Doppler effect in radar
MOVING-TARGET INDICATION (MTI)
It is possible to remove from a radar display
the majority of clutter, that is, echoes corresponding to stationary targets,
thus showing only the moving targets. This is often required, although
of course not in those radar systems that are used for mapping or for navigational
applications. One of the methods of eliminating clutter is the use of MTI,
which employs the Doppler effect in its operation.
DOPPLER EFFECT
The apparent frequency of electromagnetic waves depends
on the relative radial motion of the source and the observer.
This was postulated in 1842 by Christian Doppler, and put on a firm mathematical
basis by Armand Fizeau in 1848. The Doppler effect is observable for light,
and is responsible for the so-called red-shift of the spectral lines from
stellar objects moving away from the solar system. It is equally noticeable
for sound, being the cause of the change in the pitch of a whistle from
a passing train. It can also be used to advantage in several forms of radar.
Consider an observer situated in an aeroplane
approaching a fixed source of radiation, with a relative velocity + v .
If the pilot's plane were stationary, he would note fo, wave
crests (or troughs) per second if the transmitting frequency were fo.
However, because he is moving towards the source, he of course encounters
more than fo crests per second. In fact, the number observed
under these conditions is given by the relativistic equation, which for
speeds less than 10% of the speed of light can be approximated as shown:
Consequently, the Doppler frequency difference can
be approximated as
where:
=
the new observed frequency
=
Doppler frequency difference.
Considering the wavelength of the signal as received
by the pilot in the aeroplane, from the relativistic equation,
The above equation is where there is a positive approach
velocity, that is where the pilot is moving towards the frequency source.
If the pilot is moving away from the frequency source fo, then
v is negative, and
in the
above equations merely acquires a negative sign.
In radar where a moving target is
involved, the signal undergoes the Doppler shift when impinging upon the
target. This target becomes the "source" of the reflected waves, so that
we now have a moving source (the pilot and the aeroplane), moving and a
stationary observer (the stationary radio receiver). For the case where
the source emitting a signal of frequency
is
now moving at a velocity v, and the observer is stationary, the relativistic
Doppler effect is such that the new observed frequency
is
given by the following equation, with the approximation for speeds less
than 10% the speed of light:
The overall effect is thus compounded. Hence the
Doppler frequency
observed
by the stationary source transmitting at a frequency fo, which
then impinges on a moving target moving radially towards this stationary
source at a velocity v, and is then reflected off of this target, is given
by, either the classical or relativistic equation :
Determining the doppler shift
,
Which for speeds less than 10% of the speed of light
reduces to the approximation:
Considering the wavelength of the signal as received
by the stationary observer, from the relativistic equation,
which gives an equation showing what the final wavelength
looks like on return from the target, that is,
For velocities less than 10% of the speed of light,
the same magnitude of Doppler shift is observed regardless of whether a
target is moving toward the radar, or away from it, with a given velocity.
However, it will represent an increase in frequency in the former case,
and a reduction in the latter. For speeds greater than 10% of the speed
of light, the magnitude of the Doppler shift is not the same in the cases
of moving away from the radar and moving towards the radar. The 10% figure
used throughout this description is not to be taken as a definite cut-off
value, but as a guide to when the relativistic effects start to become
noticeable. Note also that the Doppler effect is observed only for radial
motion, not for tangential motion. Thus, no Doppler effect will be noticed
if a target moves across the field of view of a radar. However, a Doppler
shift will be apparent if the target is rotating, and the resolution of
the radar is sufficient to distinguish its leading edge from its trailing
edge. One example where this has been employed is the measurement of the
rotation of the planet Venus (whose rotation cannot be observed by optical
telescope because of the very dense cloud cover).
On the basis of this frequency change, it is possible
to determine the relative velocity of the target, with either pulsed or
CW radar.
The source code (version
Rev.1 98/08/10) is available according to the GNU
Public License.
Tony Townsend,
tonyart@ieee.org