Overlaying optical field with Zernike aberration

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SUMMARY

The discussion centers on the application of Zernike polynomials Vmn(ρ,θ) for modeling optical aberrations in simulations. Key parameters include R, the radius, and A, the amplitude of aberration expressed in radians at R. The optical field is computed using complex expressions involving the real and imaginary components of the field, which are influenced by the amplitude and Zernike polynomial values. The source of these formulas is linked to the Fresnel diffraction integral and the definitions provided in the textbook "Born and Wolf."

PREREQUISITES
  • Understanding of Zernike polynomials and their application in optical aberration modeling.
  • Familiarity with complex numbers and their role in representing optical fields.
  • Knowledge of Fresnel diffraction integrals and their significance in optics.
  • Basic grasp of trigonometric functions and their dimensional requirements.
NEXT STEPS
  • Study the derivation and application of Zernike polynomials in optical systems.
  • Explore the Fresnel diffraction integral and its implications in wavefront analysis.
  • Review "Born and Wolf" for a comprehensive understanding of optical aberrations and their mathematical representations.
  • Investigate the relationship between amplitude and angle in trigonometric functions within optical contexts.
USEFUL FOR

Optical engineers, physicists, and researchers involved in wavefront analysis and optical system design will benefit from this discussion.

lechris
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Hi there,
optical aberrations can be expressed by Zernike polynomials Vmn(ρ,θ).
Now, for my simulations i am using software that takes 4 inputs for creating aberrations onto an optical flat: m,n,R,A
m,n are the Zernike orders which is perfectly clear.
For R,A the manual says:
R: the radius
A: the amplitude of aberration in radians reached at R
I am still unclear how to interpret these parameters. I was looking through the source code and could make up the following:
ρ = sqrt( x*x + y*y )/ R*R) which i suppose does some kind of spatial scaling of the aberration
A is the Amplitude of the Zernike polynomial A*Vmn(ρ,θ), which i suppose does some kind of height scaling

Finally the optical field is composed as such:
RE{Field} = RE{Field_old}*cos(A*Vmn(ρ,θ)) - IM{Field_old}*sin(A*Vmn(ρ,θ))
IM{Field} = RE{Field_old}*sin(A*Vmn(ρ,θ)) + IM{Field_old}*cos(A*Vmn(ρ,θ))

Can someone explain to me how the parameters are supposed to work? Since when is amplitude expressed in radians?
I couldn't find the aforementioned formulas in any standard textbook yet (i see that the last 2 are just complex numbers multiplied, which represent the optical fields). Where are these formulas taken from?
 
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Zoiks... you're definitely out in the weeds here, based on your notation I recommend checking out the relevant sections in Born and Wolf. Ok- first, some background. Zernike polynomials are one way to parameterize the aberration function, which itself is a way to describe the departure of the actual wavefront from an ideal (spherical) wavefront. Zernike polynomials are defined on a circle: Vmn(ρ sinθ,ρ cosθ)=Rmn(ρ) einθ. This is the connection with your RE{field} and IM{field} expressions (and also derived in Born and Wolf).

Because the polynomials are defined on the unit circle, you can scale by the actual radius (as you mention). Why is the amplitude in radians? Because of the way the aberration function Φ is defined: the optical field at a point P, U(P), is given as a Fresnel diffraction integral, and the aberration function gets placed in the integrand e ik(Φ+s).

Does this help? The topic is very math-intensive, too much for my limited LaTex abilities here.
 
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lechris said:
Since when is amplitude expressed in radians?
I never heard of Zernike polynomials but the dimensions must be right in any formula.
If A is inside a trig function then you have to be talking in terms of angles and radians are the way to specify an angle. (The argument of a trig function has to be dimensionless)
 

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