Measuring Chromatic Aberrations in Imaging Systems Using Plasmonic Nano‐Particles
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Depth-Aware Blending of Smoothed Images for Bokeh Effect Generation
1 Depth-aware Blending of Smoothed Images for Bokeh Effect Generation Saikat Duttaa,∗∗ aIndian Institute of Technology Madras, Chennai, PIN-600036, India ABSTRACT Bokeh effect is used in photography to capture images where the closer objects look sharp and every- thing else stays out-of-focus. Bokeh photos are generally captured using Single Lens Reflex cameras using shallow depth-of-field. Most of the modern smartphones can take bokeh images by leveraging dual rear cameras or a good auto-focus hardware. However, for smartphones with single-rear camera without a good auto-focus hardware, we have to rely on software to generate bokeh images. This kind of system is also useful to generate bokeh effect in already captured images. In this paper, an end-to-end deep learning framework is proposed to generate high-quality bokeh effect from images. The original image and different versions of smoothed images are blended to generate Bokeh effect with the help of a monocular depth estimation network. The proposed approach is compared against a saliency detection based baseline and a number of approaches proposed in AIM 2019 Challenge on Bokeh Effect Synthesis. Extensive experiments are shown in order to understand different parts of the proposed algorithm. The network is lightweight and can process an HD image in 0.03 seconds. This approach ranked second in AIM 2019 Bokeh effect challenge-Perceptual Track. 1. Introduction tant problem in Computer Vision and has gained attention re- cently. Most of the existing approaches(Shen et al., 2016; Wad- Depth-of-field effect or Bokeh effect is often used in photog- hwa et al., 2018; Xu et al., 2018) work on human portraits by raphy to generate aesthetic pictures. -
Chapter 3 (Aberrations)
Chapter 3 Aberrations 3.1 Introduction In Chap. 2 we discussed the image-forming characteristics of optical systems, but we limited our consideration to an infinitesimal thread- like region about the optical axis called the paraxial region. In this chapter we will consider, in general terms, the behavior of lenses with finite apertures and fields of view. It has been pointed out that well- corrected optical systems behave nearly according to the rules of paraxial imagery given in Chap. 2. This is another way of stating that a lens without aberrations forms an image of the size and in the loca- tion given by the equations for the paraxial or first-order region. We shall measure the aberrations by the amount by which rays miss the paraxial image point. It can be seen that aberrations may be determined by calculating the location of the paraxial image of an object point and then tracing a large number of rays (by the exact trigonometrical ray-tracing equa- tions of Chap. 10) to determine the amounts by which the rays depart from the paraxial image point. Stated this baldly, the mathematical determination of the aberrations of a lens which covered any reason- able field at a real aperture would seem a formidable task, involving an almost infinite amount of labor. However, by classifying the various types of image faults and by understanding the behavior of each type, the work of determining the aberrations of a lens system can be sim- plified greatly, since only a few rays need be traced to evaluate each aberration; thus the problem assumes more manageable proportions. -
Sky & Telescope
S&T Test Report by Rod Mollise Meade’s 115-Millimeter ED Triplet This 4.5-inch apochromat packs a lot of bang for the buck. 115mm Series 6000 THIS IS A GREAT TIME to be in the ice and was eager to see how others market for a premium refracting tele- performed. So when I was approached ED Triplet APO scope. The price for high-quality refrac- about evaluating Meade’s 115mm Series U.S. Price: $1,899 tors has fallen dramatically in recent 6000 ED Triplet APO, I was certainly up meade.com years, and you can now purchase a for the task. 4- to-5-inch extra-low dispersion (ED) First impressions are important, and What We Like apochromatic (APO) telescope that’s when I unboxed the scope on the day Sharp, well-corrected optics almost entirely free of the false color it arrived, I lit up when I saw it. This is Color-free views that plagues achromats for a fraction of Attractive fi nish the cost commonly seen a decade ago. I’ve had a ball with my own recently q The Meade 115mm Series 6000 ED Triplet What We Don’t Like purchased apochromat after using APO ready for a night’s activity, shown with an optional 2-inch mirror diagonal. The scope Visual back locking almost nothing but Schmidt-Cassegrain also accepts fi nderscopes that attach using a system can be awkward telescopes for many years. However, I standardized dovetail system commonly found Focuser backlash still consider myself a refractor nov- on small refractors. -
A N E W E R a I N O P T I
A NEW ERA IN OPTICS EXPERIENCE AN UNPRECEDENTED LEVEL OF PERFORMANCE NIKKOR Z Lens Category Map New-dimensional S-Line Other lenses optical performance realized NIKKOR Z NIKKOR Z NIKKOR Z Lenses other than the with the Z mount 14-30mm f/4 S 24-70mm f/2.8 S 24-70mm f/4 S S-Line series will be announced at a later date. NIKKOR Z 58mm f/0.95 S Noct The title of the S-Line is reserved only for NIKKOR Z lenses that have cleared newly NIKKOR Z NIKKOR Z established standards in design principles and quality control that are even stricter 35mm f/1.8 S 50mm f/1.8 S than Nikon’s conventional standards. The “S” can be read as representing words such as “Superior”, “Special” and “Sophisticated.” Top of the S-Line model: the culmination Versatile lenses offering a new dimension Well-balanced, of the NIKKOR quest for groundbreaking in optical performance high-performance lenses Whichever model you choose, every S-Line lens achieves richly detailed image expression optical performance These lenses bring a higher level of These lenses strike an optimum delivering a sense of reality in both still shooting and movie creation. It offers a new This lens has the ability to depict subjects imaging power, achieving superior balance between advanced in ways that have never been seen reproduction with high resolution even at functionality, compactness dimension in optical performance, including overwhelming resolution, bringing fresh before, including by rendering them with the periphery of the image, and utilizing and cost effectiveness, while an extremely shallow depth of field. -
Adaptive Optics in Laser Processing Patrick S
Salter and Booth Light: Science & Applications (2019) 8:110 Official journal of the CIOMP 2047-7538 https://doi.org/10.1038/s41377-019-0215-1 www.nature.com/lsa REVIEW ARTICLE Open Access Adaptive optics in laser processing Patrick S. Salter 1 and Martin J. Booth1 Abstract Adaptive optics are becoming a valuable tool for laser processing, providing enhanced functionality and flexibility for a range of systems. Using a single adaptive element, it is possible to correct for aberrations introduced when focusing inside the workpiece, tailor the focal intensity distribution for the particular fabrication task and/or provide parallelisation to reduce processing times. This is particularly promising for applications using ultrafast lasers for three- dimensional fabrication. We review recent developments in adaptive laser processing, including methods and applications, before discussing prospects for the future. Introduction enhance ultrafast DLW. An adaptive optical element Over the past two decades, direct laser writing (DLW) enables control over the fabrication laser beam and allows with ultrafast lasers has developed into a mature, diverse it to be dynamically updated during processing. Adaptive – and industrially relevant field1 5. The ultrashort nature of elements can modulate the phase, amplitude and/or the laser pulses means that energy can be delivered to the polarisation of the fabrication beam, providing many focus in a period shorter than the characteristic timescale possibilities for advanced control of the laser fabrication for thermal diffusion, leading to highly accurate material process. In this review, we briefly outline the application modification1. Thus, by focusing ultrashort pulses onto areas of AO for laser processing before considering the 1234567890():,; 1234567890():,; 1234567890():,; 1234567890():,; the surface of the workpiece, precise cuts and holes can be methods of AO, including the range of adaptive elements manufactured with a minimal heat-affected zone. -
A Curriculum Guide
FOCUS ON PHOTOGRAPHY: A CURRICULUM GUIDE This page is an excerpt from Focus on Photography: A Curriculum Guide Written by Cynthia Way for the International Center of Photography © 2006 International Center of Photography All rights reserved. Published by the International Center of Photography, New York. Printed in the United States of America. Please credit the International Center of Photography on all reproductions. This project has been made possible with generous support from Andrew and Marina Lewin, the GE Fund, and public funds from the New York City Department of Cultural Affairs Cultural Challenge Program. FOCUS ON PHOTOGRAPHY: A CURRICULUM GUIDE PART IV Resources FOCUS ON PHOTOGRAPHY: A CURRICULUM GUIDE This section is an excerpt from Focus on Photography: A Curriculum Guide Written by Cynthia Way for the International Center of Photography © 2006 International Center of Photography All rights reserved. Published by the International Center of Photography, New York. Printed in the United States of America. Please credit the International Center of Photography on all reproductions. This project has been made possible with generous support from Andrew and Marina Lewin, the GE Fund, and public funds from the New York City Department of Cultural Affairs Cultural Challenge Program. FOCUS ON PHOTOGRAPHY: A CURRICULUM GUIDE Focus Lesson Plans Fand Actvities INDEX TO FOCUS LINKS Focus Links Lesson Plans Focus Link 1 LESSON 1: Introductory Polaroid Exercises Focus Link 2 LESSON 2: Camera as a Tool Focus Link 3 LESSON 3: Photographic Field -
A Theoretical and Practical Introduction to Optics a Theoretical and Practical Introduction to Optics
White Paper A Theoretical and Practical Introduction to Optics A Theoretical and Practical Introduction to Optics Be honest: do you really know how to calculate the focal length of a lens? If so, you are an exception to the rule and can stop reading here !! For the rest of you, here is a second chance. Back to square one "Piece of broken glass starts forest fire"– a common headline during the summer. But how could this have happened? Due to the enormous distance between the Earth and the Sun, the Sun only appears as a tiny point emitting parallel rays of light (figure 1a) Should these parallel rays pass through a lens (or a piece of glass, which has similar characteristics) the rays would meet behind the lens at what is called the focal point. But what happens if our point of light is so near to the lens that we can not assume to have parallel rays of light? They cross each other behind the focal point (figure 1b). If we take a look at the image of our point of light at the focal points position we will see a unclear blurred spot. And so the question arises- "what is focusing?". Focusing is to increase the distance between the focal plane and the lens until the focal plane and the junction of the rays overlap each other (figure 1c). Thus, for single points of light the situation is quite simple. But what happens to the image of screws, PCBs or plates of steel? From points of light to images A point of light does not necessarily originate directly from the sun, candles or lamps, it can also result from a reflection. -
Mission to the Solar Gravity Lens Focus: Natural Highground for Imaging Earth-Like Exoplanets L
Planetary Science Vision 2050 Workshop 2017 (LPI Contrib. No. 1989) 8203.pdf MISSION TO THE SOLAR GRAVITY LENS FOCUS: NATURAL HIGHGROUND FOR IMAGING EARTH-LIKE EXOPLANETS L. Alkalai1, N. Arora1, M. Shao1, S. Turyshev1, L. Friedman8 ,P. C. Brandt3, R. McNutt3, G. Hallinan2, R. Mewaldt2, J. Bock2, M. Brown2, J. McGuire1, A. Biswas1, P. Liewer1, N. Murphy1, M. Desai4, D. McComas5, M. Opher6, E. Stone2, G. Zank7, 1Jet Propulsion Laboratory, Pasadena, CA 91109, USA, 2California Institute of Technology, Pasadena, CA 91125, USA, 3The Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723, USA,4Southwest Research Institute, San Antonio, TX 78238, USA, 5Princeton Plasma Physics Laboratory, Princeton, NJ 08543, USA, 6Boston University, Boston, MA 02215, USA, 7University of Alabama in Huntsville, Huntsville, AL 35899, USA, 8Emritus, The Planetary Society. Figure 1: A SGL Probe Mission is a first step in the goal to search and study potential habitable exoplanets. This figure was developed as a product of two Keck Institute for Space Studies (KISS) workshops on the topic of the “Science and Enabling Technologies for the Exploration of the Interstellar Medium” led by E. Stone, L. Alkalai and L. Friedman. Introduction: Recent data from Voyager 1, Kepler and New Horizons spacecraft have resulted in breath-taking discoveries that have excited the public and invigorated the space science community. Voyager 1, the first spacecraft to arrive at the Heliopause, discovered that Fig. 2. Imaging of an exo-Earth with solar gravitational Lens. The exo-Earth occupies (1km×1km) area at the image plane. Using a 1m the interstellar medium is far more complicated and telescope as a 1 pixel detector provides a (1000×1000) pixel image! turbulent than expected; the Kepler telescope According to Einstein’s general relativity, gravity discovered that exoplanets are not only ubiquitous but induces refractive properties of space-time causing a also diverse in our galaxy and that Earth-like exoplanets massive object to act as a lens by bending light. -
Camera Settings Guide
Camera Settings Guide • " " and " " are trademarks or registered trademarks of Sony Corporation. • All other company and product names mentioned herein are used for identification purposes only and may be the trademarks or registered trademarks of their respective owners. TM and ® symbols are not included in this booklet. • Screen displays and effects used to illustrate some functions are simulated. Conventional autofocus has until now dealt with space alone. Sony goes one step further — a big step, with an innovative image sensor that picks up both space and time to capture moving subjects with new clarity. Sony spells the beginning of a new autofocus era. 4D FOCUS allows you to take crisper photos than ever. Plain old autofocus is a thing of the past. The future of photography is in motion. What is 4D FOCUS? Space: 3D Time: 4D 4D FOCUS Area Depth Time Wide Fast Steadfast The wide AF area, covering nearly the Fast Hybrid AF, combining phase- An advanced AF algorithm accurately entire frame, allows focusing on a detection AF and contrast-detection AF, predicts subject’s next move. Precise AF subject positioned even off the center instantly detects distance to the subject tracking allows focus to be maintained of the frame. to focus accurately. even on fast-moving subjects. Meeting your focusing demands Basic AF performance of Wide Fast Steadfast Focusing over wide area Instant focusing! Once it's focused, it never lets go The 6000 employs a focal plane phase- Advanced Fast Hybrid AF combines phase- With Focus Mode set to AF-C, the camera detection AF sensor with 179 AF points spread detection AF and contrast-detection AF to achieve displays one or more small green frames to cover nearly the entire frame. -
Longitudinal Chromatic Aberration
Longitudinal Chromatic Aberration Red focus Blue focus LCA Transverse Chromatic Aberration Decentered pupil Transverse Chromatic Aberration Chromatic Difference of Refraction Atchison and Smith, JOSA A, 2005 Why is LCA not really a problem? Chromatic Aberration Halos (LCA) Fringes (TCA) www.starizona.com digitaldailydose.wordpress.com Red-Green Duochrome test • If the letters on the red side stand out more, add minus power; if the letters on the green side stand out more, add plus power. • Neutrality is reached when the letters on both backgrounds appear equally distinct. Colligon-Bradley P. J Ophthalmic Nurs Technol. 1992 11(5):220-2. Transverse Chromatic Aberration Lab #7 April 15th Look at a red and blue target through a 1 mm pinhole. Move the pinhole from one edge of the pupil to the other. What happens to the red and blue images? Chromatic Difference of Magnification Chief ray Aperture stop Off axis source Abbe Number • Also known as – Refractive efficiency – nu-value –V-value –constringence Refractive efficiencies for common materials water 55.6 alcohol 60.6 ophthalmic crown glass 58.6 polycarbonate 30.0 dense flint glass 36.6 Highlite glass 31.0 BK7 64.9 Example • Given the following indices of refraction for BK7 glass (nD = 1.519; nF = 1.522; nC = 1.514) what is the refractive efficiency? • What is the chromatic aberration of a 20D thin lens made of BK7 glass? Problem • Design a 10.00 D achromatic doublet using ophthalmic crown glass and dense flint glass Carl Friedrich Gauss 1777-1855 Heinrich Seidel 1842-1906 Approximations to -
31 the Superachromat
Lesson 31: The Superachromat This lesson will explore a unique feature of SYNOPSYS that can be helpful when you need exceptional color correction, better even than an apochromat. Lesson 8 in this Online Tutorial showed how to select three glass types that make it possible to correct axial color at three wavelengths. For many tasks, that is as good as you will need. But not always. Suppose you are designing a lens to be used over the range 0.4 to 0.9 um. Can you do it with an apochromat? Let’s find out. Here is the RLE file for a starting system, where all surfaces are flat except for the last, which will give us an F/8 telescope objective of 6-inch aperture. (Copy these lines and paste them into the MACro editor.) RLE ID WIDE SPECTRAL RANGE EXAMPLE OBB 0 .25 3 UNITS INCH 1 GLM 1.6 50 3 GLM 1.6 50 5 GLM 1.6 50 6 UMC -0.0625 YMT 7 1 TH .6 2 TH .1 3 TH .6 4 TH .1 5 TH .6 END We did not specify the wavelengths yet, so we get the default CdF lines. We need to change this. Open the Spectrum Wizard (MSW), and change the points indicated. 1 After clicking the Get Spectrum button, click the Apply to lens button. Our lens now has a wider spectrum. Here is our starting lens, in the SketchPad display Uggh! Yes, it’s really awful. Let’s optimize it, varying the glass models. Make a MACro: LOG STO 9 PANT VLIST RAD 1 2 3 4 5 VLIST TH ALL AIR VLIST GLM ALL END AANT END SNAP SYNOPSYS 50 Now put the cursor on the blank line after the AANT command, and click the button . -
Optical Performance Factors
1ch_FundamentalOptics_Final_a.qxd 6/15/2009 2:28 PM Page 1.11 Fundamental Optics www.cvimellesgriot.com Fundamental Optics Performance Factors After paraxial formulas have been used to select values for component focal length(s) and diameter(s), the final step is to select actual lenses. As in any engineering problem, this selection process involves a number of tradeoffs, wavelength l including performance, cost, weight, and environmental factors. The performance of real optical systems is limited by several factors, material 1 including lens aberrations and light diffraction. The magnitude of these index n 1 effects can be calculated with relative ease. Gaussian Beam Optics v Numerous other factors, such as lens manufacturing tolerances and 1 component alignment, impact the performance of an optical system. Although these are not considered explicitly in the following discussion, it should be kept in mind that if calculations indicate that a lens system only just meets the desired performance criteria, in practice it may fall short material 2 v2 of this performance as a result of other factors. In critical applications, index n 2 it is generally better to select a lens whose calculated performance is significantly better than needed. DIFFRACTION Figure 1.14 Refraction of light at a dielectric boundary Diffraction, a natural property of light arising from its wave nature, poses a fundamental limitation on any optical system. Diffraction is always Optical Specifications present, although its effects may be masked if the system has significant aberrations. When an optical system is essentially free from aberrations, its performance is limited solely by diffraction, and it is referred to as diffraction limited.