Spectroscopy Using the Michelson Interferometer

March 20, 1998

Ben Kinnaman,Davidson College

Ansel Singer-Barnum, Davidson College


Abstract

The purpose of this experiment was to experimentally determine the two dominant wavelengths present in a sodium light using the Michelson Interferometer. The michelson Interferometer uses a beam splitter to split an input wave into two waves which are reflected and combined again so that an interference pattern of minimum and maximum intensities is observable. The path length of one of the waves is changed by moving one mirror. This changing path length creates a changing interference pattern. The wavelength is related to the frequency of the changes in intensity and the velocity of the mirror by the expression l = 2*v/f. Using this expression, we computationally simulated the data to find the two primary wavelengths present in a Na lamp and their relative intensities. Our data is consistant with the known wavelengths for sodium.


Theory

Below is the Michelson interferometer. Light entering the interferometer is split by the beam splitter. The beam splitter is a semi-reflective mirror allowing some light to pass directly through the splitter to the stationary mirror. The rest of the light is reflected to the moveable mirror. The light is then reflected back to the splitter where, again some light is allowed to pass from the moveable mirror to the ditector and some light from the stationary mirror is reflected to the detector. These two waves of light from the stationary and movable mirrors combine at the splitter. This combination is what the detector detects. (It should be noted however, that this is a simplified view of what is really happening. We are ignoring internal reflection and the spreading of the wave. we have discussed what was important to this experiment.)

When these two waves of light combine, they interfere constructively or destructively, depending on the path lengths traveled by each wave. The path lengths traveled by each wave will affects the relative phase of the two waves, so that when they combine, they will combine contructively or destructively. The images below illustrate constructive and destructive interference with the red and blue waves being the descrete waves and the purple wave representing the combination of the two.

 

The moving mirror on the interferometer is driven at a constant rate by the motor shown. We found that the mirror moved about 1666.4 nm/s (the process of finding this velocity will be discussed later). As the mirror moves, the path length of the light wave reflected off of that mirror changes. this changing path length produces a changing interference pattern that is visible. The interference pattern forms a series of bright and dark concentric circles, similar to what is illustrated below. As the mirror moves, the fringes move to or from the center of the circle.

The path length of the wave is equal to an integral number of half wavelengths, or x = n*[l/2]. By taking the time-derivative of this equation, we can derive a fringe frequency and mirror velocity dependence: v = f *[l/2]. The velocity of the mirror is related to the frequency of the fringe procession through the expression v = f *[l/2], or, velocity is equal to the fringe frequency multiplied by the number of half wavelengths. Using this relation, if the frequency and velocity are known, we can find the wavelength of the light entering the interferometer. If the light has more than one wavelength, a frequency of the intensity of the fringes emerges. This is due to one wave processing faster than the other, resulting in periods of high intensity and periods of low intensity. This forms what is known as beats, or a beat frequency. the images below illustrate a monofrequency wave and a beat wave. The beat wave, on the right, is the sum of two frequencies 0.8HZ different.

Knowing the frequency with which the beats occur, we could know the wavelengths present in the wave.


Procedure

The purpose of this experiment was to experimentally determine the two dominant wavelengths present in a sodium light using the Michelson Interferometer. We know that the frequency of the constructive and destructive interference of the waves of light emitted from the Michelson Interferometer is related to the wavelength of the light and the rate at which the path distance of one of the waves changes (the velocity with which the mirror moves). This relationship is simply v = f*[l/2]. Because the motor turning the screw which in turn, moves the mirror is moving the mirror very slowly, it would be very inaccurate, if not impossible to measure the velocity of the mirror mechanically. By using the above equation with a light emitting a known wave length, we very easily calculated the velocity of the mirror.

In order to determine the frequency of the fringe pattern we recorded the intensity of the light going into the detector as a function of time, the data is in volts per unit of time. Next we found the frequency of the bright fringes, constructive interference, by counting how many fringes passed per unit time. The graphical data is available.

We used a HeNe laser with a known wavelength of 632.8 nm. We took two data sets with this laser, finding the fringe frequency to be 5.2631 fringes/sec. Thus, our moved with a velocity of 1666.4 mm/sec. We used this velocity to find the dominant wavelengths present in sodium light.

Setting up the appartus for the sodium light required great care in order to have the highest intensity of light possible going into the detector, with as little periphial light going in as possible. in order to do this we had to set up two aperatures. Each was about a 1/4 in. hole that when set up successively, focused the light so that as narrow of a beam was traveling in the interferometer. The light was weak enough to require a 500V detector voltage.

After the apparatus was set up and we were sure the sharpest signal was being received as possible we could begin taking and analyzing data, which we did in the following manner:

*We know that two waves are combining in this experiment. A fundamental way to model this is [A*sin(2*p*f*t)+A1*sin(2*p*f1*t)]. This is simply the addition of two waves with different frequencies. We set f equal to the experimental frequency and let f1 vary until the plot of this function duplicated the experimental data set. the next step was to vary A and A1 until the intensity of the simulated plot matched the data.


Data and Results

Below is a data set showing the intensity, or fringes, as a function of time.

Light Intensity as a Function of time for a Na Lamp (small scale)

This data was taken during a period of greatest intensity. A large scale sample of the data clearly shows the beat pattern of the intensity due to constructive and destructive interference patterns.

Light Intensity as a Function of time for a Na Lamp (large scale)

The section indicated above is the region that the data for the fringe frequency was taken.

We found the frequency of the fringes to be 5.749 fringes/sec. And found the beats to have a period of about 178.1717 sec. Notice on the large scale intensity plot that at during the period of smallest Intensity, the beginning and end of the beats, there is still some intensity. It does not go al the way to zero. This is because the combining waves do not have equal intensities. One wave and its associated wavelength has a greater intensity than the other wave and its associated wavelength. The relative intensities are important in modeling the data.

Our simulated data is shown below.


Simulated Light Intensity as a Function of time for a Na Lamp (large scale)

We were able to match the period of the beats exactly, our indication that we had the correct relative frequecies. We adjusted the intensities of each wave to match the relatve minimums and maximums with the data. We found the maximum and the minimum of the beats to have a relationship of 1.6:1. This is the relative intensities of the waves and their corresponding wavelengths. Using this data we found the primary wavelengths of the Na lamp to be 579.674 nm, and 580.23 nm.

Zooming in on our simulated data, we can very clearly se the contructve interference occurring at the minimums and the constructive interference occurring at the maximums. the two plots below were taken out of our simulated plot and show the discrete waves at the first minimum and second maximum (notice the t scale). The relative intensities of the waves and their phases at the minimums and maximums are obvious. The red series is the lower intensity while the blue series is the higher intensity. (Note: the red series in the above plot does not indicate the same series in the lower two.)

 


Conclusions

We were able to find the two primary wavelengths of the sodium lamp. Our findings were consistent with the known values.

Na Wavelength Experimental Accepted % Error
Wavelength 1 580.230 nm 589.592 nm 1.58 %
Wavelength 2 579.674 nm 588.995 nm 1.61 %

We also found the relative intensity between the two wavelengths to be 1.6:1.

What is more relevant than the absolute wavelengths that we found is the difference between the wavelengths. There is a scaling error in our simulated data, which is introduced by making the frequency of the superposition of the two discrete waves a constant. It is impossible to detect the two discrete waves with the Michelson Interferometer so we had to use the frequecy of the combined wave. Because of this scaling error, we would not expect our calculations to yield the known wavelengths exactly. We could expect the difference between the two experimental wavelengths to be the same as the difference between the known wavelengths.

  Experimental Accepted % Error
D l 0.556 nm 0.597 nm 6.86 %

There was plenty of room for error in this experiment that could explain the large error. The mechanical turning mechanism was suspected of not having totally constant velocity, since all of our data is based on the experimental frequency of the fringes, this could have been quite significant. Extraneous light entering the detector could have also been a source of error.