With a relatively slow moving source,
vs,r is small in comparison to
v and the equation approximates to
where .
However the limitations mentioned above still apply. When the more complicated exact equation is derived without using any approximations (just assuming that everything: source, receiver, and wave or signal are moving linearly) several interesting and perhaps surprising results are found. For example, as Lord Rayleigh noted in his classic book on sound, by properly moving it would be possible to hear a symphony being played backwards. This is the so-called "time reversal effect" of the Doppler effect. Other interesting cases are that the Doppler effect is time dependent in general (thus we need to know not only the source and receivers' velocities, but also their positions at a given time) and also in some circumstances it is possible to receive two signals or waves from a source (or no signal at all). In addition there are more possibilities than just the receiver approaching the signal and the receiver receding from the signal.
All these additional complications are for the classical—i.e., non-
relativistic Doppler effect. However, all these results also hold for the relativistic Doppler effect as well.
The first attempt to extend Doppler's analysis to light waves was soon made by Fizeau. In fact, light waves do not require a medium to propagate and the correct understanding of the Doppler effect for light requires the use of the
Special Theory of Relativity. See
relativistic Doppler effect.
A common misconception
Craig Bohren pointed out that some physics textbooks erroneously state that the observed frequency
increases as the object approaches an observer and then decreases only as the object passes the observer. In fact, the observed frequency of an approaching object declines monotonically from a value above the emitted frequency, through a value equal to the emitted frequency when the object is closest to the observer, and to values increasingly below the emitted frequency as the object recedes from the observer. Bohren proposed that this common misconception might occur because the
intensity of the sound increases as an object approaches an observer and decreases once it passes and recedes from the observer and that this change in intensity is misperceived as a change in frequency.
Applications
Sirens
The
siren on a passing
emergency vehicle will start out higher than its stationary pitch, slide down as it passes, and continue lower than its stationary pitch as it recedes from the observer. Astronomer
John Dobson explained the effect thus:
- "The reason the siren slides is because it doesn't hit you."
In other words, if the siren approached the observer directly, the pitch would remain constant (as
vs, r is only the radial component) until the vehicle hit him, and then immediately jump to a new lower pitch. Because the vehicle passes by the observer, the radial velocity does not remain constant, but instead varies as a function of the angle between his line of sight and the siren's velocity:
where
vs is the velocity of the object (source of waves) with respect to the medium, and is the angle between the object's forward velocity and the line of sight from the object to the observer.
Astronomy
The Doppler effect for electromagnetic waves such as light is of great use in
astronomy and results in either a so-called
redshift or
blue shift. It has been used to measure the speed at which
stars and
galaxies are approaching or receding from us, that is, the
radial velocity. This is used to detect if an apparently single star is, in reality, a close
binary and even to measure the rotational speed of stars and galaxies.
The use of the Doppler effect for light in
astronomy depends on our knowledge that the
spectra of stars are not continuous. They exhibit
absorption lines at well defined frequencies that are correlated with the energies required to excite
electrons in various
elements from one level to another. The Doppler effect is recognizable in the fact that the absorption lines are not always at the frequencies that are obtained from the spectrum of a stationary light source. Since blue light has a higher frequency than red light, the spectral lines of an approaching astronomical light source exhibit a blue shift and those of a receding astronomical light source exhibit a redshift.
Among the
nearby stars, the largest radial velocities with respect to the
Sun are +308 km/s (BD-15°4041, also known as LHS 52, 81.7 light-years away) and -260 km/s (Woolley 9722, also known as Wolf 1106 and LHS 64, 78.2 light-years away). Positive radial velocity means the star is receding from the Sun, negative that it is approaching.
Temperature measurement
Another use of the Doppler effect, which is found mostly in plasma physics and astronomy, is the estimation of the temperature of a gas (or ion temperature in a plasma) which is emitting a
spectral line. Due to the thermal motion of the emitters, the light emitted by each particle can be slightly red- or blue-shifted, and the net effect is a broadening of the line. This line shape is called a
Doppler profile and the width of the line is proportional to the square root of the temperature of the emitting species, allowing a spectral line (with the width dominated by the Doppler broadening) to be used to infer the temperature.
Radar
The Doppler effect is used in some types of
radar, to measure the velocity of detected objects. A radar beam is fired at a moving target — e.g. a motor car, as police use radar to detect speeding motorists — as it approaches or recedes from the radar source. Each successive radar wave has to travel farther to reach the car, before being reflected and re-detected near the source. As each wave has to move farther, the gap between each wave increases, increasing the wavelength. In some situations, the radar beam is fired at the moving car as it approaches, in which case each successive wave travels a lesser distance, decreasing the wavelength. In either situation, calculations from the Doppler effect accurately determine the car's velocity. Moreover, the
proximity fuze, developed during World War II, relies upon Doppler radar to explode at the correct time, height, distance, et cetera.
Medical imaging and blood flow measurement
An echocardiogram can, within certain limits, produce accurate assessment of the direction of blood flow and the velocity of blood and cardiac tissue at any arbitrary point using the Doppler effect. One of the limitations is that the
ultrasound beam should be as parallel to the blood flow as possible. Velocity measurements allow assessment of cardiac valve areas and function, any abnormal communications between the left and right side of the heart, any leaking of blood through the valves (valvular regurgitation), and calculation of the
cardiac output. Contrast-enhanced ultrasound using gas-filled microbubble contrast media can be used to improve velocity or other flow-related medical measurements.
Although "Doppler" has become synonymous with "velocity measurement" in medical imaging, in many cases it is not the frequency shift (Doppler shift) of the received signal that is measured, but the phase shift (
when the received signal arrives).
Velocity measurements of blood flow are also used in other fields of
medical ultrasonography, such as
obstetric ultrasonography and
neurology. Velocity measurement of blood flow in arteries and veins based on Doppler effect is an effective tool for diagnosis of vascular problems like stenosis.
Flow measurement
Instruments such as the
laser Doppler velocimeter (LDV), and
Acoustic Doppler Velocimeter (ADV) have been developed to measure
velocities in a fluid flow. The LDV emits a light beam and the ADV emits an ultrasonic acoustic burst, and measure the Doppler shift in wavelengths of reflections from particles moving with the flow. The actual flow is computed as a function of the water velocity and face. This technique allows non-intrusive flow measurements, at high precision and high frequency.
Velocity profile measurement
Developed originally for velocity measurements in medical applications (blood flows), Ultrasonic Doppler Velocimetry (UDV) can measure in real time complete velocity profile in almost any liquids containing particles in suspension such as dust, gas bubbles, emulsions. Flows can be pulsating, oscillating, laminar or turbulent, stationary or transient. This technique is fully non-invasive.
Underwater acoustics
In military applications the Doppler shift of a target is used to ascertain the speed of a
submarine using both passive and active
sonar systems. As a submarine passes by a passive
sonobuoy, the stable frequencies undergo a Doppler shift, and the speed and range from the sonobuoy can be calculated. If the sonar system is mounted on a moving ship or another submarine, then the relative
velocity can be calculated.
Audio
The
Leslie speaker, associated with and predominantly used with the
Hammond B-3 Organ, takes advantage of the Doppler Effect by using an
electric motor to rotate a speaker continuously, rapidly alternating the received frequency of a keyboard note.
See also
Further reading
- "Doppler and the Doppler effect", E. N. da C. Andrade, Endeavour Vol. XVIII No. 69, January 1959 (published by ICI London). Historical account of Doppler's original paper and subsequent developments.
External links
- , ScienceWorld
-
- at MathPages
-
-
- - Doppler flow meters with engineering examples and applications
- from John de Pillis. An animation showing that the speed of a moving wave source does not affect the speed of the wave.
- from John de Pillis. How an electromagnetic wave propagates through a vacuum
- - Ultrasonic Doppler Velocimeters for real time measurement of velocity profiles in liquids
- - Interactive flash simulation for demonstrating Doppler shift.
- Excellent interactive applet, go to applet thumbnails>upcoming applets.