RADIATED EMISSIONS MEASUREMENT
SYSTEMS
TUTORIAL
BY
MICHAEL
A. NICOLAY
INTRODUCTION
Measuring radiated electromagnetic emissions
first requires a measurement system. A basic measurement system
usually contains a minimum of an antenna and a receiver. To measure
very small signal levels may require the addition of a pre-amplifier to
the receiver system. Figure 1 shows a typical receiver system block
diagram including a pre-amplifier. Figure 1 will be used for the
following discussion.
FIGURE 1. RECEIVER SYSTEM BLOCK DIAGRAM
It is beyond the scope of this text to address
in detail such measurement errors as receiver detection mode errors, radio
frequency pre-selection (RF) filtering, or tuner overload errors. Peak
detection of continuous waves (CW) will mainly be discussed.
There are many terms currently used
to define radiated electromagnetic energy. Some common terms used are non-ionizing
radiation (NIR), electromagnetic fields (EMFs), radiated emissions, and
broadcast signals. In this paper, "emissions" will be used to describe
radiated electromagnetic energy.
Electromagnetic measurement systems are used
to measure power densities, or power spectral densities, of electromagnetic
fields at a point in space. Power density is defined as the "power
per unit area normal to the direction of propagation usually expressed
in units of Watts per square meter W/m2), or for convenience
in units such as milliwatts per square meter (mW/m2), or even
in microwatts per square centimeter (mW/cm2)."
Plane-waves, power densities, electric field strengths (E), and magnetic
field strengths (H) are related by free space loss, i.e, 377 ohms
(W ). Electric field strengths and magnetic
field strengths are expressed in units of Volts per meter (V/m) and Amperes
per meter (A/m), respectively. A field strength is therefore defined
as:
E = Square Root (120pP)
where,
E = rms value of field strength in Volts/meter
P = power density in watt/meter2
120 = impedance of free space in ohms
Power density (PD) is related to the
electric field strength (E) and the magnetic field strength (H) as:
PD = E2/377W
= 377WH2
Again, the rate at which electromagnetic energy
(power) is propagated by a wave -- power density -- is usually specified
in Watts per square meter (W/m2). The power density equation
is:
PD = PT/4pr2
where,
PD = power density in watts/meter2
PT = transmitted power in Watts
r = distance in meters
Radiated electromagnetic fields -- radiated emissions
-- are produced from many sources. Sources of electromagnetic energy
range from manmade sources such as commercial broadcast stations and automobile
ignition systems to natural sources such as galactic noise and lightning.
To further complicate matters, these emissions can drastically differ in
frequencies and in their magnitudes.
Because of the potential wide range of measurement
requirements special measurement systems are sometimes necessary. These
systems must be well-planned or inaccurate measurements may result. Important
design specifications should include system selectivity and system
sensitivity. These terms will be defined and demonstrated in
the following sections.
THE ANTENNA
Measuring radiated emissions, or electromagnetic
energy, begins with the antenna. Antennas are devices that receive
(capture) electromagnetic energy traveling through space. Antennas
can also
be used for transmitting electromagnetic energy. There are many
different types of antennas, some are designed to be "broad-banded," to
receive or transmit over a large frequency range, and some are designed
to receive or transmit at specific frequencies. In any case, all receive
antennas are intended to capture "off-air" electromagnetic energy and to
deliver these "signals" to a receiver. For this discussion, electric
fields (E) will mainly be addressed.
Because antennas can only capture a small
portion of the radiated power, or energy, a correction factor must be added
to the detected emission levels to accurately determine the radiated power
being measured. The actual power received by an antenna is determined
by multiplying the power density of the emission by the receiving
area of the antenna, Ae. This antenna correction factor
is called the "antenna factor."
To further understand antenna factors see
Figure 2. Below are the antenna factor derivation equations.
FIGURE 2. ANTENNA FACTOR
Ae = l2/4p
(Meters2)
The power received by the antenna is then defined by:
Pr = PAe = PGl2/4p
(Watts)
where,
P = power density in Watts/meter2
G = antenna (power) gain
l = wavelength in meters
Combining these equations with the field strength
equation yields:
Pr = E2Gl2/480p2
also,
Pr = Vr2/Zo
where,
Vr = received voltage
Zo = receiver input impedance
then,
Vr2/Zo =
E2Gl2/480p2
Knowing that:
l = 300 meters/second/f(MHz)
since an antenna factor is defined as:
E = (Vrfp/50W)(Square
Root (30/ZoG))
we can simplify and rearrange terms to yield:
K = E/Vr
then,
K = (fp/50W)(Square
Root(30/ZoG))
or in logarithmic form [for Zo = 50 W
(ohm) system]:
K = 20log10 fMHz-GdB-29.78
(dB)
THE RECEIVER AND AMPLIFIER
A receiver is an electro-mechanical device
that receives electromagnetic energy captured by the antenna and then processes
(extracts) the information, or data, contained in the "signal."
The basic function of all receivers is the
same regardless of their specific design intentions, broadcast radio receivers
receive and reproduce commercial broadcast programming, likewise, TV receivers
detect and reproduce commercial television broadcasting programming.
Special, or unique, receivers are sometimes needed to detect and measure
all types of radiated, or transmitted, electromagnetic emissions. These
specialized receivers may be called tuned receivers, field intensity meters
(FIMs), or spectrum analyzers.
Radiated emissions that receiver systems may
be required to measure can be generated from intentional radiators or unintentional
radiators. The information contained in intentionally radiated signals
may contain analog information, such as audio, or they may contain digital
data, such as radio navigation beacon transmissions. Television transmissions,
for example, contain both analog and digital information. This information
is placed in the transmitted emission, called the "carrier," by a process
called "modulation." Again, there are many different types of modulation,
the most common being amplitude modulation (AM) and frequency modulation
(FM). Receivers detect, or extract, the information/data from radiated
emissions by a process called "demodulation", the reverse of modulation.
Many radiated emissions requiring measurements
do not contain any useful information or data at all. As an example,
radiated emissions from unintentional radiators, such as computer systems,
are essentially undesired byproducts of electronic systems and serve no
desired or useful purpose. These undesired emissions can, however,
cause interference to communications system, and if strong enough,
they can cause interference to other unintentional radiating devices. Radiated
signals (if strong enough) can also present possible health hazards to
humans and animals. Because these emissions must be measured to determine
any potential interference problems or health hazard risks, specialized
receiver systems must be used.
An important parameter for any receiver is
its noise figure, or noise factor. This parameter will
basically define the sensitivity that can be achieved with a particular
receiver.
An amplifier, usually called a pre-amplifier,
is sometimes required when attempting to measure very small signals or
emission levels. Because these devices amplify signals, they will also
amplify ambient electromagnetic noise. If improperly used, amplifiers
can detract from the overall system's sensitivity as well as possibly causing
overloading to the receiver's tuner input stage. Overloading a tuner's
input stage is simply supplying a larger signal amplitude than the receiver's
tuner input circuitry is capable of handling, thus, saturating the tuner's
input stage.
Just as with the receiver, it is important
to know what the noise figure, or noise factor, of the selected
amplifier is when designing or specifying a measurement system containing
a pre-amplifier.
The noise figure (Nfig) for a device
(receiver or amplifier) is defined as:
Nfig=10log10No-10log10Gd-(-174
dB+10log10Br)
where,
No = measured noise in milliwatts
Gd = device power gain - linear ratio
BR = receiver bandwidth in Hz
The use of these parameters for designing or specifying
measurement systems will be explained and demonstrated in the following
section.
SPECIFYING OR DESIGNING RADIATED MEASUREMENT
SYSTEMS
When specifying or designing any measurement
receiver system, one should consider that the "system" will include other
devices such as antennas, amplifiers, cabling, and possibly filters.
Because a receiver's selectivity, the ability
to select frequencies or frequency bands, is primarily a function of the
receiver's tuner design, and will be chiefly dependent on the individual
receiver selection, selectivity will not be specifically addressed in this
text. Receiver system sensitivity, however, presents one of
the greatest difficulties, or challenges, when designing or specifying
receiver measurement systems. Therefore, the sensitivity of the two
basic types of receiver systems, one with a pre-amplifier
and one without a pre-amplifier, will be addressed in some detail.
Because antennas are not perfect devices and
have associated "losses," the following examples will include explanations
for these error corrections. As mentioned previously, amplifiers
will not only amplify the emissions being measured but they will also amplify
ambient electromagnetic noise. These ambient conditions can drastically
change the overall sensitivity of a measurement system. Another potential
problem associated with using amplifiers is that they also generate internal
electromagnetic noise. Being active devices they will introduce their own
internal electromagnetic noise into the receiver system, again having an
influence on the total system's noise level, thus, its sensitivity.
Some corrections for the above mentioned problems
are necessary to accurately calculate both the receiver's signal input
sensitivity and (more importantly) the total system's ambient sensitivity.
Without knowing the total measurement system's ambient sensitivity,
measurements may not be possible down to anticipated emission levels.
In electromagnetic measurement systems terms
such as ambient sensitivity, system sensitivity, and receiver sensitivity
have been used interchangeably. More confusing expressions commonly
used are terms such as "receiver noise floor," or "system noise floor."
In this text, the term "system sensitivity"
will be defined as ambient electromagnetic noise level seen by, and at,
the antenna for 0 dB Signal-to-Noise ratio at the receiver's intermediate-
frequency (I-F) stage. System sensitivities defined herein are for
far-field conditions.
The following are general terms and definitions
that will be used in describing and calculating the following receiver/system
parameters:
General Definitions:
1. Nfig (dB) = Noise Figure = 10log10 Noise Factor
(NF)
2. Ae (dB) = Effective Capture Area = 10log10
( l2/4p ) - for unity gain
3. T (dB) = Average Room Temperature = 10log10 290°K
(K=degrees Kelvin)
4. BR (dB) = 10log10 Receiver Bandwidth (Hertz)
5. K (dB) = Boltzman's Constant
= 10log10 1.4 x 10-23 Watts/K/Hz
6. Se (dBm/m2) = System Sensitivity = Nfig-174+BR-Ae
THE RECEIVER AND ANTENNA SYSTEM SENSITIVITY
Receiver sensitivity is one of the most important
design parameters to consider when designing or specifying any measurement
system. This parameter will determine the lowest signal level that
the receiver will be capable of detecting or measuring. However,
when designing a system to measure radiated radio frequency (RF) emissions
(signals), it is important to go further in your analysis. The sensitivity
level at the receiver may be considerably different than the sensitivity
level at the antenna, especially if a pre-amplifier is attached between
the antenna and the receiver. If not considered, measuring the "noise floor"
of the receiver system, itself, instead of the anticipated radiated
emissions levels may result. The following measurement system discussion
will be as shown in Figure 1, without the use of the pre-amplifier.
Receiver sensitivity (SR) is defined
as the RF noise power level generated within the receiver. It may
also be defined as the co-channel interference level for 0 dB signal-to-noise
ratio, defined as:
SR = NF K T Br (Watts)
or in logarithmic form:
SR=10log10NF+10log10K+10log10T+10log10BR
(dBW)
where,
K = Boltzman's Constant = 1.4 x 10-23 Watts/K/Hz
T = temperature in degrees Kelvin
BR = receiver I-F bandwidth in Hertz
NF = receiver noise factor
Note: Noise figures and noise factors
are different ways of specifying noise. In this text, noise factors
will be used to describe linear ratios, and noise figures will be
used to describe logarithmic ratios.
Again, a receiver's selectivity, the ability
to select frequencies or frequency bands, is chiefly dependent on the receiver's
tuner design, which is mainly the function of the receiver selection.
Because receiver system sensitivity presents one of the greatest challenges,
sensitivity will be ddressed in detail.
For simplicity, a spectrum analyzer
will be used as the receiver for this discussion. We will first determine
the receiver's sensitivity from its indicated power level. The indicated
power level of a spectrum analyzer is essentially the base-line trace observed
on its cathode-ray tube (CRT) display,
usually expressed in dBm. It may be more useful to convert this unit
(dBm) to a more useful unit such as dBV. In a 50W
system this conversion is done by adding 107 dB to the indicated power
level displayed on the analyzers CRT display. As an example, an indicated
power level of -90 dBm (on the CRT display) is equivalent to an electric
plane-wave of 17mV. Note: The
107 dB factor is
only applicable in a 50W system.
FIGURE 3. SPECTRUM ANALYZER DISPLAY
Converting the receiver's
sensitivity into a plane-wave field strength equivalency, ambient field
strength reference at the antenna, is not difficult but may be confusing
at first because of the unit
conversions and the concept of equivalent field strengths. As shown above,
it may be easier to first convert the receiver's indicated sensitivity
power level (dBm), to a plane-wave equivalent voltage
( dBmV). After this conversion, the equivalent
field strength sensitivities can be easily calculated in units of dBmV/m
or V/m. This conversion can be accomplished using "antenna factors."
The antenna factor (dB/m) when added to the
indicated sensitivity level (dBmV) of the receiver
will produce the equivalent field strength sensitivity referenced at the
antenna (dBmV/m), referenced to an isotropic
antenna. For example, an indicated field strength of 17 dBmV
plus an antenna factor of 25 dB/m is equal to a field strength of 42 dBmV/m.
Because the antenna factor does not
include any losses such as cable losses and filter losses, these losses
will have to be accounted for to accurately calculate equivalent field
strengths or field strength sensitivities.
For ease in calculating, these losses (in
dB) can be added to the antenna factor. This resultant number, when added
to the indicated receiver sensitivity, in dBmV,
will yield an equivalent ambient field strength or electric plane-wave
sensitivity. Note: This will only be true for a particular
antenna at a specific frequency. Each antenna factor will be different
for each measurement frequency.
Using the following measurement receiver (spectrum
analyzer) system specifications as an example:
System Specifications:
1. Receiver sensitivity (indicated) = -90 dBm
2. The antenna factor at 45.50 MHz = 25 dB
3. The cable loss at 45.50 MHz = 2 dB
By performing the following steps the measurement
system's plane-wave equivalent sensitivity, in dBm
V/m, would be:
Step 1. First, converting the indicated receiver
sensitivity level from a power (dBm) to an equivalent voltage (dBmV),
assume a 50W system, would yield:
SR = -90 dBm + 107 dB = 17 dBmV
Step 2. Correcting for cable losses and antenna
factors, the system sensitivity (Se) would be:
Se = 17 dBmV + 25 dB/m
+ 2 dB = 44.0 dBmV/m
Step 3. By taking the antilog of the sensitivity
level calculated in step 2, the equivalent, or effective, plane-wave electric
field strength sensitivity (Se) in mV/m
will be:
Se = 44.0 dBmV/m = 10
(44.0dBmV/m/20) = 158.49 mV/m
THE RECEIVER, PRE-AMPLIFIER, AND ANTENNA
SYSTEM SENSITIVITY
Now that the sensitivity of a receiver system with
just an antenna has been defined, the sensitivity of a measurement system
including a pre-amplifier will be explained -- without the use
of antenna factors. This will be slightly more complicated than
a measurement system containing only a receiver and an antenna.
Again, the system's sensitivity will be defined
as the minimum ambient signal level, power density, or field strength that
the system can detect or measure referenced at the receive antenna.
To determine the overall system sensitivity
the total system's noise factor must be calculated using the noise factors
of each active device within the system. If the manufacturer of each
device has not specified these parameters they can be measured and/or calculated.
To calculate the system noise factor the following
equation is used when a preamplifier is included in the measurement system:
NFs = NF1 + ((NF2-1)/G))
where,
NFs
= noise factor of the system
NF1
= noise factor of the preamplifier
NF2
= noise factor of the receiver
G = Gain of
the Preamplifier (Power)
Because antenna factors will not be used, there
are two other parameters that will be needed to complete the overall system
sensitivity calculations, the measurement frequency must be defined
and the antenna gain must be known. The frequency is important because
the effective capture area (Ae) of the antenna must be
known. This calculation is based on the equation l
2/4p ; Lambda (l
) being the emission wavelength specified in meters. The antenna gain is
important because it obviously effects the system's sensitivity.
To make the system sensitivity calculations
easier, logarithmic expressions will be used in most cases. Again,
noise figures will be used to express noise factors in logarithmic form.
The system sensitivity (Se) of
the measurement system can be calculated using the following:
Se = Nfig-174*+Br-Ae
(dBW/m2)
where,
Nfig
= system noise figure (dB)
BR
= receiver bandwidth, in Hertz (dB)
Ae
= antenna effective capture area (dB)
* = 10 log10 Boltzman's Constant x 290 °K
+ 30 dB
As an example, the following will demonstrate
how to calculate the system's sensitivity (Se) using the following
device parameters:
Device Parameters:
1. Receiver I-F Bandwidth = 9 kHz
2. Receiver Noise Figure = 15 dB
3. RF Preamplifier Power Gain = 26 dB
4. Preamplifier Noise Figure = 4.15 dB
5. Measurement Frequency = 635 MHz
First, the receiver sensitivity (SR)
is equal to:
SR = 15+(-228.5)+24.6+39.5=-149.4
(dBW)
= -119.4 (dBm)
(For convenience in later comparisons, dBW was converted
to dBm. You will notice (later) the difference between the receiver
sensitivity and the ambient system's sensitivity.)
Next, we must calculate the system noise figure
(Nfig). This will be more complicated because we must obtain
the answer in logarithmic form from calculations done in a linear
manner:
1. NF1 = 4.15 dB=10(4.15/10)=
2.6
2. NF2 = 15 dB=10(15/10)=
31.6
3. G = 26 dB=10(26/10)= 398
4. NF3=2.6+((31.6-1)/398)=2.68
then,
Nfig = 10log10 2.68 = 4.3 dB
The effective capture area of the antenna, Ae,
will now be calculated as follows (for unity gain antenna):
1. l= 300
m/s ÷ frequency (MHz)
= 300 / 635
= .47 meters
2. Ae= l2
/4p
= .472 / (4
x 3.1415)
= .0176 meters2
= 10 log10
.0176 = -17.5 dB
The receiver bandwidth (BR) calculation
will be:
1. BR = 10 log10 Frequency (Hz)
2. BR = 10 log10 9000 Hz = 39.5 dB
Finally, using equation Se= Nfig-174+Br-Ae,
we can calculate the total system sensitivity. The system sensitivity (power
density) will be:
Se= 4.3-174+39.5-(-17.5)= -112.7
dBm/m2
Now that the system sensitivity (Se)
is known, defined in power density units (dBm/m2), it may be
more useful to convert further to more commonly used units such as
field strengths. Again, the units of measurement for field strengths are
Volts per meter (V/m), or for convenience dBmV/m
(decibel ratio of V/m referenced to 1 microvolt).
For ease in understanding, and for simplicity
in calculating, it is recommended that unit changes be done by first converting
power densities (dBm/m2) to milliwatts per square centimeter
(mW/cm2), then converting to field strength units such as V/m
or dBmV/m. In converting power densities
to field strengths the following conversion factors will be
helpful:
1. Units/cm2 (square centimeters)
= units/m2 - 40 dB
2. Volts/meter (V/m) = Square Root
(mW/cm2 x 3763.6W)
Using the above conversion factors (1 and 2),
the equivalent field strength sensitivity would be:
1. -112.7 dBm/m2 = -152.7 dBm/cm2
2. -152.7 dBm/cm2 = 10(-152.7dBm/10) = 5.4 x
10-16 mW/cm2
3. Square Root (5.4 x 10-16mW/cm2 x 3763.6W)
= 1.4 x 10-6V/m
4. 20log101.4 x 10-6V/m = 2.9dBmV/m
Some additional helpful conversion factors for radiated measurement
units are:
dBW/m2 = dBV/m-25.8
dBW/m2 = dBmV/m-145.8
dBm/m2 = dBmV/m-115.8
dBm/cm2 = dBmV/m-155.8
dBm/cm2 = dBV/m-35.8
dBW/m2 = dBm/m2-30.0
dBW/m2 = dBW/cm2+40.0
dBW/m2 = dBm/cm2+10.0
The measurement system's sensitivity has now been
calculated and defined. It is important to note, however, that the
system may not be capable of measuring all ambient signal levels down to
this level. As mentioned earlier, ambient noise levels may be higher
than the measurement system sensitivity. This will result in the ambient
noise levels masking potential measurements down to these levels.
These potential problems can be resolved with
proper system pre-selection (RF input filtering) and receiver I-F bandwidth
adjustments.
SUMMARY
In summary, designing or specifying receiver
systems requires that each system be designed or specified for its particular
application. Two important design parameters that must be addressed
are the system's selectivity and its sensitivity. This can become
demanding because measurement systems may be required to detect and measure
radiated emissions comprised of narrow-band and/or wide-band signals, they
may also be required to measure radiated signal strengths varying from
very small to very large amplitude levels.
Selectivity, the ability to
tune (select) to a frequency or a band of frequencies, is primarily dependent
on the particular tuner (receiver) selection in addition to any radio frequency
(RF) input
filtering, called pre-selection. By filtering undesired input
RF emissions, and with proper receiver intermediate-frequency (I-F) filter
adjustments, it is possible to measure very low emission amplitudes present
in frequency bands containing much higher amplitude emissions or noise
levels. These filter selections will be based on the emission types being
measured and on the ambient conditions under which the measurements are
made.
Sensitivity, the lowest rf amplitude
levels that a receiver system will be capable of measuring, is dependent
on several variables. These variables are involved with specific
antenna selections, receiver noise figures/factors, pre-amplifier gains
and noise figures/factors (if used), and the system's filtering and cabling.
If not properly planned, all these devices can detract from the overall
system's performance.
The first step in designing or specifying
a measurement system is to understand the actual measurement requirements.
This should include the emission frequencies, their bandwidth's, and probable
emission amplitude levels. This information will determine any required
RF and I-F filtering and, in particular, the overall system's sensitivity
needs.
The second step should be to calculate the
total system parameters to include all the devices selected to be used
in the measurement system. Any pre-selection required can usually
be
accomplished using passive high-pass, low-pass, or band-pass filters.
These types of filters can greatly assist in removing any undesired ambient
noise or signals removed from the intended measurement frequency or frequency
band of interest.
The RF filtering will primarily determine the "carrier-to-noise
ratio" of the system. RF filtering will also prevent possible overloading
to the system's pre-amplifier or to the receiver if a pre-amplifier is
not used. Overloading, exceeding the maximum allowed input levels,
to the system's pre-amplifier or receiver input levels can result in creating
intermodulation products within these devices and may result in inaccurate
measurement results.
The I-F filtering selection will primarily
determine the "signal-to-noise ratio" within the receiver itself.
The overall system sensitivity will thus be
dependent on the noise figure of the selected receiver, the noise figure
and gain of the preamplifier (if used), the system cabling losses, and
the gains of the selected antennas.
For high-gain systems, used for measuring
low signal levels, extreme caution should be taken to ensure that the combination
of the antenna gains and amplifier gains will not produce signal levels
that exceed the maximum input levels allowed for the selected receiver.
Again, because of the importance, saturating an amplifier or a receiver's
input stage may create intermodulation products and may result in inaccurate
measurements.
REFERENCES
Brench, C.E., "Antenna Differences and Their Influences on Radiated
Emission Measurements," Paper presented at the 1990 IEEE
Interference Symposium on EMC.
Duff, W.G. 1976. A handbook on mobile communications. Don
White
Consultants, Inc.
Hewlett Packard. Spectrum Analyzer Series. Application Note 150-10.
Kraus, J.D. 1988. Antennas, 2nd ed. New York: MGraw Hill.
Nahan, N.S., Kanda, M., Larsen, E.B., Crawford, M.L., 1985.
Methodology for standard electromagnetic field measurements. IEEE
transactions on instrumentation and measurement. IM-34, No.
4
(December)
Society of Automobile Engineers. 1978. EMC antennas and antenna
factors: how to use them. Aerospace Information Report. 1509
(January).