Aberrations  Aberrations of Lenses  Analogue to Holographic Model  Aberrations in Holography  Implications in the aberration equations  Experimental.

Slides:



Advertisements
Similar presentations
Consider Refraction at Spherical Surfaces:
Advertisements

Notation for Mirrors and Lenses
Flat Mirrors Consider an object placed in front of a flat mirror
Lenses in the Paraxial Limit
Lens Aberrations Aberration: a departure from the paraxial limit.
Chapter 23 Mirrors and Lenses.
Chapter 31 Images.
Chapter 23 Mirrors and Lenses.
Chapter 23 Mirrors and Lenses Conceptual questions: 4,5,10,14,15,17
Chapter 36 Image Formation.
A wave front consists of all points in a wave that are in the same phase of motion. A wave front is one of many properties that light waves share with.
Chapter 23 Mirrors and Lenses.
Chapter 32Light: Reflection and Refraction. Electromagnetic waves can have any wavelength; we have given different names to different parts of the wavelength.
Chapter 23 Mirrors and Lenses. Notation for Mirrors and Lenses The object distance is the distance from the object to the mirror or lens Denoted by p.
Chapter 23 Mirrors and Lenses.
Lecture 23 Mirrors Lens.
Reference Book is Geometric Optics.
Chapter 23 Mirrors and Lenses.
Light: Geometric Optics
Image Formation by Mirrors and Lenses
Light and Reflection Level 1 Physics. Facts about Light It is a form of Electromagnetic Energy It is a part of the Electromagnetic Spectrum and the only.
Chapter 25. Mirrors and the Reflection of Light Our everyday experience that light travels in straight lines is the basis of the ray model of light. Ray.
Reflective Optics Chapter 25. Reflective Optics  Wavefronts and Rays  Law of Reflection  Kinds of Reflection  Image Formation  Images and Flat Mirrors.
Aperture Pupil (stop) Exit Pupil Entrance Pupil.
Geometric Optics of thick lenses and Matrix methods
Optics 1----by Dr.H.Huang, Department of Applied Physics
Small f/number, “fast” system, little depth of focus, tight tolerances on placement of components Large f/number, “slow” system, easier tolerances,
Interference Physics 202 Professor Lee Carkner Lecture 22.
Lenses We will only consider “thin” lenses where the thickness of the lens is small compared to the object and image distances. Eugene Hecht, Optics, Addison-Wesley,
Optical Center Eugene Hecht, Optics, Addison-Wesley, Reading, MA, 1998.
Fiber Optics Defining Characteristics: Numerical Aperture Spectral Transmission Diameter.
Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display. Chapter 23: Reflection and Refraction of Light.
Mirrors and Lenses. Optics Terminology and Assumptions Focus or focal point – point from which a portion of waves diverge or on which they converge Optical.
Chapter 23 Mirrors and Lenses.
Imaging Science FundamentalsChester F. Carlson Center for Imaging Science Mirrors and Lenses.
Physics 1C Lecture 26A.
Chapter 23 Mirrors and Lenses.
Physics 014 Images. Topics  Plane mirrors  Spherical mirrors  Thin lenses.
Fundamental of Optical Engineering Lecture 3.  Aberration happens when the rays do not converge to a point where it should be. We may distinguish the.
Chapter 36 Image Formation (Lens and Mirrors) Using the ray approximation of geometric optics, we can now study how images are formed with mirrors and.
Unit 11: Part 2 Mirrors and Lenses. Outline Plane Mirrors Spherical Mirrors Lenses The Lens Maker’s Equation Lens Aberrations.
3/4/ PHYS 1442 – Section 004 Lecture #18 Monday March 31, 2014 Dr. Andrew Brandt Chapter 23 Optics The Ray Model of Light Reflection; Image Formed.
1 Chapter 5 Geometrical optics January 21,23 Lenses 5.1 Introductory remarks Image: If a cone of rays emitted from a point source S arrives at a certain.
Chapter 34 Lecture Seven: Images: I HW 3 (problems): 34.40, 34.43, 34.68, 35.2, 35.9, 35.16, 35.26, 35.40, Due Friday, Sept. 25.
Yi-Chin Fang, Institute of Electro-Optical Engineering, National Kaohsiung First Univ. of Science and Technology Improvements of Petzval Field Curvature.
In describing the propagation of light as a wave we need to understand: wavefronts: a surface passing through points of a wave that have the same phase.
Lenses and imaging MIT 2.71/ /10/01 wk2-a-1 Huygens principle and why we need imaging instruments A simple imaging instrument: the pinhole camera.
Lenses and Imaging (Part I) Why is imaging necessary: Huygen’s principle – Spherical & parallel ray bundles, points at infinity Refraction at spherical.
Light Reflection and Mirrors.  The Law of Reflection  When a wave traveling in two dimensions encounters a barrier, the angle of incidence is equal.
Physics 203/204 4: Geometric Optics Images formed by refraction Lens Makers Equation Thin lenses Combination of thin lenses Aberration Optical Instruments.
Prof. Charles A. DiMarzio Northeastern University Fall 2003 July 2003
Physics 212 Lecture 27, Slide 1 Physics 212 Lecture 27: Mirrors.
Calculate distances and focal lengths using the mirror equation for concave and convex spherical mirrors. Draw ray diagrams to find the image distance.
July © Chuck DiMarzio, Northeastern University ECEG105/ECEU646 Optics for Engineers Course Notes Part 2: Geometric Optics (Reflection,
Chapter 18 Mirrors and Lenses. Curved Mirrors Concave shaped mirrors cause parallel light rays to converge. Convex shaped mirrors cause parallel light.
ECEG105 & ECEU646 Optics for Engineers Course Notes Part 2: Geometric Optics (Reflection, Refraction, Thin Lenses) Prof. Charles A. DiMarzio Northeastern.
Image Formation. The light rays coming from the leaves in the background of this scene did not form a focused image on the film of the camera that took.
Part 10 Optics --Mirrors and Lenses Chapter 24 Geometric Optics.
Basics Reflection Mirrors Plane mirrors Spherical mirrors Concave mirrors Convex mirrors Refraction Lenses Concave lenses Convex lenses.
Spherical Aberration. Rays emanating from an object point that are incident on a spherical mirror or lens at different distances from the optical axis,
July © Chuck DiMarzio, Northeastern University ECEG105/ECEU646 Optics for Engineers Course Notes Part 4: Apertures, Aberrations Prof.
Chapter 23 Mirrors and Lenses © 2014 A. Dzyubenko.
Chapter 5 Geometrical optics
Mirrors and Lenses Images can be formed by reflection from mirrors.
IMAGE FORMATION e.g. lens, mirors
Chapter 5 Geometrical optics
Mirrors, Plane and Spherical Spherical Refracting Surfaces
The Reflection of Light: Mirrors
The Reflection of Light: Mirrors
Presentation transcript:

Aberrations  Aberrations of Lenses  Analogue to Holographic Model  Aberrations in Holography  Implications in the aberration equations  Experimental Demonstration

Lenses image on-axis points perfectly. Non-paraxial and extended images exhibit aberrations.

An aberration in an imaging system is defined as any distortion of an image due to imperfections in the imaging system. In standard optics, these occur for non-axial object points and extremal rays. Note that a mis-aligned optic effectively creates an off-axis point.

There are 5 standard aberrations known as the Seidel Aberrations: o Spherical Aberration o Coma o Astigmatism o Petzval (Field)(Curvature o Distortion

Spherical Aberration

Coma

When sagittal rays focus, transverse rays make a horizontal line. When transverse is in focus, sagittal rays make a vertical line.

Field curvature

Distortion is due to magnification being different for the axial and marginal rays (This shows the stretching of a flat image – not a 3D bulging view)

The wave model compares the aberrated focus to an ideal spherical focus which is defined by the physical optic.

W = 0 C 40 (r 4 ) + 1 C 31 (  )(r 3 )cos(  ) + 2 C 22 (  ) 2 (r 2 )cos 2 (  ) + 2 C 20 (  ) 2 (r 2 ) + 3 C 11 (  ) 3 (r)cos(  ) Each of the the five terms in the aberration function represent the five Seidel aberrations: The first three terms lead to a blurring of the image point and the next two lead to a distortion of the image.

The Holographic Model In order to show a correlation between holography and conventional lenses, an equivalent “focal length”, f R for the hologram may be derived from the reconstructed phase wavefront. This is allowable insofar as the reconstructed phase wavefront is also a converging spherical wavefront and maybe thought of as the “reference sphere”.

Analogue of Seidel aberrations for Holography: Assume a point-source object, and compare the aberrated wavefront to the correct wavefront.

1.Assume a point source for the object and a point source for the reference. 2.Assume a different point source for the reconstruction source. 3.An image point is derived from the coordinates of the original object point, the original reference point and the alternate reference point. 4.Seidel aberrations are determined by the phase mismatch between the image point from the correct reference and the image point from the alternate reference point.

The Derivation: The emerging reconstructed phase wavefront is the sum of the recorded phases and the phase of the reconstruction wave.  =  c +/-  r +/-  o Signs indicate original (virtual) image or conjugate (real). The general expression from a point G for a spherical wave is  = 2  {[(x - x g ) 2 + (y-y g ) 2 + z g 2 ] 1/2 – [x g 2 + y g 2 + z g 2 ] 1/2 } Substituting this into the above, with the specific coordinates and replacing the general coordinates, an exact expression is obtained for the phase at the hologram plane.

This analysis now creates an image point derived from the coords of the original ref, the object and the recon beam and is given by image coordinates X i, Y i and Z i X i =(x c z o z r +  x o z c z r -  x r z c z o )/(z o z r +  z c z r -  z c z o ) Z i = z o z c z r /(z o z r +  z c z r -  z c z o )

 Thus, for the object beam coordinate, zo, and the equivalent image position Zi, under the assumption of a spherical wavefront, we may construct a lens equivalent expression  (1/z o ) + (1/Z i ) = 1/ f R ) = 1/z o +/- (  )(1/z o + 1/z r  by comparing the standard lens equation 1/s i + 1/s o = 1/f  and also Champagne's derivation of image distance 1/R f = 1/R c +/- (  )(1/R o + 1/R r )

Resolution Not valid to compare with electronic pixels. Strictly, the resolution of the image as a function of source size needs to be calculated using the Van Cittert-Zernike theorem May be described as a comparison of the size of the reconstruction point to the size of the image source, giving: dX i /d x c = (z o z r )/(z o z r +  ( z o z r – z o z c )) dZ i /d z c = (z o z r )/(z o z r +  (z c z r – z c z o ))

Magnification o Transverse o Longitudinal o Angular M T = dX i /dx o = 1/(1+/- z o /  z c – z o /z r ) (paraxial) M T = (cos  o /cos  i ){1/(1+/-z o /  z c – z o /z r )} (nonparaxial) M L = dZ i /dz o = -(1/  ){1/(1-z o [(1/  z c ) + (1/z r )} 2 -(1/  )MT M A = d(X i /Z i )/d(x o /z o ) =  (paraxial) M A =  cos  o /cos  i ) (nonparaxial)

Expanding the spherical wavefront expression to third order produces the third order aberrations – the Seidel Aberrations for holography. Once again, the difference between the ideal sphere and the actual wavefront, W, gives the actual aberratiion function.

W = 2  c [(-1/8)   S Spherical Aberration +(1/2)    C x cos  C y sin  Coma -(1/2)    x cos 2  A y sin 2  A xy cos  sin  Astigmatism +1(1/4)   F Petzval Curvature +(1/2) r(D x cos  + D y sin  )] Distortion Transforming to a circular coordinate system, this gives for the Seidel aberration function:

Experimental results A planar image was recorded at 514nm with a collimated reference at 30 degrees.

This was reconstructed under a variety of alternate beam geometries: o Varying reconstruction angle + /- o Varying beam divergence + / - o Alternate wavelength at those geometries We shall see how these changes affect the image by imaging onto a screen with a calibrated scale.

Lateral Displacement and Coma appear when the reconstruction angle is off.

Magnification occurs both laterally and longitudinally when the divergence is off.

When the angle and divergence are off, the image rolls to the side, exhibiting multiple aberrations.

When reconstructed at 633nm, all of these effects are further shifted… Image is displaced, shrunken, bowed, and cannot be focused

Conclusion: Best practice is to always reconstruct a hologram with a source that matches the construction geometry, including avoiding aberrations occurring within the reconstruction source itself. When aberrations occur, understanding the different effects will aid in troubleshooting the system.