform, making FFT based spectrum analyzers limited in frequency range.
Frequency spectrum of the heating up period of a switching power supply (spread spectrum) incl. waterfall diagram over
a few minutes.
Hybrid superheterodyne-FFT[
Since FFT based analyzers are only capable of considering narrow bands, one technique is to combine
swept and FFT analysis for consideration of wide and narrow spans. This technique allows for faster sweep
time.
This method is made possible by first down converting the signal, then digitizing the intermediate
frequency and using superheterodyne or FFT techniques to acquire the spectrum.
One benefit of digitizing the intermediate frequency is the ability to use digital filters, which have a range
of advantages over analog filters such as near perfect shape factors and improved filter settling time. Also,
for consideration of narrow spans, the FFT can be used to increase sweep time without distorting the
displayed spectrum.
Realtime FFT
Illustration showing Spectrum Analyzer Blind Time
Comparison between Swept Max Hold and Realtime Persistence displays
Bluetooth signal hidden behind wireless LAN signal
Most modern spectrum analyzers are now almost exclusively Hybrid Superheterodyne-FFT based giving a
significant improvement in sweep time. However, even in such cases there is still processing time required
to sample the spectrum and calculate the FFT. For this reason, both swept-tuned and FFT based analyser
produce "blind time" meaning that while calculation of the spectrum is being performed, the instrument has
gaps and misses information of the RF spectrum being applied to the RF front end.
A realtime spectrum analyser does not have any such blind time—up to some maximum span, often called
the "realtime bandwidth". The analyser is able to sample the incoming RF spectrum in the time domain and
convert the information to the frequency domain using the FFT process. FFT's are processed in parallel,
gapless and overlapped so there are no gaps in the calculated RF spectrum and no information is missed.
Online realtime and offline realtime
In a sense, any spectrum analyzer that has vector signal analyzer capability is a realtime analyzer. It
samples data fast enough to satisfy Nyquist Sampling theorem and stores the data in memory for later
processing. This kind of analyser is only realtime for the amount of data / capture time it can store in
memory and still produces gaps in the spectrum and results during processing time.
FFT overlapping
Minimizing distortion of information is important in all spectrum analyzers. The FFT process applies
windowing techniques to improve the output spectrum due to producing less side lobes. The effect of
windowing may also reduce the level of a signal where it is captured on the boundary between one FFT
and the next. For this reason FFT's in a Realtime spectrum analyzer are overlapped. Overlapping rate is
approximately 80%. An analyzer that utilises a 1024 point FFT process will re-use approximately 819
samples from the previous FFT process.[6]
Minimum signal detection time
This is related to the sampling rate of the analyser and the FFT rate. It is also important for the realtime
spectrum analyzer to give good level accuracy.
Example: for an analyser with 40 MHz of realtime bandwidth (the maximum RF span that can be processed
in realtime) approximately 50 Msample/second (complex) are needed. If the spectrum analyzer
produces 250 000 FFT/s an FFT calculation is produced every 4 µs. For a 1024 point FFT a full spectrum is
produced 1024 x (1/50 x 106), approximately every 20 µs. This also gives us our overlap rate of 80% (20 µs
− 4 µs) / 20 µs = 80%.
Realtime display examples
Persistence
Realtime spectrum analyzers are able to produce much more information for users to examine the
frequency spectrum in more detail. A normal swept spectrum analyzer would produce max peak, min peak
displays for example but a realtime spectrum analyzer is able to plot all calculated FFT's over a given
period of time with the added colour-coding which represents how often a signal appears. For example, this
image shows the difference between how a spectrum is displayed in a normal swept spectrum view and
using a "Persistence" view on a realtime spectrum analyzer.
Hidden signals
Realtime spectrum analyzers are able to see signals hidden behind other signals. This is possible because
no information is missed and the display to the user is the output of FFT calculations. An example of this
can be seen on the right.
Typical functionality
Center frequency and span
In a typical spectrum analyzer there are options to set the start, stop, and center frequency. The frequency
halfway between the stop and start frequencies on a spectrum analyzer display is known as the center
frequency. This is the frequency that is in the middle of the display’s frequency axis. Span specifies the
range between the start and stop frequencies. These two parameters allow for adjustment of the display
within the frequency range of the instrument to enhance visibility of the spectrum measured.
Resolution bandwidth
As discussed in the operation section, the resolution bandwidth filter or RBW filter is the bandpass
filter in the IF path. It's the bandwidth of the RF chain before the detector (power measurement device).[7] It
determines the RF noise floor and how close two signals can be and still be resolved by the analyzer into
two separate peaks.[7] Adjusting the bandwidth of this filter allows for the discrimination of signals with
closely spaced frequency components, while also changing the measured noise floor. Decreasing the
bandwidth of an RBW filter decreases the measured noise floor and vice versa. This is due to higher RBW
filters passing more frequency components through to the envelope detector than lower bandwidth RBW
filters, therefore a higher RBW causes a higher measured noise floor.
Video bandwidth
The video bandwidth filter or VBW filter is the low-pass filter directly after the envelope detector. It's the
bandwidth of the signal chain after the detector. Averaging or peak detection then refers to how the digital
storage portion of the device records samples—it takes several samples per time step and stores only one
sample, either the average of the samples or the highest one.[7] The video bandwidth determines the
capability to discriminate between two different power levels.[7] This is because a narrower VBW will
remove noise in the detector output.[7] This filter is used to “smooth” the display by removing noise from the
envelope. Similar to the RBW, the VBW affects the sweep time of the display if the VBW is less than the
RBW. If VBW is less than RBW, this relation for sweep time is useful:
Where ST is sweep time in seconds, k is proportionality constant, Span is the frequency range under
consideration in Hertz, RBW is the resolution bandwidth in Hertz, and VBW is the video bandwidth in
Hertz.[8]
Detector
With the advent of digitally based displays, some modern spectrum analyzers use analog-to-digital
converters to sample spectrum amplitude after the VBW filter. Since displays have a discrete number of
points, the frequency span measured is also digitised. Detectors are used in an attempt to adequately map
the correct signal power to the appropriate frequency point on the display. There are in general three types
of detectors: sample, peak, and average

Sample detection – sample detection simply uses the midpoint of a given interval as the display point
value. While this method does represent random noise well, it does not always capture all sinusoidal
signals.

Peak detection – peak detection uses the maximum measured point within a given interval as the
display point value. This insures that the maximum sinusoid is measured within the interval; however,
smaller sinusoids within the interval may not be measured. Also, peak detection does not give a good
representation of random noise.

Average detection – average detection uses all of the data points within the interval to consider the
display point value. This is done by power (rms) averaging, voltage averaging, or log-power averaging.
Displayed average noise level[
The Displayed Average Noise Level (DANL) is just what it says it is—the average noise level displayed
on the analyzer. This can either be with a specific resolution bandwidth (usually in dBm), or normalized to
1 Hz (usually in dBm/Hz)[9]
Radio-frequency uses[
Spectrum analyzers are widely used to measure the frequency
response, noise and distortion characteristics of all kinds of radio-frequency (RF) circuitry, by comparing
the input and output spectra.
In telecommunications, spectrum analyzers are used to determine occupied bandwidth and track
interference sources. For example, cell planners use this equipment to determine interference sources in
the GSM frequency bands and UMTS frequency bands.
In EMC testing, a spectrum analyzer is used for basic precompliance testing; however, it can not be used
for full testing and certification. Instead, an EMI receiver like the Rohde & Schwarz ESU EMI
Receiver, Agilent Technologies N9038A MXE EMI, or Gauss Instruments TDEMI is used.
A spectrum analyzer is used to determine whether a wireless transmitter is working according to federally
defined standards for purity of emissions. Output signals at frequencies other than the intended
communications frequency appear as vertical lines (pips) on the display. A spectrum analyzer is also used
to determine, by direct observation, the bandwidth of a digital or analog signal.
A spectrum analyzer interface is a device that connects to a wireless receiver or a personal computer to
allow visual detection and analysis of electromagnetic signals over a defined band of frequencies. This is
called panoramic reception and it is used to determine the frequencies of sources of interference to
wireless networking equipment, such as Wi-Fi and wireless routers.
Spectrum analyzers can also be used to assess RF shielding. RF shielding is of particular importance for
the siting of a magnetic resonance imaging machine since stray RF fields would result in artifacts in an MR
image.[10]
Audio-frequency uses[
Spectrum analysis can be used at audio frequencies to analyse the harmonics of an audio signal. A typical
application is to measure the distortion of a nominally sinewave signal; a very-low-distortion sinewave is
used as the input to equipment under test, and a spectrum analyser can examine the output, which will
have added distortion products, and determine the percentage distortion at each harmonic of the
fundamental. Such analysers were at one time described as "wave analysers". Analysis can be carried out
by a general-purpose digital computer with a sound card selected for suitable performance[11] and
appropriate software. Instead of using a low-distortion sinewave, the input can be subtracted from the
output, attenuated and phase-corrected, to give only the added distortion and noise, which can be
analysed.[12]
An alternative technique, total harmonic distortion measurement, cancels out the fundamental with a notch
filter and measures the total remaining signal, which is total harmonic distortion plus noise; it does not give
the harmonic-by-harmonic detail of an analyser.
Optical spectrum analyzer[
An optical spectrum analyzer uses reflective and reflective techniques to separate out the wavelengths of
light. An electro-optical detector is used to measure the intensity of the light, which is then normally
displayed on a screen in a similar manner to a radio- or audio-frequency spectrum analyser.
The input to an optical spectrum analyzer may be simply via an aperture in the instrument's case, an optical
fiber or an optical connector to which a fiber-optic cable can be attached.
Different techniques exist for separating out the wavelengths. One method is to use a monochromator, for
example a Czerny-Turner design, with an optical detector placed at the output slit. As the grating in the
monochromator moves, bands of different frequencies (colors) are 'seen' by the detector, and the resulting
signal can then be plotted on a display.
The frequency response of optical spectrum analyzers tends to be relatively limited, eg 1600 - 800
nm (infrared to red), depending on the intended purpose, although (somewhat) wider-bandwidth general
purpose instruments are available.
See also[

Electrical measurements

Electromagnetic spectrum

Measuring receiver

Radio frequency sweep

Spectral leakage

Spectral music

Spectrogram

Spectrometer