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Design and construction of a refracting telescope
Design and construction of a refracting telescope

C f= s moO moo (8)
C f= s moO moo (8)

... from Eq. (11) we see that u(wc,,wy) for a real function f (xy) is bipolar, not complex, when evaluated at (cow,xy) = (pcoo,qwo). Thus a simplified detection scheme can be used, since the output (in 1-D for simplicity) is of the where form u(wcf)lp. = mpip! = (ImpI/p!)exp(j-rn), n = 0 or 1 only. Spec ...
In text you refer to OAP mirrors as 2nd etc, In fig, they are labeled
In text you refer to OAP mirrors as 2nd etc, In fig, they are labeled

... bending it into an arc-like pattern. Adjustment of this tilt itself proved one of the more effective means of determining the correct tilt angle for the OAP mirrors due to the observable aberrations introduced by even small initial errors. Simulations predict a spot size of 65 microns at the focal ...
Focusing of light through a stratified medium: a practical
Focusing of light through a stratified medium: a practical

Inexpensive optical tweezers for undergraduate laboratories
Inexpensive optical tweezers for undergraduate laboratories

Coherent Laser Beam Addition: Application of Binary-Optics Technology An
Coherent Laser Beam Addition: Application of Binary-Optics Technology An



Structure of Optical Vortices
Structure of Optical Vortices

... also forms images of trapped particles that are relayed to an attached video camera through a dichroic mirror. The SLM can shift the light’s phase to any of 150 distinct levels in the range 0 ≤ ϕ ≤ 2π radians at each 40 µm wide pixel in a 480 × 480 square array. Imprinting a discrete approximation t ...
Optimized back-focal-plane interferometry directly measures forces
Optimized back-focal-plane interferometry directly measures forces

... variables, found a linear relationship between stiffness and detector sensitivity (equivalent to our Eq. (6) and Fig. 3, below). More recently, by means of an experimental setup consisting of two traps of different stiffness simultaneously trapping the same sample, Jahnel et al. [19] observed that t ...
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Sample pages 1 PDF

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Identification and Determination of Crystal Structures and

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Chapter 34 Geometric Optics

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High-speed addressable confocal microscopy for functional imaging

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Observation of optical polarization Möbius strips

... of –1/2 and –3/2. (A and C) The numerically calculated polarization topologies in the focal plane of the beam. (B and D) The experimentally observed polarization topologies in the focal plane of the beam. Our experiment was performed under tight-focusing (nonparaxial) conditions, which accentuates t ...
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LABORATORY MANUAL (Modern Physics & General Optics) PL – 402 (2013-2014)

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Planoconcave lens by negative refraction of stacked subwavelength

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1 Introduction - Stony Brook Laser Teaching Center

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EBSD SEM TEM

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Total internal reflection holography for optical interconnections

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Lecture 16 - EECS @ UMich

Performance of extended depth of field systems and
Performance of extended depth of field systems and

... design the lens so that the MTF is as most insensitive as possible to the (unknown) object distance and easily invertible by digital processing. Many pupils have been designed to implement WFC; they all propose different trade-offs between MTF and DOF. In this paper, we demonstrate that for any symm ...
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Intensity Interferometry toward high resolution

Ultra-thin plasmonic optical vortex plate based on phase
Ultra-thin plasmonic optical vortex plate based on phase

- Phasics
- Phasics

... temporal10–13 coherence of the laser beam and to improve the focal pattern’s homogeneity. Such smoothed beams, currently planned to be used in the future megajoule-scale ICF facilities, however, still have speckles with local intensities a few times the average intensity. Performing laser–plasma int ...
P - University of South Florida
P - University of South Florida

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Airy disk



In optics, the Airy disk (or Airy disc) and Airy pattern are descriptions of the best focused spot of light that a perfect lens with a circular aperture can make, limited by the diffraction of light. The Airy disk is of importance in physics, optics, and astronomy.The diffraction pattern resulting from a uniformly-illuminated circular aperture has a bright region in the center, known as the Airy disk which together with the series of concentric bright rings around is called the Airy pattern. Both are named after George Biddell Airy. The disk and rings phenomenon had been known prior to Airy; John Herschel described the appearance of a bright star seen through a telescope under high magnification for an 1828 article on light for the Encyclopedia Metropolitana:...the star is then seen (in favourable circumstances of tranquil atmosphere, uniform temperature, &c.) as a perfectly round, well-defined planetary disc, surrounded by two, three, or more alternately dark and bright rings, which, if examined attentively, are seen to be slightly coloured at their borders. They succeed each other nearly at equal intervals round the central disc....However, Airy wrote the first full theoretical treatment explaining the phenomenon (his 1835 ""On the Diffraction of an Object-glass with Circular Aperture"").Mathematically, the diffraction pattern is characterized by the wavelength of light illuminating the circular aperture, and the aperture's size. The appearance of the diffraction pattern is additionally characterized by the sensitivity of the eye or other detector used to observe the pattern.The most important application of this concept is in cameras and telescopes. Owing to diffraction, the smallest point to which a lens or mirror can focus a beam of light is the size of the Airy disk. Even if one were able to make a perfect lens, there is still a limit to the resolution of an image created by this lens. An optical system in which the resolution is no longer limited by imperfections in the lenses but only by diffraction is said to be diffraction limited.
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