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Chapter 3 Geometric Optics
Chapter 3 Geometric Optics

Basic Wavefront Aberration Theory for Optical Metrology
Basic Wavefront Aberration Theory for Optical Metrology

PHYS 242 BLOCK 11 NOTES Sections 33.1 to 33.7 Geometrical
PHYS 242 BLOCK 11 NOTES Sections 33.1 to 33.7 Geometrical

... However, for any angle of incidence greater than or equal to the critical angle θcrit, all of the incident light reflects (therefore, none refracts), a phenomenon called total internal reflection. See Figure 33.13a. When θa = θcrit, θb nb = 90˚. Therefore, Snell’s law gives na sin θcrit = nb sin 90˚ ...
L32
L32

Using ray matrices to derive analytical expressions of optical
Using ray matrices to derive analytical expressions of optical

Thin Lenses
Thin Lenses

f = l - UCSD Department of Physics
f = l - UCSD Department of Physics

... “near point”, L = 25 cm. So, the largest angular size of a fine-print object with height h is a = h/L. A magnifying glass creates a virtual image with the same angular size as the object, but you can now have the object at a small distance f from your eye. So, the angular size is ...
Plane Mirrors
Plane Mirrors

Correcting chromatic aberrations using a diffraction grating in a
Correcting chromatic aberrations using a diffraction grating in a

Chester F - RIT Center for Imaging Science
Chester F - RIT Center for Imaging Science

A1982PU06800001
A1982PU06800001

... Chase’s discussion was the most com3 plete and the one published. “The problem was caused by an extra term in the solution arising from a possible statistical correlation between the coherence function and the local variation in the air’s index of refraction. Some time later it was shown that this e ...
ppt
ppt

Essentials of the AV Industry Pretest Not sure if you need to take
Essentials of the AV Industry Pretest Not sure if you need to take

... 33. A common technique for reducing the depth requirements of a rear projection space is ______ a. Increasing image size. b. Splitting the light path. c. Folding the light path. d. Intensifying light output. 34. The changing of direction of a light or sound ray is called _______ a. Spherical aberrat ...
trigonometry
trigonometry

First Order Optics
First Order Optics

... prisms which can be used to fold an optical system into different geometries. They are the deviation, dispersion, displacement, rotation and expansion prisms. In addition to the 3D coordinate system, image motion due to a prism can also be described by the image handedness and parity. Image handedne ...
PPT
PPT

... • The default/conventional behavior has light going from left to right (toward positive z) • But changing the sign of the refractive index signals a change of direction – after all, refractive index indicates the speed of light in a medium, and the speed changes sign at a reflection ...
the P3 `bus stop`
the P3 `bus stop`

Microscope
Microscope

Universal Description of Spherical Aberration Free Lenses
Universal Description of Spherical Aberration Free Lenses

... this function assumes the form of all the conic sections and expands the theory of aplanatic optical surfaces. There are two different symmetry centers with respect to the index that create an asymmetric relationship between positive and negative index lens profiles. In the thin lens limit the famil ...
Drawing Ray Diagrams for Concave Mirrors
Drawing Ray Diagrams for Concave Mirrors

Document
Document

PowerPoint (PPT) One: The theories of light in historical perspective
PowerPoint (PPT) One: The theories of light in historical perspective

... a spherical shell acts as a concave mirror, and a beam of parallel rays is incident on it,then all rays after being reflected pass through the same point, call it F, or the “focal point”. The distance between F and the mirror surface (usually denoted as f ) is ½ R, where R is the radius of the spher ...
PowerPoint (PPT) One: The theories of light in historical perspective
PowerPoint (PPT) One: The theories of light in historical perspective

... a spherical shell acts as a concave mirror, and a beam of parallel rays is incident on it,then all rays after being reflected pass through the same point, call it F, or the “focal point”. The distance between F and the mirror surface (usually denoted as f ) is ½ R, where R is the radius of the spher ...
setting up of a total internal reflection fluorescent microscope
setting up of a total internal reflection fluorescent microscope

... does not vanish due to the continuity of the Maxwell equations for interfaces of different refractive indices. The resulting electromagnetic wave is called an evanescent wave. The conundrum of a non-zero intensity in the second medium, while having total internal reflection, is solved by the fact th ...
Focal length
Focal length

... by making sure the concave surface of the mirror is parabolic ...
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Optical aberration



An optical aberration is a departure of the performance of an optical system from the predictions of paraxial optics. In an imaging system, it occurs when light from one point of an object does not converge into (or does not diverge from) a single point after transmission through the system. Aberrations occur because the simple paraxial theory is not a completely accurate model of the effect of an optical system on light, rather than due to flaws in the optical elements.Aberration leads to blurring of the image produced by an image-forming optical system. Makers of optical instruments need to correct optical systems to compensate for aberration.The articles on reflection, refraction and caustics discuss the general features of reflected and refracted rays.
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