Single Mode Optical Fiber

Sarah Campbell
SUNY Stony Brook
Optics Rotation Project 2, Fall 2002

Advisor: Dr. John Noe



Project Goal

In this project, I hope to measure the far field radiation of a single mode step index optical fiber to a high degree of precision, with an angular precision of half a degree and intensity precision of 10^-12 Watts. These measurements are important because fiber optics are used in a variety of communication applications and these additional modes could cause anomalies in the fiber's output, especially when the fibers are bundled together.


Far-Field Radiation

The goal of this project is to study the far field radiation of a single mode step index optical fiber. Studying the far field radiation means studying the light intensity profile of the beam from the fiber far away from the fiber, a distance of around 10 inches. This profile is expected to have a gaussian distribution about the center of the beam. However, additional modes or fringes are expected. These fringes are rings of light around the bright spot of the beam. These modes are the result of interference because the end of the fiber optic acts as an aperature. Below is a picture of the fiber optic output. In this picture the first fringe, a red ring is visible. The center of the beam is blocked inorder to prevent the center of the beam from washing out the first fringe. This picture was taken by John Noe.


The far field radiation can be shown graphically by looking at a intensity versus angular position graph. A very nice graph of the far-field radiation is shown as an example in the image below.


Experimental Set Up

Two lasers, a metrologia Helium-Neon laser (shown above) and a Helium-Neon from Meredith Instruments, both at 633nm, were directed into the fiber during the course of this experiment. The alignment of the laser light into the fiber is aided by 2 mirrors and the PAF fiber port. The light travels through the fiber (yellow) from the right side of the picture to the output end of the cable on the left side of the picture. A dectector (silver with black cord) measures the intensity of the light once is has past through a slit (not shown), 1.25 inches in front of the dectector. The dectector is on a black metal arm of length, 10.625 inches. This arm pivots at the end of the fiber allowing the dectector to cover an angular range of around 25 degrees on each side. A white grid is taped to the table under the arm, to allow angular measurements. The grid has 20 boxes per inch and the slit with a width of 1mm allow an angular precision of less than half a degree.

The detector produces an current proportional to the intensity of light. This current passes through a resistor and the voltage is read off of a multimeter. The voltage measurements consist of the average voltage reading over a minute of measurement.


Fiber Optics

A fiber optics is a transmission channel that carries a beam of light. A fiber optic consists of a glass, plastic or silica core surrounded by cladding. Cladding is an outer covering with a lower index of refraction than the core. Fiber optics transmit light via total internal reflection. The light inside of the fiber optic completely reflects off of the cladding and back into the core. The light then travels down the fiber by bouncing off thecladding until it reaches the end of the fiber. The benefit of an optical fiber is that it can bend and travel fairly long distances without losing energy or distorting the light. A diagram of total internal reflection in a fiber optic is shown in the picture below.

The physics of total internal reflection will be presented shortly, but it relies on a boundary, such as the core-cladding boundary, where the initial material, the core, has a higher index of refraction than the second material, the cladding. Without this boundary total internal reflection would not occur. A nice animation of the difference between total internal reflection and regular reflection and transmission can be seen at the Schott website. Just click on "click here for flash animation" after clicking the link below.

http://www.us.shott.com/fiberoptics/english/allaboutfiberoptics.html

For this experiment, I used a step index single mode optical fiber. Step index means that the optical fiber has a constant index of refraction in the inner core and a different constant index of refraction in the outer core. This is in contrast to other types of optical fibers that have gradations in the index of refraction of the core.

A single mode optical fiber means that only one mode of light can propagate in the optical fiber. In contrast, a mulitmode optical fiber allows several modes to propagate. A single mode fiber is able to prevent other modes from propagating by operating above the cutoff frequency, thus cutting off all other modes. Since the fundamental mode of the fiber can not be cut off, the single mode fiber only allows the fundamental mode. explain modes

Click here for a brief history of fiber optics provided by Jeff Hecht


Total Internal Reflection

Fiber optics work by using a electromagnetic phenomena called total internal reflection. Normal reflection and transmission happens when light or an electromagnetic wave hits the boundary of two media, with indices of refraction n1 and n2. Total internal reflection is characterized by the lack of a transmitted wave, meaning that the incident wave was completely reflected, thus total reflection. The word internal signifies that the index of refraction of the initial medium is larger than that of the second medium.



Total internal reflection occurs when the incident angle of the wave, theta1, is greater than or equal to the critical angle, thetaC, where the critical angle is defined as


It presents the profile of the far-field radiation of the optical fiber. The total internal reflection is due to Snell's law.

If theta1 equals the critical angle then sin(theta2) = 1, this means that theta2 = 90 degrees. This represents the transmitted wave traveling parallel to the surface of the boundary. Since energy can not flow on the boundary, no energy can propagate from this wave. Therefore, all of the energy must propagate in the reflected wave; this is total internal reflection.

If theta1 is greater than the critical angle, then there exists an A such that sin(theta1) = A*(n2/n1), where A > 1. Using Snell's law, this implies that sin(theta2) = A, and therefore sin(theta2) must be greater than 1. In order to obtain sin(theta2) greater than 1, theta2 must be a complex angle. In electromagnetic theory, it is given that an electromagnetic wave has the form


For the transmitted wave, the propagation factor, exp(ik*x), can now be calculated using the information from Snell's law.

k*x = k(x*sin(theta2) + y*cos(theta2))

where x is the horizontal direction
and y is the vertical direction
k*x = k(x*(n1/n2)*sin(theta1) + iy*sqrt((sin(theta1)*(n1/n2))^2 - 1)
since sin(theta2) = sin(theta1)*(n1/n2)
and cos(theta2) = 1 - (sin(theta2))^2

exp(ik*x) = exp(ikx*(n1/n2)*sin(theta1) * exp(-k*sqrt((sin(theta1)*(n1/n2))^2 - 1))

So propagation in the vertical, or y, direction is exponentially damped below the surface. This means that no energy can flow beyond a few wavelengths on the other side of the boundary. This is total internal reflection


Aligning the Fiber Optic

I found aligning the laser into the fiber optic to be an exceedingly frustrating and time consuming process. This is because the laser beam must be directed into the PAF fiber port, which is shown below. The PAF fiber port not only holds the fiber optic (yellow) in place, but it also contains a lens that focuses the laser light. This lens allows the whole of the laser beam's cross-section, which can be larger than the fiber optic, to be directed into the fiber. Alignment is very difficult because the laser beam and the fiber optic need to be directed and positioned appropriately so that an optimal amount of laser light gets into the fiber optic.

PAF Fiber Port

I used a method to align the laser beam into the fiber optic that was shown to me by Dr. John Noe. This method involved using the detector to measure the intensity of light that travels through the fiber optic as I adjust the alignment. Occassionally, the detector would be unable to register any light and I would have to look into the fiber optic directly in order to see any fluctuations in the transmitted light intensity.

Alignment Method
  • With the fiber removed, line the laser beam through the coupler. This alignment is done by moving the mirrors to get the beam through the coupler without it bouncing off of the coupler's sides. The beam must also be parrallel to the table top. To verify this, I marked the position of the beam on a card held perpendicular to the table and moved the card back and forth, making sure that the laser beam always hit the card in the same spot.
  • Slide the fiber into the coupler, but do not screw the fiber in all the way. See if any light is transmitted. By adjusting the two mirrors, try and maximize the amount of light output.
  • Slowly move the fiber inwards and readjust the mirrors to find another maximum.
  • Lock the fiber's position in the coupler.

The reason that I started with the fiber farther back in the coupler is because the beam covers a larger area farther away from the focus. So it's benefitial to start farther back and work your way further up by finding the maxima. Hal Metcalf likened the iteration of adjusting the mirrors and moving the fiber forward are to moving up a 'hill' in a four-dimensional phase space. I found this to be the frustrating aspect of this project, like Sisyphus I wondered whether I would ever get the laser beam up the hill.



Procedure for Taking Data

As mentioned in the Experimental Set-Up section, the data is obtained by recording the average, minimum and maximum voltage values from the multimeter over a minute timespan. Because these voltage values correspond to light intensity, all measurements are performed in the dark. Between each measurement, the lights are turned on, in order to record the values and reposition the detector at the next angle for measurement.


Gaussian Approximation/Theory

The center of the profile of a fiber optic should be approximated by a Gaussian curve, I(x) = I(0)*exp[-a*x^2], where x is the angular position of the detector, I(0) is the central maximum power of the beam and a = 2/(sigma^2) where sigma is the standard deviation of the curve.

M.Young provides a similar equation, I(theta) = I(0)*exp[-2*(sin(theta)/sin(thetaO))^2], where I(0) is the same and thetaO is the angular radius. ThetaO is then shown to equal lambda/(pi*omegaP) where lambda is the wavelength and omegaP is half of the mode-field diameter. The correct omegaP for a fiber is chosen to fit a given far-field profile.

For this project, I have used the first theory in my data analysis.


Data for Metrologia Helium-Neon Laser

Initially a Metrologia Heluim-Neon Laser was used as a source for the fiber optic. This laser has a wavelength of 633 nm and a intensity of 988 microWatts. We were able to obtain an alignment producing 564 microWatts at the output of the fiber. This corresponds to 57.14 percentage of the laser light traveling through the fiber optic. Two different resistors were used to take this data a 2.028 MOhm resistor and a 1.994 MOhm resistor.

Since the multimeter measures voltages, a resistor is used between the detector and the multimeter. Using the V=IR law, I obtained a current (mAmp) value. Then, I used the responsivity of the detector at the 633nm wavelength, 0.425 Amps/Watts, to find the power of the light from the detector-multimeter measurements.

Far-Field Radiation Profile


This is a graph of the power of light from the fiber optic(nW) versus the off center angle of the detector (degrees). Because the fiber optic was not perfectly directed to the center of the detector arm, the data curve was shifted to the right so that the maximum power would occur on the y axis. The theoretical curve was generated using the Solver application in Excel, and follows the equation
y = 1952799.6 * exp[-0.0817457 * x^2]. This implies that the standard deviation, sigma, of the Gaussian curve is 2.47316230583728.

This graph presents the profile of the far-field radiation of the optical fiber. The first ring of the diffraction pattern is almost visible. The intensity range is 10^4 but the intensity range is only 10^-7 Watts, not a precise as I was hoping to find. Because of this failure, I continued my experiment using the Meredith Helium-Neon laser.


Data for the Meredith Helium-Neon

We then switched to the Meredith Helium-Neon laser, a more powerful laser. We did this hoping that the Meredith would allow us to have a higher intensity of light through the fiber optic so that we could have more precise measurements.

This laser has a wavelength of 633nm and has an intensity of 19 mWatts. Unfortunately, after the first mirror only 15mWatts of light still exists. I am unsure exactly the cause of this drop but I think it is that the mirror is scratched and dirty. Because the mirrors that we use are gold, they can not be cleaned. The space between the second mirror and the PAF fiber port is too tight to allow for a measurement of the light after the second mirror. We were able to obtain an alignment of 6 mWatts. This corresponds to 39.99 precentage of the laser light after the first mirror traveling through the fiber optic.

Three different resistors were used to take these measurements, a 2.033 MOhm, a 1.022 MOhm, and a 9.87 kOhm. In this instance, different resistors were used in order to measure the current provided by the detector to a the highest available precision while maintaining the voltage in a measureable range. Using these different resistor values, the same form of calculations as with the Metrologia Helium-Neon Laser were done inorder to get the power of the light emitted from the fiber optic from the measured voltage values.

Far-Field Radiation Profile


This is another graph of the power of light from the fiber optic (nW) versus the off center angle of the detector (degrees). Again the fiber optic was not perfectly directed to the center of the detector arm, and the data needed to be shifted to the left in order to have the maximum power intersect the y axis; this also explains why there is more data in the negative angles. The theoretical curve was generated using the Solver application in Excel, and has the equation y = 24964.424839048 * exp[-.074121* x^2]. This implies that the standard deviation of the Gausssian curve, sigma, is 2.59725054884501.

This graph is another view of the profile of the far-field radiation of the optical fiber. This time the first ring in the diffraction pattern is definately visible and the second ring might be the cause of the small bump near -30 degrees. The intensity range is 10^6 and it has an intensity precision of 10^-10.


Conclusion

In conclusion, I studied the far field radiation of a single mode step index optical fiber. I was able to measure this radiation with less than half a degree of angular precision and an intensity precision of 10^-10 Watts using the Meredith laser. The Meterologia results were not as good; a precision of 10^-7 Watts was obtained. The first of the additional modes are visible in both the Meterologia and the Meredith graphs, although the Meredith results are much clearer. The data from both lasers were used to calculated Gaussian approximations of the peak of the far field radiation.

I attempted to use an amplifier to improve the precision of the Meterologia measurements. However, I ran into complications, specifically, when using the amplifier for small voltages a negative number would result. In order to study this phenomena, I used a voltage box and measured the output of the amplifier at a variety of values. But the negative outputs did not occur in this test despite the fact that they were produced repeatedly while taking measurements both before and after the tests with the volt box.

This project introduced me to the process of aligning a laser into a fiber optic. I must admit that I am not very proficient at this task. However, I have been able to improve my alignment ability and I am still working on refining this skill.


Special Thanks

John Noe, Luis Orozco, Harold Metcalf, Xiyue Miao, Matt Eardley


Main References