Optics: Center of Fizeau Fringe? Michelson Interferometer

In summary, the center of the interference fringes depends on the focal length. There are books that provide a closed-form expression for the hyperbolic fringes, but so far i haven't found anything in the common literature that discusses the problem with an extended light source.
  • #1
lechris
4
0
Hello everyone,

i am simulating a Michelson interferometer, where one mirror is slightly tilted, see picture.. This results in circular arcs / hyperbolic cross-section fringes. The center of these fringes depends on the focal length i am using, see picture.
Is there an analytical expression for the center of these fringes in dependency of the focal lenght?
Are there books that show the closed-form expression for such hyperbolic fringes / Fizeau fringes (so far i haven't found anything in the common literature).

Would be great if anyone has some insights on this.

Thanks!
 

Attachments

  • interference.png
    interference.png
    24.5 KB · Views: 2,431
Science news on Phys.org
  • #2
The interference of spherical waves emitted by a pair of point sources forms a family of hyperboloids of revolution with the foci located at the two sources. Imagine a pair of point sources located at ##x=-a## and ##x=a## and further assume that the amplitudes emitted by the two source are equal, then the intensity in space at a point ##(x,y,z)## far away from either sources is given by
$$
I(x,y,z) = \frac{A}{r^2}\cos^2 \left( \frac{\pi}{\lambda}(r_2-r_1)-\frac{\Delta\phi}{2}\right)
$$
where ##\Delta\phi## is the phase lag at the sources, ##r_1 = \sqrt{(x+a)^2+y^2+z^2}##, ##r_2 = \sqrt{(x-a)^2+y^2+z^2}##, and ##r = (r_1+r_2)/2##. You can determine the shape of the surface of constant phase difference (phase difference is simply the argument of ##\cos^2##) by equating the argument of ##\cos^2## to certain value. For interference maximum, obviously this value must be ##m\pi## where ##m## is an integer. I will leave to you that the expression
$$
\frac{\pi}{\lambda}(r_2-r_1)-\frac{\Delta\phi}{2} = C
$$
with ##C## constant does form a hyperboloid of revolution, e.g. by taking square twice. Thus if you place a screen for example at the plane ##z=Z##, you will observe alternating fringes in a form of hyperbolas.
 
  • Like
Likes lechris
  • #3
Hi blue_leaf77,
thanks for your answer. The problem is, i don't have 2 spherical wave emitted by a point source. I have an extended light source with radial aperture transmitted through a positive lens, see picture original post. I still don't see how the center of the interference fringes relates to the focal length of the length.
The closest i came to the solution is what i have attached as a drawing, but it still does not address the problem of an extended light source with positive lens.
 

Attachments

  • sol_draw.png
    sol_draw.png
    1.5 KB · Views: 753
  • #4
How does the beam from your extended source come to the lens? Will it approximate your application if the beam is modeled by a Gaussian beam? If yes, the focal point behind the lens can be well approximated by a point source. If not, then it might be too complicated to give a closed form equation.
lechris said:
Are there books that show the closed-form expression for such hyperbolic fringes / Fizeau fringes (so far i haven't found anything in the common literature).
That's what you asked. The equation in post#2 addresses the indirect answer to this question. You can also find a similar expression in "Optics" by Bruno Rossi. But he also treated the case of a pair of point sources.
 
Last edited:
  • Like
Likes lechris
  • #5
blue_leaf77 said:
How does the beam from your extended source come to the lens? Will it approximate your application if the beam is modeled by a Gaussian beam? If yes, the focal point behind the lens can be well approximated by a point source. If not, then it might be too complicated to give a closed form equation.
I use a simulation software which initializes an optical field and i instantly create the lens afterwards, so the optical field source and the lens are on top of each other. The software uses Fourier optics for the simulation. All i specify is the focal length, wave length and aperture size.
My primary goal is to find the center of the fringes that appear on the screen (with respect to the mirror angle). A closed-form solution of the fringes would be great but the fringe center would suffice. I just thought it is necessary to have a closed-form solution to derive the center point.
I have attached an equivalent drawing of the Michelson setup. Shouldn't it be possible to find the center of fringes solely using ray optics (virtual screens M1' and M2' need to be overlaid)? For solving the problem with a Gaussian beam i would need the initial waist size of the beam, which i don't have unfortunately.
 

Attachments

  • michel_prob.png
    michel_prob.png
    9.6 KB · Views: 733

FAQ: Optics: Center of Fizeau Fringe? Michelson Interferometer

What is the purpose of the Center of Fizeau Fringe in optics?

The Center of Fizeau Fringe is a point on the interference pattern produced by a Michelson Interferometer where the path difference between the two beams is equal to zero. It is used to determine the wavelength of light and can also be used to measure small changes in the distance between two mirrors.

How is the Center of Fizeau Fringe calculated?

The Center of Fizeau Fringe is calculated by finding the point on the interference pattern where the intensity of light is at its maximum. This is done by adjusting the mirror position until the fringes are maximized, and then using this position to calculate the path difference between the two beams.

How does the Michelson Interferometer work?

The Michelson Interferometer works by splitting a beam of light into two beams, reflecting them off two mirrors, and then recombining them. The interference pattern produced by the recombined beams is then analyzed to measure properties of the light such as wavelength, phase, and intensity.

What are some practical applications of the Michelson Interferometer?

The Michelson Interferometer has a wide range of practical applications in various fields such as physics, astronomy, and engineering. It is used to measure small displacements, to calibrate optical devices, and to study the properties of light. It is also used in the development of precision instruments, such as lasers and telescopes, and in the study of gravitational waves.

What are the advantages of using a Michelson Interferometer?

One of the main advantages of using a Michelson Interferometer is its high precision and accuracy in measuring properties of light. It is also a relatively simple and inexpensive setup, making it widely accessible for research and educational purposes. Additionally, the interferometer can be easily modified and adapted for specific experiments, making it a versatile tool in optics research.

Back
Top