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Home » Basic Principles Of Radar
[1.0] Basic Principles Of Radar
v1.0.0 / 1 of 2 / 01 feb 03 / greg goebel / public domain
* This chapter provides basic definitions and concepts in radar technology.
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[1.1] RADIO WAVE FREQUENCY & WAVELENGTH
[1.2] RADIO WAVE POLARIZATION, PHASE, INTERFERENCE, & PROPAGATION
[1.3] RADIO SYSTEM BASICS
[1.4] ANTENNA BASICS
[1.5] A SIMPLE PULSE RADAR SYSTEM
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[1.1] RADIO WAVE FREQUENCY & WAVELENGTH
* Radar is a variant of radio technology and shares many of the same basic
concepts. It is useful to discuss fundamental concepts of radio operation
to provide a basis for discussing fundamental concepts of radar operation.
Late in the 19th century, researchers discovered that if an alternating
electric current were run through a wire or rod, it emitted an invisible
form of radiation that could generate an alternating electric current
in a separate wire or rod. This invisible radiation was quickly realized
to be a form of "electromagnetic radiation", a disturbance of
electric and magnetic fields that propagated through space.
Electromagnetic radiation is in the form of waves, conceptually similar
to the waves set up by shaking a rope up and down, and propagating at
a speed of 300,000,000 meters per second (186,000 miles per second). The
waves could be generated at varying "frequencies", defined by
the number of cyclical variations of the wave that passed through a plane
every second. Frequencies were once measured in "cycles per second
(CPS)", but now are universally defined in terms of "hertz (Hz)",
after Heinrich Hertz, a pioneering radio researcher.
The frequencies of electromagnetic radiation are usually large numbers,
and so it is useful to use "metric prefixes" as shorthand --
for example:
kilohertz (kHz): 1,000 hertz
megahertz (MHz): 1,000,000 hertz
gigahertz (GHz): 1,000,000,000 hertz
terahertz (THz): 1,000,000,000,000 hertz
The full range of frequencies of electromagnetic radiation is known as
the "electromagnetic spectrum". Radio waves only take up part
of this spectrum, generally involving kilohertz, megahertz, or gigahertz
radio emissions.
Above about 300 GHz, electromagnetic radiation moves into a region of
the spectrum known as "infrared"; and then with increasingly
higher frequencies into the region of visible light that we can see with
our eyes; and finally into energetic radiation defined as the "ultraviolet",
"X-ray", and (at the very highest frequencies) "gamma ray"
regions of the spectrum.
Put a little bit more simply, radio waves are the same thing as visible
light, both being forms of electromagnetic radiation. The only difference
is that radio waves have lower frequencies.
Incidentally, electromagnetic waves are entirely different from sound
waves, which are mechanical disturbances propagating through the air,
water, or a solid medium. The two kinds of waves can be confused because
very low frequency electromagnetic waves are sometimes said to be at "audio"
frequencies, and of course electromagnetic waves can be used to transmit
audio waves, as turning on a household radio shows.
* This document focuses only on radio waves. Sometimes it is easier to
talk about radio waves in terms of their "wavelength" in meters
instead of their frequency. There is a simple relationship between the
wavelength and frequency of a wave:
wavelength = wave_propagation_speed / frequency
Since the propagation speed of electromagnetic radiation in free space
is 300,000,000 meters per second, then for electromagnetic radiation this
is:
wavelength = 300,000,000 / frequency
If frequency is given in megahertz, this simplifies to:
wavelength = 300 / frequency
For example:
1 kHz = 300 kilometers
3 kHz = 100 kilometers
10 kHz = 30 kilometers
30 kHz = 10 kilometers
100 kHz = 3 kilometers
300 kHz = 1 kilometer
1 MHz = 300 meters
3 MHz = 100 meters
10 MHz = 30 meters
30 MHz = 10 meters
100 MHz = 3 meters
300 MHz = 1 meter
1 GHz = 30 centimeters
3 GHz = 10 centimeters
10 GHz = 3 centimeters
30 GHz = 1 centimeter
100 GHz = 3 millimeters
300 GHz = 1 millimeter
Various frequency / wavelength ranges, or "bands", have been
defined for radars, with general classes of equipment usually operating
in one or a few bands. The band names, with the frequency / wavelength
corresponding to the low end of each band, are as follows:
ELF (Extremely Low Frequency) 30 Hz 10,000 kilometers
VF (Voice Frequency) 300 Hz 1,000 kilometers
VLF (Very Low Frequency) 3 kHz 100 kilometers
LF (Low Frequency) 30 kHz 10 kilometers
MF (Medium Frequency) 300 kHz 1 kilometer
HF (High Frequency) 3 MHz 100 meters
VHF (Very High Frequency) 30 MHz 10 meters
UHF (Ultra High Frequency) 300 MHz 1 meter
L 1 GHz 30 centimeters
S 2 GHz 15 centimeters
C 4 GHz 7.5 centimeters
X 8 GHz 3.75 centimeters
Ku 12 GHz 2.5 centimeters
K 18 GHz 1.67 centimeters
Ka 27 GHz 1.1 centimeters
V 40 GHz 7.5 millimeters
W 75 GHz 4 millimeters
mm 110 GHz 2.73 millimeters
The VLF through UHF band definitions were inherited from radio engineering.
The bands above UHF don't follow a clear order, which apparently was partly
by intent, as a security measure. The K band originally included the Ku
and Ka bands, but it turned out that the center portion of the K-band
was useless for most military purposes as water vapor in the atmosphere
soaked up radio waves in that range. The portion of the K-band "above"
the absorption range became the "Ka-band", while the portion
"under" the absorption range became the "Ku-band".
Just to make things more confusing, different band definitions are used
in other electronic fields. Radio engineers retain the ELF through UHF
definitions, but take the UHF band up to 3 GHz, and then cover the higher
frequencies with the "Super High Frequency (SHF)" band from
3 to 30 GHz, covering the centimetric / microwave region, and then the
"Extremely High Frequency (EHF)" band from 30 to 300 GHz, covering
the millimeter wave region.
Electronic countermeasures systems are defined by a band scheme entirely
different from the radar and radio scheme, with the bands much more conveniently
arranged from "A" to "M" in order of increasing frequency.
Oddly, there isn't a one-to-one correspondence between the countermeasures
bands and the radar bands, and though there was some interest at one time
at applying the more rational countermeasures scheme to radar, it wasn't
practical.
BACK_TO_TOP
[1.2] RADIO WAVE POLARIZATION, PHASE, INTERFERENCE, & PROPAGATION
* As electromagnetic radiation is a wave phenomenon, it has certain characteristics
associated with waves, such as "polarization", "phase",
and "wave interference".
The oscillations of an electromagnetic wave occur back and forth across
the direction of the wave's propagation. This means that the wave has
a certain "polarity". If the wave's oscillations are up and
down, the wave is said to be "vertically polarized"; if they
are back and forth, the wave is said to be "horizontally polarized".
Of course, the wave could also be polarized at any angle between those
two extremes.
The concepts of "phase" and "wave interference" are
a bit trickier to explain. Suppose you have a tank of water, and are using
some sort of vibrating element to generate waves. If you stick another
vibrating element in the water operating at the same vibration rate and
same intensity, it will generate waves of the same frequency and height
(or "amplitude"), but the peaks and valleys of the waves generated
by the second vibrating element will not necessarily coincide with those
of the first. In other words, they won't have the same "phase".
The phase of the two sets of waves could be matched up, with the peaks
and valleys of both coinciding; or they could be completely out of phase,
with the peaks of one coinciding with the valleys of the other and the
reverse, a condition known as "antiphase"; or they could have
a phase difference anywhere between those two extremes.
The really interesting thing is that the two sets of waves add to each
other. If the two sets of waves are exactly in phase, they add up into
a single set of waves of twice the amplitude of one of the sets of waves.
If they are exactly antiphase, they cancel out, and the water in the tank
is smooth. If they are between those two extremes, the additive effect
is intermediate. This phenomenon is known as "interference".
Radio waves also have phase and can interfere. A single transmission
may go from point A to point B by various paths. For example, one path
may be a straight line, while another may be a long path due to a reflection
or "bounce" off a mountain. Such "multipath effects"
cause the "ghosting" sometimes seen on TV transmissions, with
a faint image slightly offset from the main image. They can also cause
"phase delays" that seem to alter the direction of the beam
by interference. Controlled interference effects can be used to deliberately
shift the direction of a radio beam, a scheme known as "electronic
steering" and discussed later.
* One final comment before moving on to radio and radar technology: radio
waves generally propagate over a line-of-sight, weakening with distance,
as anybody who's driven from town to town in a car with a radio realizes,
with the music fading out as one town is left behind, and becoming stronger
as another town is approached.
The radio waves can propagate through the sky or over the ground, and
as noted can often propagate by multiple paths. At night, radio waves
can bounce off the ionospheric layer in the upper atmosphere, allowing
them to propagate over the horizon, if in a somewhat unpredictable fashion.
Such "ionospheric bounce" tends to work better at lower frequencies.
Anybody's who's ever played around with a broadcast radio receiver late
at night knows remote stations can be picked up, sometimes over great
distances.
Other atmospheric effects can interfere with radio signals. Higher frequencies
can be blocked by heavy rainstorms or snowstorms, and lightning can thrown
"noise" into radio transmissions. Particle flows from eruptions
on the Sun can cause massive disruptions of radio communications. There
is also a variable background of radio noise from human sources that can
cause unwanted interference.
Radio waves vary in their interactions with solid matter. Radio waves,
like light, can be absorbed or reflected by matter. Metals and water,
for example, tend to reflect radio waves, while soils tend to absorb them.
Also as with light, radio reflections can be "specular", as
if bounced off a mirror, or "diffuse", as if bounced off a rough
and uneven surface.
If radio waves can penetrate a material, the penetration is greater at
longer wavelengths. Radio wave can penetrate buildings well enough, and
very long wavelength can even penetrate a good depth through the sea or
into the ground. Very short wavelengths are strongly attenuated and have
limited range.
BACK_TO_TOP
[1.3] RADIO SYSTEM BASICS
* A radar system is basically an evolution of a radio system, and it is
useful to define the basic elements of a radio system first.
A radio system consists of a "transmitter" that produces radio
waves and one or more "receivers" that pick them up, with both
transmitter and receiver(s) fitted with antennas. The very earliest "wireless
telegraphy" radio systems used a transmitter that simply generated
a burst of radio energy by opening an electric circuit with a telegraph
key and causing a spark. The radio waves propagated through space and
set up an electric current in a receiving antenna, which in turn closed
a relay switch, possibly using an "amplifier" circuit to boost
the electrical signal. Messages were sent using Morse code.
The problem with this simple scheme is that the spark generated waves
over a wide and indiscriminate range of frequencies, with a single receiver
picking up and mixing up transmissions from every transmitter in the line
of sight.
The way to get around this problem is to fit each transmitter with a
"variable oscillator", an electronic circuit that generates
electrical signals at different frequencies, as set by a knob turned by
the transmitter operator. Receivers are then fitted with a "variable
filter", another electronic circuit that can be set by a knob turned
by the receiver operator to block out all frequencies except one.
This scheme allows multiple transmitters to operate in a given area without
interference. The transmitter operator sets the transmitter oscillator
to a given frequency; the receiver operator sets the receiver filter to
the same frequency; and the transmitter operator uses a telegraph key
to turn the output of an oscillator on and off, with the receiver operator
picking up the output over the airwaves. The receiver will usually be
fitted with a "detector" circuit to convert high-frequency signals
into a direct-current signal to activate the relay switch.
This is obviously the same concept that is used in tuning a voice radio
to different channels, though a voice radio works somewhat differently
from a radio telegraph. A voice radio also uses a variable oscillator.
The voice of a user is converted into an electrical waveform which is
"mixed" with the output of the oscillator, shifting the voice
signal up in frequency to that of the oscillator, and transmitted. The
oscillator frequency is known as the "carrier" frequency, since
it "carries" the voice signal.
The receiver has its own variable oscillator, tuned to the same carrier
frequency, which is mixed with the received signal, a process that somewhat
magically obtains the original voice waveform. The voice waveform is converted
back into sound through a loudspeaker.
The process of converting a voice (or music or whatever) into an electrical
signal is known as "modulation". There are two classic forms
of modulation: "amplitude modulation (AM)", in which the electrical
signal varies in amplitude along with variations in amplitude of the voice
input; and "frequency modulation (FM)", in which the electrical
signal varies in frequency along with variations in the amplitude of the
voice input. The process of mixing and unmixing frequencies is known as
"heterodyning".
In many cases, heterodyning is used to translate a voice or other signal
up to an "intermediate frequency", which is then heterodyned
again to produce an output signal of even higher frequency. This is done
because it gets more difficult to handle signals at higher frequencies,
and this scheme, known as "superheterodyning", allows most of
the handling to be performed at the intermediate frequency.
A traditional analog television signal is conceptually much the same
as a voice radio. The TV sound track is transmitted with FM, while the
basic visual signal, which is black and white, is transmitted by AM. There
are various schemes used in different nations for overlaying color signals,
but they are devious and irrelevant to this discussion.
Incidentally, transmitter output power is measured in watts, or (as far
as radar is concerned) more usually kilowatts (kW, thousands of watts)
and megawatts (MW, millions of watts). Receiver "sensititivity",
or the ability of the receiver to amplify received signals, is determined
in terms of "decibels", defined as:
decibels = 10 * LOG10( output_power / input_power )
The amplification factor is commonly referred to as "gain".
Incidentally, a radio doesn't transmit or receive on a single frequency
but on a range or band of frequencies. Although the details are beyond
the scope of this simple document, the "bandwidth" is roughly
proportional to the amount of information carried by the signal. A TV
channel needs more bandwidth than a hi-fidelity radio channel, for example,
just as a hi-fidelity radio channel needs more bandwidth than a low-fidelity
radio channel.
BACK_TO_TOP
[1.4] ANTENNA BASICS
* A transmitter needs an antenna to send its radio signal, and a receiver
needs an antenna to pick up that radio signal. The design of these antennas
is not trivial.
The simplest form of antenna is the "dipole". Suppose the electrical
output of an oscillator is directed down two conductors, not connected
at the ends. This will produce radiate electromagnetic energy from the
open-circuit ends. It radiates energy much more effectively if the conductors
are bent at the ends to form a right angle, with each bend being a quarter-wavelength
long relative to the oscillator frequency.
This is a "half-wave" dipole. It is not only effective in generating
radio waves at a particular frequency, it is also effective in picking
them up. This is true in general of all antennas: they are "reciprocal",
working much the same in transmission or reception, just in different
directions.
By itself, a dipole "broadcasts" in all radial directions evenly,
but a directed focus can be obtained, through interference effects, by
building an antenna with multiple dipoles, spaced at carefully designed
intervals. Such "dipole arrays" were common with early longwave
radars, and in a modified form persist today.
Another way to create a "directional" antenna with a dipole
is to mount it within a row of parallel conductive rods, with the rods
of decreasing length to the "front" of the dipole (relative
to the direction of focus) and of increasing length to the "back"
of the dipole. This type of antenna is known as a "Yagi-Uda"
or just "Yagi" antenna. It is recognizable as the modern broadcast
TV antenna.
A conceptually simpler directional antenna is the parabolic dish. This
is configuration familiar with a modern satellite-TV receiver. It's really
very much the same as using a parabolic mirror to focus light, only the
wavelength of electromagnetic radiation is longer. While parabolic dishes
are usually circular, elliptical or cylindrical dishes with parabolic
curvature can also be used if the radio beam needs to be focused along
one axis but not along the other. An elliptical dish with the long axis
vertical is used to create a narrow horizontal beam, useful for height-finding,
while one with the long axis horizontal gives a narrow vertical beam,
useful for surface targeting.
* Incidentally, directional antennas don't always generate all their
radio output in a nice neat directional beam. They may generate "sidelobes"
that cause unwanted transmissions to the sides of the beam, or a "backlobe"
in the reverse direction. The sidelobes and backlobe not only produce
signals in undesired directions, they also rob the main lobe of energy.
In addition, as a general rule, the larger the receiver dish, the greater
the receiver sensitivity, since it creates a bigger "bucket"
or "eye" to collect radio waves. However, the longer the wavelength,
the bigger the dish has to be to focus the radio waves. Another little
related fact is that the dish doesn't have to be solid. It can be a mesh,
just as long as the mesh grid spacing is less than that of the radar operating
wavelengths. This makes for a lighter antenna, and also one not so easily
disturbed by the wind.
BACK_TO_TOP
[1.5] A SIMPLE PULSE RADAR SYSTEM
* A discussion of voice radio is useful for background in discussing simple
radar systems, but is also somewhat incidental, since a simple radar works
more like a wireless telegraphy set.
The best way to explain radar is to imagine that you are standing on
one side of a canyon, and shout in the direction of the distant wall of
the canyon. After a few moments, you will hear an echo. The length of
time it takes an echo to come back is directly related to how far away
the distant canyon wall is. Double the distance, and the length of time
doubles as well.
If you know that the speed of sound is about 1,200 KPH (745 MPH) at sea
level, then if you have a stopwatch you can actually figure out how far
away the distant canyon wall is. If it takes four seconds for the echo
to come back, then since sound travels about 330 meters (1,080 feet) in
a second, the distance is about 660 meters (2,160 feet).
Radar uses exactly the same principle, but it times echoes of radio or
microwave pulses and not sound. Like a wireless telegraphy set, a simple
radar has a transmitter and a receiver that can usually be tuned to a
range of frequencies, with the transmitter sending out pulses, short bursts,
of electromagnetic radiation and the receiver picking them up.
In the case of the radar, the receiver is picking up echoes from a distant
target, which are then timed to determine the distance to the target.
Early radars simply used an oscilloscope to perform the timing. An oscilloscope
measures an electrical signal on a beam that moves or "sweeps"
from one side of a display to the other at a certain rate. The rate is
determined by a "timebase" circuit in the oscilloscope.
For example, the sweep rate might push the sweep from one side of the
display to the other in 100 microseconds (millionths of a second). If
the display were marked into ten intervals, that would mean the sweep
would pass through each interval in ten microseconds. While 100 microseconds
would be shorter than the human eye could follow, the sweep is normally
generated repeatedly, allowing the eye to see it.
Since electromagnetic radiation propagates at 300,000,000 meters per
second, or 300 meters per microsecond, then each 10 microsecond interval
would correspond to 3,000 meters, or 3 kilometers. If the sweep on the
scope is "triggered" to start when the radar transmitter sends
out the radio pulse, and the sweep displays an echo on the eighth interval
on the display, then the pulse has traveled a total of 8 kilometers. Since
this is the two-way distance, that means that the target is 4 kilometers
away.
* The display scheme described here is known as an "A scope",
and allows the user to determine the range to a target. It would also
be nice to know what the direction to the target is, in terms of its "altitude
(vertical direction)" and "range (left to right direction".
This is a bit trickier to describe, but no more complicated in the end.
Some early radars, like the famous British "Chain Home" sets
that helped win the Battle of Britain, simply transmitted radio waves
out in a flood over their field of view, and used a directional receiver
antenna to determine the direction of the echo. Chain Home actually used
a scheme where the power of the echo was compared at separated receiver
antennas to give the direction, which astoundingly actually worked reasonably
well. Other such "floodlight" radars used directional receiver
antennas that could be steered to identify the direction of the echo.
Floodlight radars were quickly abandoned. They spread their radio energy
over a wide area, meaning that any echo was faint and so range was limited.
The next step was to make a radar with steerable antennas. For example,
two directional antennas, one for the transmitter and the other for the
receiver, could be placed on a steerable mount and pointed like a searchlight.
The transmitter antenna generated a narrow beam that could be steered
like a searchlight, and if the beam hit a target, an echo would be picked
up by the receiving antenna on the same mount. The direction of the antennas
naturally gave the direction to the target, at least to an accuracy limited
by the width in degrees of the beam, while the distance to the target
was given by the trace on the A-scope.
Of course, it would be more economical and easier to use one antenna
for both transmit and receive instead of separate antennas, and it was
possible because a radar transmits a pulse and then waits for an echo,
meaning it doesn't transmit and receive at the same time. The problem
is that the receiver is designed to listen for a faint echo, while the
transmitter is designed to send out a powerful pulse. If the receiver
were directly linked to the transmitter when a pulse is sent out, the
receiver would be fried.
The solution to this problem was the "duplexer", a circuit
element that protects the receiver, effectively becoming an open connection
while the transmit pulse was being sent, and then closing again immediately
afterward so that the receiver could pick up the echo. The receiver is
also generally fitted with a "limiter" circuit that blocked
out any signals above a certain power level. This prevents, say, transmissions
from another nearby radar from destroying the receiver.
* After this evolution of steps, we have a simple, workable radar. It
has a single, steerable antenna that can be pointed like a searchlight.
The antenna repeatedly sends out a radio pulse and picks up any echoes
reflected from a target. An A-scope display gives the interval from the
time the pulse is sent out and the time the echo is received, allowing
the operator to determine the distance to the target.
The transmitter emits pulses on a regular interval, typically a few dozen
or a few hundred times a second, with the A scope trace triggered each
time the transmitter sends out a pulse. The number of pulses sent out
each second is known as the "pulse repetition rate" or more
generally as the "pulse repetition frequency (PRF)", measured
in hertz.
The width of a pulse is an important but tricky consideration. The longer
the pulse, the more energy sent out, improving sensitivity and range.
Unfortunately, the longer the pulse, the harder it is to precisely estimate
range. For example, a pulse that last 2 microseconds is 600 meters long,
and in that case there is no real way to determine the range to an accuracy
of better than 600 meters, and there is also no way to track a target
that is closer than 600 meters. In addition, a long pulse makes it hard
to pick out two targets that are close together, since they show up as
a single echo.
PRF is another tricky consideration. The higher the PRF, the more energy
is pumped out, again improving sensitivity and range. The problem is that
it makes no sense to send out pulses at a rate faster than echoes come
back, since if the radar sends a pulse and then gets back an echo from
an earlier pulse, the operator is likely to be confused by the "ghost
echo". This is actually not too much of a problem, since a little
quick calculation shows that even a PRF of 1,000 gives enough time to
get an echo back from 150 kilometers (185 miles) away before the next
pulse goes out.
However, propagation of radar waves can be freakishly affected by atmospheric
conditions, and sometimes radars can get back echoes from well beyond
their design range. This is why radars were developed that could be switched
between two different PRFs. Switching from one PRF to another would not
affect an echo from the current pulse, since the timing would remain the
same, but such a switching would cause a ghost return from a current pulse
to jump on the display.
* Incidentally, the power of the pulse is given as "peak power",
usually in kilowatts or megawatts. This may be an impressive value, but
it's only the power that goes into the pulse itself. Suppose we have a
pulse width of 2 microseconds with a peak power of 150 kilowatts. If we
have a PRF of 500, then the time from pulse to pulse, or "pulse period",
is 1/500 = 2 milliseconds, or two thousandths of a second.
This means that the average power transmitted by our radar is only:
150 kW * ( 2 microseconds / 2 milliseconds) = 0.15 kW = 150 watts
-- which is about as much as the power draw of a bright household light
bulb.
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