phys 307 sound and music
TRANSCRIPT
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Pa e 1Bisho - S rin 2013 PHYS/MHIS 307 Notes: Waves and Sound Ch. 2
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Pa e 2Bisho - S rin 2013 PHYS/MHIS 307 Notes: Waves and Sound Ch. 2
Wave Basics: Transverse and Longitudinal
compression rarefaction
Transverse
(rope)
Longitudinal
(Slinky, sound)
Wave = Disturbance that propagates with a velocity v (l/T)dependent
on the material through which it travels
propagation
oscillation
oscillation
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Pa e 3Bisho - S rin 2013 PHYS/MHIS 307 Notes: Waves and Sound Ch. 2
Wave Basics: Inverse Square Law
3-D Sphere2-D Circle
Power spread over circumference Power spread over area
*Laser light is different due to coherency and collimation
2p r 4p r2
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Pa e 4Bisho - S rin 2013 PHYS/MHIS 307 Notes: Waves and Sound Ch. 2
Wavelets: Huygens Principle
Wave Fronts
Circular Wave
Wave Sources
Plane WaveAll points = source
of circular (orspherical waves)
http://www.falstad.com/ripple/ Setup: Single Slit; 1 Plane Src, 1 Freq
http://www.falstad.com/ripple/http://www.falstad.com/ripple/ -
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Pa e 5Bisho - S rin 2013 PHYS/MHIS 307 Notes: Waves and Sound Ch. 2
Superposition of Wavelets
Two sources
Longerl Lowerf
FOR DEMONSTRATION,
http://www.falstad.com/ripple/ Setup: Two sources; 2 Src, 1 Freq.
Two sources
Shorterl Higherf Five sources
To find resultant pattern, add waves algebraically.
http://www.falstad.com/ripple/http://www.falstad.com/ripple/ -
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Pa e 6Bisho - S rin 2013 PHYS/MHIS 307 Notes: Waves and Sound Ch. 2
Superposition: Same frequency, different phases
FOR DEMONSTRATION, we will do this in Mathematica. You can also
try Example 3 on the web site:
http://webphysics.davidson.edu/Applets/superposition/default.html
In Phase: 0 Out of Phase: 180
f(x,t) = 2.5 * sin[8 *(x - t) - pi]
f(x,t) = 2.5 *sin[8 * (x - t)]f(x,t) = 2.5 * sin[8 *(x - t)]
f(x,t) = 2.5 *sin[8 * (x - t)]
f(x, t) +g(x,t) f(x,t) +g(x,t)
http://webphysics.davidson.edu/Applets/superposition/default.htmlhttp://webphysics.davidson.edu/Applets/superposition/default.html -
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Pa e 7Bisho - S rin 2013 PHYS/MHIS 307 Notes: Waves and Sound Ch. 2
Superposition: Different frequencies and phases
FOR DEMONSTRATION, we will do this in Mathematica, or try the site:
http://webphysics.davidson.edu/Applets/superposition/default.html
(Example 3)
l1
l2
l1=1
2l2
or f1=2f
2
http://webphysics.davidson.edu/Applets/superposition/default.htmlhttp://webphysics.davidson.edu/Applets/superposition/default.html -
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Pa e 8Bisho - S rin 2013 PHYS/MHIS 307 Notes: Waves and Sound Ch. 2
Superposition: Similar frequencies give BEATS
f1
f2= 1.1f1
Slower Beat Frequency
f1
f2 = 1.2 f1
Faster Beat Frequency
ftone = (f1 +f2 )/2
fbeat = f2f1
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Pa e 9Bisho - S rin 2013 PHYS/MHIS 307 Notes: Waves and Sound Ch. 2
Reflection & Refraction: Ray Diagram
Reflection Refraction
Angle is smaller forslower velocity.
http://lectureonline.cl.msu.edu/
~mmp/kap13/cd372.htm for an
animated explanation
http://lectureonline.cl.msu.edu/~mmp/kap13/cd372.htmhttp://lectureonline.cl.msu.edu/~mmp/kap13/cd372.htmhttp://lectureonline.cl.msu.edu/~mmp/kap13/cd372.htmhttp://lectureonline.cl.msu.edu/~mmp/kap13/cd372.htm -
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Pa e 10Bisho - S rin 2013 PHYS/MHIS 307 Notes: Waves and Sound Ch. 2
Reflection: Concave Mirror
Light Source
far from Mirror
Light Sourceat Focus
Light Sourcenear to Mirror
http://webphysics.davidson.ed
u/physlet_resources/optics4/de
fault.html
http://webphysics.davidson.edu/physlet_resources/optics4/default.htmlhttp://webphysics.davidson.edu/physlet_resources/optics4/default.htmlhttp://webphysics.davidson.edu/physlet_resources/optics4/default.htmlhttp://webphysics.davidson.edu/physlet_resources/optics4/default.htmlhttp://webphysics.davidson.edu/physlet_resources/optics4/default.htmlhttp://webphysics.davidson.edu/physlet_resources/optics4/default.html -
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Refraction: Bending of Light due to Speed Change
Slower
Faster
Marching Band Analogy
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12/17Pa e 12Bisho - S rin 2013 PHYS/MHIS 307 Notes: Waves and Sound Ch. 2
Refraction: Explanation of Sound Travel at Night
Slower
Faster
http://www.falstad.com/ripple/index.html
Setup: Temperature Gradient 1, 1 Src, 1 Freq., Source in lower left corner
http://www.falstad.com/ripple/index.htmlhttp://www.falstad.com/ripple/index.html -
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13/17Pa e 13Bisho - S rin 2013 PHYS/MHIS 307 Notes: Waves and Sound Ch. 2
http://www.falstad.com/ripple/index.html
Setup: Temperature Gradient 1, 1 Src, 1 Freq., Source in lower left corner
Sound Travel at Night Applet Lower is Cooler
Sound Travels slower at lower temperatures
http://www.falstad.com/ripple/index.htmlhttp://www.falstad.com/ripple/index.html -
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Diffraction: Bending of Light without Speed Change
http://dev.physicslab.org/asp/applets/javaphysmath/java/slitdiffr/default.asp
Local file
http://dev.physicslab.org/asp/applets/javaphysmath/java/slitdiffr/default.asphttp://dev.physicslab.org/asp/applets/javaphysmath/java/slitdiffr/default.asphttp://dev.physicslab.org/asp/applets/javaphysmath/java/slitdiffr/default.asphttp://dev.physicslab.org/asp/applets/javaphysmath/java/slitdiffr/default.asp -
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Doppler Effect
FOR DEMONSTRATION,
http://ephysics.physics.ucla.edu/physlets/edoppler_shift.htm
Velocity = 1/2 of Sound Speed
http://ephysics.physics.ucla.edu/physlets/edoppler_shift.htmhttp://ephysics.physics.ucla.edu/physlets/edoppler_shift.htm -
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http://lectureonline.cl.msu.edu/~mmp/applist/doppler/d.htmThis site has an applet that is even easier to use.
http://lectureonline.cl.msu.edu/~mmp/applist/doppler/d.htmhttp://lectureonline.cl.msu.edu/~mmp/applist/doppler/d.htm -
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Shock Wave
FOR DEMONSTRATION,
http://ephysics.physics.ucla.edu/physlets/edoppler_shift.htm
Velocity = 3/2 of Sound Speed
http://ephysics.physics.ucla.edu/physlets/edoppler_shift.htmhttp://ephysics.physics.ucla.edu/physlets/edoppler_shift.htm