Pasco Scientific OS-9255A Instruction Manual Download Page 13

Precision Interferometer

012-07137B

10

®

Sources of Experimental Error

Backlash—

 Although PASCO's  carefully designed mirror

movement reduces backlash considerably, every mechani-
cal system is susceptible to backlash. However, the effects
of backlash can be practically eliminated by using proper
technique when counting fringes (see item 3 under Accu-
rate Fringe-Counting, on the previous page).

Mirror Travel—

 The amount of mirror movement per

dial turn of the micrometer is constant to within 1.5%.
Most of this error occurs at the extreme ends of the
mirror’s total possible movement. For very accurate
measurements, see 

Calibrating the Micrometer

, above,

and remember that the mirrors are flat to within 1/4
wavelength across their surface.

Troubleshooting

If you have trouble producing  a clear set of interference
fringes, consider the following possible sources of diffi-
culty:

1.

Warm up your Laser—

 Many lasers vary in intensity

and/or polarization as they warm up.  To eliminate any
possible fringe or intensity variations, allow the laser to
warm up prior to setting up an experiment.  (The
PASCO laser should warm up in about 1 hour.)

2.

Check your Mirrors—

 The beam-splitter and

movable mirror are carefully mounted in their brackets
to remain perpendicular to the interferometer base
when set up.  If the brackets are bent slightly out of
alignment, the resulting fringe patterns will be distorted
somewhat. If they are significantly out of alignment, it
may be impossible to obtain fringes.

3.

Background Fringes—

 Reflections from the front

and 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 is
moved, and have no impact on measurements made
using the main interference pattern.

4.

Convection Currents—

 If the fringe pattern ap-

pears to wave or vibrate, check for air currents. Even
a slight breeze can effect the fringes.

5.

Vibration—

 Under normal conditions, the

interferometer base and mirror mounts are stable
enough to provide a vibration free setup.  However, if
the experiment table is vibrating sufficiently, it will
effect the interference pattern.

IMPORTANT:

  If the movable mirror doesn't

move when you turn the micrometer dial, see

Micrometer Spacer Replacement

 in the

Maintenance

 section at the end of this manual.

Component Specifications

Interferometer Mirrors—

 3.175 cm in diameter;

0.635 + 0.012 cm thick; flat to 1/4 wavelength on both
sides; coated on one side for 80% reflectance and 20%
transmission.

Beam-Splitter—

 3.175 cm in diameter; 0.635 + 0.012 cm

thick; flat to 1/4 wavelength on both sides; coated on one
side for 50% reflectance and 50% transmission.

Compensator—

 Identical to the beam-splitter, but

uncoated.

Movable Mirror

— movement is controlled by the

micrometer that is built-into the interferometer base;
turning the dial clockwise moves the mirror toward the
right (looking from the micrometer side); 25 microns per
micrometer dial revolution (±1% near center of move-
ment); movement through full distance of travel is linear to
within 1.5%.

IMPORTANT:

  Avoid touching all mirror surfaces.

Minute scratches and dirt can impair the clarity of
interference images. See the 

Maintenance

 section at

the end of this manual for cleaning instructions.

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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