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Precision Interferometer

012-07137B

14

®

4.

Be sure that the air in the vacuum cell is at atmospheric pressure.  If you are using the OS-8502 Hand-
Held Vacuum Pump, this is accomplished by flipping the vacuum release toggle switch.

5.

Record 

P

i

, the initial reading on the vacuum pump gauge. Slowly pump out the air in the vacuum cell. As

you do this, count 

N

, the number of fringe transitions that occur. When you're done, record 

N

 and also

P

f

, the final reading on the vacuum gauge.  (Some people prefer to begin with the vacuum cell evacuated,

then count fringes as they let the air slowly out. Use whichever method is easier for you.)

   NOTE:

  Most vacuum gauges measure pressure with respect to atmospheric pressure (i.e., 34 cm Hg

means that the pressure is 34 cm Hg below atmospheric pressure, which is 

~

 76 cm Hg).  The actual

pressure inside the cell is:

P

absolute

 = P

atmospheric

 – P

gauge

Analyzing Your Data

As the laser beam passes back and forth between the beam-splitter and the movable mirror, it passes
twice through the vacuum cell.  Outside the cell the optical path lengths of the two interferometer beams
do not change throughout the experiment.  Inside the cell, however, the wavelength of the light gets longer
as the pressure is reduced.

Suppose that originally the cell length, 

d

, was 10 wavelengths long (of course, it's much longer).  As you

pump out the cell, the wavelength increases until, at some point, the cell is only 9-1/2 wavelengths long.
Since the laser beam passes twice through the cell, the light now goes through one less oscillation within
the cell.  This has the same effect on the interference pattern as when the movable mirror is moved
toward the beam-splitter by 1/2 wavelength.  A single fringe transition will have occurred.

Originally there are 

N

i

 = 2

d

/

λλλλλ

i

 wavelengths of light within the cell (counting both passes of the laser

beam).  At the final pressure there are 

N

f

 = 2

d

/

λλλλλ

f

 wavelengths within the cell.  The difference between

these values, 

N

i

 – N

f

 , is just 

N

, the number of fringes you counted as you evacuated the cell.  Therefore:

N

 = 2

d

/

λλλλλ

i

 - 2

d

/

λλλλλ

f

.

However, 

λλλλλ

i

 = 

λλλλλ

0

/

n

i

 and 

λλλλλ

f

 = 

λλλλλ

0

/

n

f

; where 

n

i

 and 

n

f

 are the initial and final values for the index of

refraction of the air inside the cell.  Therefore 

N

 = 2

d

(

n

i

 – 

n

f

) /

λλλλλ

0

; so that 

n

i

 – 

n

f

 = 

N

λλλλλ

0

/2d.  The slope of

the n vs pressure graph is therefore:

where 

P

i

 = the initial air pressure; 

P

f

 = the final air pressure; 

n

i

 = the index of refraction of air at pressure

P

i

; n

f

 = the index of refraction of air at pressure 

P

f

 

; N

 = the number of fringe transitions counted during

evacuation; 

λλλλλ

0

 = the wavelength of the laser light in vacuum (see your instructor);

d

 = the length of the vacuum cell (3.0 cm).

1.

Calculate the slope of the n vs pressure graph for air.

2.

On a separate piece of paper, draw the n vs pressure graph.

Questions

1.

From your graph, what is 

n

atm

, the index of refraction for air at a pressure of 1 atmosphere (76 cm Hg).

2.

In this experiment, a linear relationship between pressure and index of refraction was assumed.  How
might you test that assumption?

3.

The index of refraction for a gas depends on temperature as well as pressure.  Describe an experiment
that would determine the temperature dependence of the index of refraction for air.

n i – nf

Pi – Pf

=

N

λ

0

2d(Pi – Pf)

Summary of Contents for OS-9255A

Page 1: ...Instruction Manual and Experiment Guide for the PASCO scientific Models OS 9255A thru OS 9258A 012 07137B PRECISION INTERFEROMETER Includes Teacher s Notes and Typical Experiment Results...

Page 2: ...ion 4 Michelson Twyman Green Fabry Perot Setup and Operation 6 Tips on Using the Interferometer 9 Sources of Error Troubleshooting Experiments Experiment1 IntroductiontoInterferometry 11 Experiment 2...

Page 3: ...ghted and all rights reserved However permission is granted to non profit educational institutions for reproduction of any part of the manual providing the reproductions are used only for their labora...

Page 4: ...vide asimpleintroductiontothisimportantapplicationof interferometry Fabry Perot The Fabry Perot Interferometer is also an important contemporary tool used most often for high resolution spectrometry T...

Page 5: ...Ocatalogfordetails Additional Equipment Recommended TheOS 9256AInterferometerAccessoriesincludes RotatingPointer VacuumCell ComponentHolder Lens 18 mm Focal Length Lens 48 mm Focal Length GlassPlate 2...

Page 6: ...r Movable Mirror Adjustable Mirror Vacuum Cell Vacuum Pump withGauge Rotating Pointer Beam Splitter Compensator Plate Component Holder OS 9255A Precision Interferometer Lens 18 mm Fitted Case 2 Polari...

Page 7: ...m the two slits struck the screen a regular pattern of dark and bright bands appeared When firstperformed Young sexperimentofferedimportant evidence for the wave nature of light Young s slits can be u...

Page 8: ...he mirror a measured distance dm and counting m the number of times the fringe pattern is restoredtoitsoriginalstate thewavelengthofthelight canbecalculatedas 2dm m If the wavelength of the light is k...

Page 9: ...aser see Suggestions for Additional Experiments near the end of the manual To set up and align your PASCO Laser 1 Set the interferometer base on a lab table with the mi crometerknobpointingtowardyou 2...

Page 10: ...ks so that the beam is reflected to the fixed mirror Adjust the angle of the beam splitter as needed so that the reflected beam hits the fixed mirror near its center 4 There should now be two sets of...

Page 11: ...t s at least 12 inches from the edge of the interferometerbase Fringesshouldappearinthebright disk of the viewing screen Fine adjustments of L1 may be necessary to find the fringes A piece of white pa...

Page 12: ...he diffuser rather than on the viewing screen Just place the diffuser where you would normally place the viewing screen and look through it toward the interferometer Tips on Using the Interferometer F...

Page 13: ...nd back surfaces of the mirrors and beam splitter of ten cause minor interference patterns in the back ground of the main fringe pattern These background patterns normally do not move when the mirror...

Page 14: ...rferometerintheMichelsonmode soaninterferencepatternisclearlyvisibleonyour viewing screen See Setup and Operation for instructions 2 Adjustthemicrometerknobtoamediumreading approximately50 m Inthispos...

Page 15: ...ht 2dm N then average your results If you tried the Fabry Perot mode also calculate the wavelength independently for that data The same formula applies PartII 1 From your observations in step 1 of the...

Page 16: ...exactly 1 A graph of index of refraction versus pressure for a gas is shown in Figure2 1 Byexperimentallydeterminingtheslope the index of refraction of air can be determined at various pressures Proce...

Page 17: ...helightnowgoesthroughonelessoscillationwithin the cell This has the same effect on the interference pattern as when the movable mirror is moved towardthebeam splitterby1 2wavelength Asinglefringetrans...

Page 18: ...2 Placetherotatingtablebetweenthebeam splitter and movable mirror perpendicular to the optical path NOTE if the movable mirror is too far forward the rotating table won t fit You may need to loosen t...

Page 19: ...ction of air see Experiment 2 ng the index of refraction of the glass plate as yet unknown 0 the wavelength of your light source in vacuum and N the number of fringetransitionsthatyoucounted Carrying...

Page 20: ...pticalimperfections Thenremovetheviewing screenandreplacethelaserwiththespectrallight source Iffringesaren tvisiblewhenlookingintothe beam splitter proceedasfollows a Tape two thin pieces of wire or t...

Page 21: ...ate the Micrometer Knob fully IN before storing the Interferometer MicrometerCalibration The micrometer is calibrated before it is shipped How ever ifrecalibrationbecomesnecessary usethefollowing proc...

Page 22: ...03956 MovableMirror 003 03955 ComponentHolder 003 05161 Compensator 003 03958 InterferometerManual 012 05187 VacuumPump OS 8502 Component Part No VacuumCell 003 05162 RotationalPointer 003 05160 Fitt...

Page 23: ...imitingfactorsareplayinthesystemanduncertainty inourmicrometerposition 6 Losingcountoffringes andinexactpositioningofthe fringes relative to our reference mark 7 In order to interfere the two light be...

Page 24: ...e vacuum first then count the fringes as the vacuum was released The average slope starting at a guage reading of 60 was 3 462x10 6 0 9995 0 9996 0 9997 0 9998 0 9999 1 1 0001 1 0002 1 0003 1 0004 1 0...

Page 25: ...drews Prentice Hall 1960 is Thesecondtermisnegligibleforvisiblewavelengths and may be ignored Notes General It is often difficult to count large numbers of fringes due to eyestrain If you find this to...

Page 26: ...com web www pasco com Contacting Technical Support Before you call the PASCO Technical Support staff it wouldbehelpfultopreparethefollowinginformation If your problem is with the PASCO apparatus note...

Page 27: ...PrecisionInterferometer 012 07137B 24...

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