diffraction gratings
Posted: Fri Nov 11, 2016 1:58 pm
I apologize in advance for the long read.
As I mentioned in another post, early this fall my son explored Ed Wesley’s method of making a diffraction grating, described in his “Seven Single Beam Projects,” as the basis for his science project. In his project, he varied the angle between plate and mirror to see how it affected the spread of the rainbow produced by the grating. This was a great project for him, because he could position the mirrors and holo plate all on his own, and he already had experience measuring diffraction angles.
I started thinking about one result my son found, which in retrospect should have been obvious. In the single reflecting mirror setup of Ed’s method, the central axis of the spreading reference beam hits the holo plate at a 45 degree angle. So the reconstructing white light must illuminate the plate at the same 45 degree angle to produce a rainbow. Whereas with a normal diffraction grating, the light illuminates a grating at normal incidence. And so I started thinking about making a “normal incidence” diffraction grating. I know one could split a beam into two, send one in at normal incidence and send the other through at an angle with repect to the plate. But I wondered if there might be a way to make the “normal incidence” diffraction grating while still preserving the “single beam” nature of the project. It was obvious that it will take more than one plane mirror that is used in Ed’s method, but it took me a while playing with arrangements in my head to sort out how to do it.
Once I figured out how to do it, I thought this would be a great research project for one of my majors. I'm sure this has been done before, and so even if the results don’t really interest anyone else, I could file it under “proof of principle.” So this fall, a student and I began making normal incidence diffraction gratings.
The gratings were made with a 532 nm laser. We used Litiholo plates to make the gratings, because they are easy to use. But more importantly, we didn’t have to worry about shrinking or swelling of emulsion while the plate dried.
I’ll describe the geometry we used for making the grating.
First, normal incidence diffraction gratings are meant to be use with collimated light, so we had to (expand and) collimate the laser beam. We used a Galilean telescope composed from two plano-convex lenses to do this. All my good lenses are only one inch diameter, and so all the gratings we made are one inch diameter circles. (Note to self, need to purchase a good long-focal-length, two inch diameter lens.)
With the collimated beam at normal incidence to a plate on one side, we placed a plane first-surface mirror on the other side. This mirror was oriented 45 degrees from the plate. We chose a 10 cm distance between plate and mirror along beam central axis of the beam for no particular reason, and it seemed to work well. So now the beam passing through the plate is reflected 90 degrees, running parallel to the plate surface.
Then we intercepted the reflected beam with another plane first-surface mirror set at an angle from the first mirror, so that the second-reflected beam passes back through the plate, overlapping the incident beam. To achieve this overlap, the distance separating the two mirrors depends on the angle between the two mirrors. For our setup, we varied the angle between mirrors across the range 55 - 85 degrees, where mirror separation decreases as the angle between mirrors increases.
So in the setup we kept beam, plate position, and first mirror position always the same and we varied angle (and corresponding separation) of the second mirror. Subsequent measurements of diffraction from the gratings allowed us to deduce each grating’s characteristic lines/mm. We found a nice linear relation between lines/mm and angle between mirrors. This allowed us to set angles to produce standard gratings, I.e. 600 lines/mm and 1200 lines/mm.
The gratings behaved pretty much like normal gratings, even exhibiting a blaze angle where one first order spot was brighter than the other. It was pretty clear the gratings had maximum efficiency in the green region of the rainbow… not surprising since we were using green laser light to make them.
One issue we came across in the experimental setup is what to do with the reflected beam that passes through the plate. And another issue was that some of the reflected beam hitting the plate is reflected back into the mirror setup. Quite fun figuring out how to divert those beams, because their directions change with every change in angle between the mirrors. The major errors and uncertainties in the setup and in measuring the diffraction patterns arose from positioning everything by hand and not having precision angle measurements. Typically we might be off by one degree in the angle between mirrors and we had an uncertainty of half a degree in in diffraction pattern measurements. This could be improved, but again this is a "proof of principle" project.
So… if another student decides they want to work on this… next up is to try making gratings using different laser wavelength.
As I mentioned in another post, early this fall my son explored Ed Wesley’s method of making a diffraction grating, described in his “Seven Single Beam Projects,” as the basis for his science project. In his project, he varied the angle between plate and mirror to see how it affected the spread of the rainbow produced by the grating. This was a great project for him, because he could position the mirrors and holo plate all on his own, and he already had experience measuring diffraction angles.
I started thinking about one result my son found, which in retrospect should have been obvious. In the single reflecting mirror setup of Ed’s method, the central axis of the spreading reference beam hits the holo plate at a 45 degree angle. So the reconstructing white light must illuminate the plate at the same 45 degree angle to produce a rainbow. Whereas with a normal diffraction grating, the light illuminates a grating at normal incidence. And so I started thinking about making a “normal incidence” diffraction grating. I know one could split a beam into two, send one in at normal incidence and send the other through at an angle with repect to the plate. But I wondered if there might be a way to make the “normal incidence” diffraction grating while still preserving the “single beam” nature of the project. It was obvious that it will take more than one plane mirror that is used in Ed’s method, but it took me a while playing with arrangements in my head to sort out how to do it.
Once I figured out how to do it, I thought this would be a great research project for one of my majors. I'm sure this has been done before, and so even if the results don’t really interest anyone else, I could file it under “proof of principle.” So this fall, a student and I began making normal incidence diffraction gratings.
The gratings were made with a 532 nm laser. We used Litiholo plates to make the gratings, because they are easy to use. But more importantly, we didn’t have to worry about shrinking or swelling of emulsion while the plate dried.
I’ll describe the geometry we used for making the grating.
First, normal incidence diffraction gratings are meant to be use with collimated light, so we had to (expand and) collimate the laser beam. We used a Galilean telescope composed from two plano-convex lenses to do this. All my good lenses are only one inch diameter, and so all the gratings we made are one inch diameter circles. (Note to self, need to purchase a good long-focal-length, two inch diameter lens.)
With the collimated beam at normal incidence to a plate on one side, we placed a plane first-surface mirror on the other side. This mirror was oriented 45 degrees from the plate. We chose a 10 cm distance between plate and mirror along beam central axis of the beam for no particular reason, and it seemed to work well. So now the beam passing through the plate is reflected 90 degrees, running parallel to the plate surface.
Then we intercepted the reflected beam with another plane first-surface mirror set at an angle from the first mirror, so that the second-reflected beam passes back through the plate, overlapping the incident beam. To achieve this overlap, the distance separating the two mirrors depends on the angle between the two mirrors. For our setup, we varied the angle between mirrors across the range 55 - 85 degrees, where mirror separation decreases as the angle between mirrors increases.
So in the setup we kept beam, plate position, and first mirror position always the same and we varied angle (and corresponding separation) of the second mirror. Subsequent measurements of diffraction from the gratings allowed us to deduce each grating’s characteristic lines/mm. We found a nice linear relation between lines/mm and angle between mirrors. This allowed us to set angles to produce standard gratings, I.e. 600 lines/mm and 1200 lines/mm.
The gratings behaved pretty much like normal gratings, even exhibiting a blaze angle where one first order spot was brighter than the other. It was pretty clear the gratings had maximum efficiency in the green region of the rainbow… not surprising since we were using green laser light to make them.
One issue we came across in the experimental setup is what to do with the reflected beam that passes through the plate. And another issue was that some of the reflected beam hitting the plate is reflected back into the mirror setup. Quite fun figuring out how to divert those beams, because their directions change with every change in angle between the mirrors. The major errors and uncertainties in the setup and in measuring the diffraction patterns arose from positioning everything by hand and not having precision angle measurements. Typically we might be off by one degree in the angle between mirrors and we had an uncertainty of half a degree in in diffraction pattern measurements. This could be improved, but again this is a "proof of principle" project.
So… if another student decides they want to work on this… next up is to try making gratings using different laser wavelength.