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Beats and Doppler Chapter 17

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Title: Beats and Doppler Chapter 17


1
Beats and Doppler Chapter 17 18
  • PHYS 2326-28

2
Concepts to Know
  • Beats
  • Doppler Effect
  • Sign Convention

3
Beats
  • Listening to a band or orchestra of relative
    beginners, youll notice the problem that the
    music just doesnt sound good. If you even
    listen to two people playing the same thing it
    could sound bad as well.
  • Quite often this is due to tuning of the musical
    instruments. If one is at a different pitch from
    the other there is a beat that may be fairly low
    to very high speed.

4
Beats
  • This beating ruins the effect of the music.
  • It is caused by the instruments playing at
    slightly different pitches and the intensity
    changes with time rather than with space.
  • Beating is the periodic variation in amplitude
    caused by the superposition of two waves of
    slightly different frequencies
  • The frequency of the beat equals the difference
    in frequency of the two sources

5
Beats
  • Section 18.7 shows that given two wave functions
    of different frequencies can be superimposed
    using a trigonometric identity cos a cos b 2
    cos((a-b)/2)cos((ab)/2)
  • The superposition gives y 2a cos (2pi
    ((f1-f2)/2)t) cos(2pi((f1f2)/2)t) eqn 18.10
  • This shows there is an average frequency that is
    beating at the difference frequency.

6
Beats
  • The envelope that beats becomes
  • 2Acos(2 pi ((f1-f2)/2)t)
  • the beat frequency (f1-f2) since cosine goes to
    zero twice every 2pi radians

7
An Interesting Effect
  • Since this qualifies regardless of the actual
    frequencies and differences, one can achieve a
    fascinating musical effect under some conditions.
    Given 2 flutists playing a duet, music can (and
    has) been written that makes use of these sum and
    difference of frequencies so that rather than a
    irritating beat due to poor tuning, one can
    achieve what sounds like 3 or 4 instruments
    playing different notes played at one time with
    even a different melody line

8
Doppler Effect
  • So far, weve dealt with observing waves emitted
    from and observed from positions at rest
  • We know that the waves travel at a speed relative
    to the medium
  • What happens if the transmitter and / or the
    receiver are traveling relative to the medium?
  • Weve all heard train and car horns shift
    frequency as they travel past us

9
Moving Observer
  • Eqns 17.9 and 17.10 show what happens to the
    frequency if an observer moves relative to the
    medium. Since vf ?
  • f v/? and for a moving observer fv/ ?
    (vvo)/ ? where v is the velocity of the wave and
    vo is the velocity of the observer
  • f ((vvo)/v) f moving towards the source and
    f ((v-vo)/v) f moving away from the source

10
Moving Source
  • When a source moves, it moves a distance vsT
    during each period vs/f and the wavelength is
    shortened to ? ?-?? ?- vs/f
  • The observer hears f v/ ? v/(v/f - vs/f)
  • f (v/(v vs)) f source moving towards
    observer and
  • f (v/(v vs)) f for the source moving away

11
Sound Wave Doppler
  • The general equation becomes eqn 17.13
  • f ((vvo)/(v-vs))f
  • SIGNS these signs are for the observer or
    source moving towards the other and for the case
    where one is moving away from the other the
    appropriate sign is reversed.

12
For Electromagnetic Waves
  • fr sqrt((c-v)/(cv)) fs
  • where c is the speed of light and v the velocity
    difference between transmitter and receiver.
    This is the relativistic equation and cannot
    distinguish between which is in motion wrt the
    medium or even if there is a medium.

13
Example 1
  • A car traveling at 20m/s blows its horn, f300Hz
    as it passes a second car at rest. If the speed
    of sound is 345m/s, find a) the frequency heard
    in the second car before it passes, b) the
    frequency heard after it passes, c) the
    wavelength ahead of the car, d) the wavelength
    behind the first car, e) If the second car blows
    its horn after the first passes, what is the beat
    frequency heard by those in the second car, f) by
    those in the first car?

14
Example 1
  • a) observer at rest vo0,f ((vvo)/(v-vs))f
  • f ((3450)/(345-20))300 318.5Hz
  • b) f((3450)/(345-(-20)) 345/365 284.4Hz
  • c) wavelength v/f 345/317.5 1.083m
  • d) wavelength v/f 345/284.4 1.213m
  • e) fbeat fa-fb 300Hz-284.4Hz 15.6Hz
  • f) f ((345(-20))/(3450) 282.6Hz
  • f-f 300 282.6 17.4Hz

15
Example 2
  • Student skating at 3m/s towards a wall, blows a
    500Hz whistle at 100m from the wall and times the
    echo. a) How far does he travel before hearing
    the echo, b) what is the echo frequency? c) what
    is the beat frequency with the whistle? assume
    v345m/s

16
Example 2
  • in time t, sound travels vt and skater travels
    v2t. The distance traveled by the sound is D D-
    v2t since the skater is that much closer to the
    wall when the sound returns. hence 2D v2t vt
    2(100) 345t 3t 348t, t 0.5745 s
  • x vt 3 0.5745 1.72m
  • b) f ((vvo)/(v-vs))f ((3450)/(345-3))500
    504.4 Hz heard by the wall and reflected
  • For the skater f((3453)/(3450))504.4 508.8
    Hz
  • c) fbeat fa-fb 508.8-500 8.8 Hz

17
Example 3
  • Hydrogen gas emits spectral lines in the visible
    in what is called the Balmer series. The first
    two are the H-alpha 656.1nm (nice and red) and
    H-beta 486.1nm (bluish green). a) how fast is a
    galaxy moving away from us if its beta line is
    shifted all the way to the alpha wavelength b)
    what is the fractional change what is the
    fractional change in wavelength if the star is
    moving away from us at 0.5c, c) what is the
    observed shift in the alpha line for a star
    moving towards the earth at a speed equal to that
    of the earth around the sun orbital radius
    1.5E11m

18
Example 3
  • source wavelength 4.861E-7, cfs?s
  • received wavelength 6.563E-7, cfr ?r
  • fr sqrt((c-v)/(cv))fs, fr/fs
    sqrt((c-v)/(cv)) ?s/ ?r, square both sides
  • (?s/ ?r)2 (c-v)/(cv), solving for v
  • v (1-(?s/ ?r)2)c/(1 (?s/ ?r)2) 0.291c

19
  • b) v 0.5c, fr sqrt((c-v)/(cv))fs
  • fs/fr sqrt((cv)/(c-v)) ?r/?s
    sqrt(1.5c/0.5c) 1.732
  • fractional change in wavelength ??/? ?r/?s-1
    0.732
  • c) t 1 year 3.156E7 sec
  • ?s 6.563E-7 s, 2pi r vt,
  • v2pi r/t 29863 m/s
  • ??/?s sqrt ((c-v)/(cv)) 1, multiply sqrt by
    c-v and
  • get sqrt((c-v)2/(c2-v2)) and v2 ltltc2 so
    result
  • is (c-v)/(c) 1-v/c 1v/c 29863/3.0E8
    9.96E-5
  • ?? (v/c) ?s
  • ?? 9.96 E-5 6.563E-7 6.531E-11 m

20
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