Bubble Optics
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Observation of Elliptically Polarized Light from Total Internal Reflection in Bubbles
Observation of elliptically polarized light from total internal reflection in bubbles Item Type Article Authors Miller, Sawyer; Ding, Yitian; Jiang, Linan; Tu, Xingzhou; Pau, Stanley Citation Miller, S., Ding, Y., Jiang, L. et al. Observation of elliptically polarized light from total internal reflection in bubbles. Sci Rep 10, 8725 (2020). https://doi.org/10.1038/s41598-020-65410-5 DOI 10.1038/s41598-020-65410-5 Publisher NATURE PUBLISHING GROUP Journal SCIENTIFIC REPORTS Rights Copyright © The Author(s) 2020. Open Access This article is licensed under a Creative Commons Attribution 4.0 International License. Download date 29/09/2021 02:08:57 Item License https://creativecommons.org/licenses/by/4.0/ Version Final published version Link to Item http://hdl.handle.net/10150/641865 www.nature.com/scientificreports OPEN Observation of elliptically polarized light from total internal refection in bubbles Sawyer Miller1,2 ✉ , Yitian Ding1,2, Linan Jiang1, Xingzhou Tu1 & Stanley Pau1 ✉ Bubbles are ubiquitous in the natural environment, where diferent substances and phases of the same substance forms globules due to diferences in pressure and surface tension. Total internal refection occurs at the interface of a bubble, where light travels from the higher refractive index material outside a bubble to the lower index material inside a bubble at appropriate angles of incidence, which can lead to a phase shift in the refected light. Linearly polarized skylight can be converted to elliptically polarized light with efciency up to 53% by single scattering from the water-air interface. Total internal refection from air bubble in water is one of the few sources of elliptical polarization in the natural world. -
A Monte Carlo Ray Tracing Study of Polarized Light Propagation in Liquid Foams
ARTICLE IN PRESS Journal of Quantitative Spectroscopy & Radiative Transfer 104 (2007) 277–287 www.elsevier.com/locate/jqsrt A Monte Carlo ray tracing study of polarized light propagation in liquid foams J.N. Swamya,Ã, Czarena Crofchecka, M. Pinar Mengu¨c- b,ÃÃ aDepartment of Biosystems and Agricultural Engineering, 128 C E Barnhart Building, University of Kentucky, Lexington, KY 40546, USA bDepartment of Mechanical Engineering, 269 Ralph G. Anderson Building, University of Kentucky, Lexington, KY 40506, USA Received 10 July 2006; accepted 28 July 2006 Abstract A Monte Carlo ray tracing scheme is used to investigate the propagation of an incident collimated beam of polarized light in liquid foams. Cellular structures like foam are expected to change the polarization characteristics due to multiple scattering events, where such changes can be used to monitor foam dynamics. A statistical model utilizing some of the recent developments in foam physics is coupled with a vector Monte Carlo scheme to compute the depolarization ratios via Stokes–Mueller formalism. For the simulations, the incident Stokes vector corresponding to horizontal linear polarization and right circular polarization are considered. It is observed that bubble size and the polydispersity parameter have a significant effect on the depolarization ratios. This is partially owing to the number of total internal reflection events in the Plateau borders. The results are discussed in terms of applicability of polarized light as a diagnostic tool for monitoring foams. r 2006 Elsevier Ltd. All rights reserved. Keywords: Polarized light scattering; Liquid foams; Bubble size; Polydispersity; Foam characterization; Foam diagnostics; Cellular structures 1. Introduction Liquid foams are random packing of bubbles in a small amount of immiscible liquid [1] and can be found in a wide variety of applications. -
The Synergistic Effect of Focused Ultrasound and Biophotonics to Overcome the Barrier of Light Transmittance in Biological Tissue
Photodiagnosis and Photodynamic Therapy 33 (2021) 102173 Contents lists available at ScienceDirect Photodiagnosis and Photodynamic Therapy journal homepage: www.elsevier.com/locate/pdpdt The synergistic effect of focused ultrasound and biophotonics to overcome the barrier of light transmittance in biological tissue Jaehyuk Kim a,b, Jaewoo Shin c, Chanho Kong c, Sung-Ho Lee a, Won Seok Chang c, Seung Hee Han a,d,* a Molecular Imaging, Princess Margaret Cancer Centre, Toronto, ON, Canada b Health and Medical Equipment, Samsung Electronics Co. Ltd., Suwon, Republic of Korea c Department of Neurosurgery, Brain Research Institute, Yonsei University College of Medicine, Seoul, Republic of Korea d Department of Medical Biophysics, University of Toronto, Toronto, ON, Canada ARTICLE INFO ABSTRACT Keywords: Optical technology is a tool to diagnose and treat human diseases. Shallow penetration depth caused by the high Light transmission enhancement optical scattering nature of biological tissues is a significantobstacle to utilizing light in the biomedical field. In Focused Ultrasound this paper, light transmission enhancement in the rat brain induced by focused ultrasound (FUS) was observed Air bubble and the cause of observed enhancement was analyzed. Both air bubbles and mechanical deformation generated Mechanical deformation by FUS were cited as the cause. The Monte Carlo simulation was performed to investigate effects on transmission Rat brain by air bubbles and finiteelement method was also used to describe mechanical deformation induced by motions of acoustic particles. As a result, it was found that the mechanical deformation was more suitable to describe the transmission change according to the FUS pulse observed in the experiment. 1. -
Ocean Storage
277 6 Ocean storage Coordinating Lead Authors Ken Caldeira (United States), Makoto Akai (Japan) Lead Authors Peter Brewer (United States), Baixin Chen (China), Peter Haugan (Norway), Toru Iwama (Japan), Paul Johnston (United Kingdom), Haroon Kheshgi (United States), Qingquan Li (China), Takashi Ohsumi (Japan), Hans Pörtner (Germany), Chris Sabine (United States), Yoshihisa Shirayama (Japan), Jolyon Thomson (United Kingdom) Contributing Authors Jim Barry (United States), Lara Hansen (United States) Review Editors Brad De Young (Canada), Fortunat Joos (Switzerland) 278 IPCC Special Report on Carbon dioxide Capture and Storage Contents EXECUTIVE SUMMARY 279 6.7 Environmental impacts, risks, and risk management 298 6.1 Introduction and background 279 6.7.1 Introduction to biological impacts and risk 298 6.1.1 Intentional storage of CO2 in the ocean 279 6.7.2 Physiological effects of CO2 301 6.1.2 Relevant background in physical and chemical 6.7.3 From physiological mechanisms to ecosystems 305 oceanography 281 6.7.4 Biological consequences for water column release scenarios 306 6.2 Approaches to release CO2 into the ocean 282 6.7.5 Biological consequences associated with CO2 6.2.1 Approaches to releasing CO2 that has been captured, lakes 307 compressed, and transported into the ocean 282 6.7.6 Contaminants in CO2 streams 307 6.2.2 CO2 storage by dissolution of carbonate minerals 290 6.7.7 Risk management 307 6.2.3 Other ocean storage approaches 291 6.7.8 Social aspects; public and stakeholder perception 307 6.3 Capacity and fractions retained -
Bubble-Mania the Bubbling Clues to Magma Viscosity and Eruptions
Earthlearningidea - http://www.earthlearningidea.com/ Bubble-mania The bubbling clues to magma viscosity and eruptions Pour a viscous liquid (eg. honey, syrup) into Honey and a one transparent container and a pale-coloured soft drink – ready for soft drink (eg. ginger beer) or just coloured bubble-mania. water into another. Put both of these onto a plastic tray or table. Ask your pupils to use a drinking straw to blow bubbles into the soft Apparatus photo: drink, then ask them to ‘use the same blow’ to Chris King blow bubbles in the more viscous liquid. When nothing happens, ask them to blow harder until the liquid ‘erupts’. Ask: • How were the ‘eruptions’ different? • How were the bubbles different? • What caused the differences? • Some volcanoes have magmas that are Magma fountain ‘runny’ (like the soft drink) and some have within the crater much more viscous magmas (like the other of Volcan liquid) – how might these volcanoes erupt Villarrica, Pucón, differently? Chile. • Which sort of eruption would you most like to This file is see – one with low viscosity (runny) magma, licensed by Jonathan Lewis like the soft drink, or one with high viscosity under the Creative (thick) magma like the viscous liquid? Commons Attribution-Share Alike 2.0 Generic license. ……………………………………………………………………………………………………………………………… The back up Title: Bubble-mania • How were the ‘eruptions’ different? It was easy to blow bubbles into the soft drink Subtitle: The bubbling clues to magma viscosity and it ‘fizzed’ a bit, but the bubbles soon and eruptions disappeared; it was much harder to blow bubbles into the viscous liquid and they grew Topic: A simple test of the viscosity of two similar- large and sometimes burst out of the container looking liquids, linked to volcanic eruption style. -
Beam Expander Basics: Not All Spots Are Created Equal
LEARNING – UNDERSTANDING – INTRODUCING – APPLYING Beam Expander Basics: Not All Spots Are Created Equal APPLICATION NOTES www.edmundoptics.com BEAM EXPANDERS A laser beam expander is designed to increase the diameter from well-established optical telescope fundamentals. In such of a collimated input beam to a larger collimated output beam. systems, the object rays, located at infinity, enter parallel to Beam expanders are used in applications such as laser scan- the optical axis of the internal optics and exit parallel to them ning, interferometry, and remote sensing. Contemporary laser as well. This means that there is no focal length to the entire beam expander designs are afocal systems that developed system. THEORY: TELESCOPES Optical telescopes, which have classically been used to view eye, or image created, is called the image lens. distant objects such as celestial bodies in outer space, are di- vided into two types: refracting and reflecting. Refracting tele- A Galilean telescope consists of a positive lens and a negative scopes utilize lenses to refract or bend light while reflecting lens that are also separated by the sum of their focal length telescopes utilize mirrors to reflect light. (Figure 2). However, since one of the lenses is negative, the separation distance between the two lenses is much shorter Refracting telescopes fall into two categories: Keplerian and than in the Keplerian design. Please note that using the Effec- Galilean. A Keplerian telescope consists of positive focal length tive Focal Length of the two lenses will give a good approxima- lenses that are separated by the sum of their focal lengths (Fig- tion of the total length, while using the Back Focal Length will ure 1). -
The Life of a Surface Bubble
molecules Review The Life of a Surface Bubble Jonas Miguet 1,†, Florence Rouyer 2,† and Emmanuelle Rio 3,*,† 1 TIPS C.P.165/67, Université Libre de Bruxelles, Av. F. Roosevelt 50, 1050 Brussels, Belgium; [email protected] 2 Laboratoire Navier, Université Gustave Eiffel, Ecole des Ponts, CNRS, 77454 Marne-la-Vallée, France; fl[email protected] 3 Laboratoire de Physique des Solides, CNRS, Université Paris-Saclay, 91405 Orsay, France * Correspondence: [email protected]; Tel.: +33-1691-569-60 † These authors contributed equally to this work. Abstract: Surface bubbles are present in many industrial processes and in nature, as well as in carbon- ated beverages. They have motivated many theoretical, numerical and experimental works. This paper presents the current knowledge on the physics of surface bubbles lifetime and shows the diversity of mechanisms at play that depend on the properties of the bath, the interfaces and the ambient air. In particular, we explore the role of drainage and evaporation on film thinning. We highlight the existence of two different scenarios depending on whether the cap film ruptures at large or small thickness compared to the thickness at which van der Waals interaction come in to play. Keywords: bubble; film; drainage; evaporation; lifetime 1. Introduction Bubbles have attracted much attention in the past for several reasons. First, their ephemeral Citation: Miguet, J.; Rouyer, F.; nature commonly awakes children’s interest and amusement. Their visual appeal has raised Rio, E. The Life of a Surface Bubble. interest in painting [1], in graphism [2] or in living art. -
Study on Bubble Cavitation in Liquids for Bubbles Arranged in a Columnar Bubble Group
applied sciences Article Study on Bubble Cavitation in Liquids for Bubbles Arranged in a Columnar Bubble Group Peng-li Zhang 1,2 and Shu-yu Lin 1,* 1 Institute of Applied Acoustics, Shaanxi Normal University, Xi’an 710062, China; [email protected] 2 College of Science, Xi’an University of Science and Technology, Xi’an 710054, China * Correspondence: [email protected]; Tel.: +86-181-9273-7031 Received: 24 October 2019; Accepted: 29 November 2019; Published: 4 December 2019 Featured Application: This work will provide a reference for further simulations and help to promote the theoretical study of ultrasonic cavitation bubbles. Abstract: In liquids, bubbles usually exist in the form of bubble groups. Due to their interaction with other bubbles, the resonance frequency of bubbles decreases. In this paper, the resonance frequency of bubbles in a columnar bubble group is obtained by linear simplification of the bubbles’ dynamic equation. The correction coefficient between the resonance frequency of the bubbles in the columnar bubble group and the Minnaert frequency of a single bubble is given. The results show that the resonance frequency of bubbles in the bubble group is affected by many parameters such as the initial radius of bubbles, the number of bubbles in the bubble group, and the distance between bubbles. The initial radius of the bubbles and the distance between bubbles are found to have more significant influence on the resonance frequency of the bubbles. When the distance between bubbles increases to 20 times the bubbles’ initial radius, the coupling effect between bubbles can be ignored, and after that the bubbles’ resonance frequency in the bubble group tends to the resonance frequency of a single bubble’s resonance frequency. -
Head Mounted Display Optics II
Head Mounted Display Optics II Gordon Wetzstein Stanford University EE 267 Virtual Reality Lecture 8 stanford.edu/class/ee267/ Lecture Overview • focus cues & the vergence-accommodation conflict • advanced optics for VR with focus cues: • gaze-contingent varifocal displays • volumetric and multi-plane displays • near-eye light field displays • Maxwellian-type displays • AR displays Magnified Display • big challenge: virtual image appears at fixed focal plane! d • no focus cues d’ f 1 1 1 + = d d ' f Importance of Focus Cues Decreases with Age - Presbyopia 0D (∞cm) 4D (25cm) 8D (12.5cm) 12D (8cm) Nearest focus distance focus Nearest 16D (6cm) 8 16 24 32 40 48 56 64 72 Age (years) Duane, 1912 Cutting & Vishton, 1995 Relative Importance of Depth Cues The Vergence-Accommodation Conflict (VAC) Real World: Vergence & Accommodation Match! Current VR Displays: Vergence & Accommodation Mismatch Accommodation and Retinal Blur Blur Gradient Driven Accommodation Blur Gradient Driven Accommodation Blur Gradient Driven Accommodation Blur Gradient Driven Accommodation Blur Gradient Driven Accommodation Blur Gradient Driven Accommodation Top View Real World: Vergence & Accommodation Match! Top View Screen Stereo Displays Today (including HMDs): Vergence-Accommodation Mismatch! Consequences of Vergence-Accommodation Conflict • Visual discomfort (eye tiredness & eyestrain) after ~20 minutes of stereoscopic depth judgments (Hoffman et al. 2008; Shibata et al. 2011) • Degrades visual performance in terms of reaction times and acuity for stereoscopic vision -
A Simple but Precise Method for Quantitative Measurement of the Quality of the Laser Focus in a Scanning Optical Microscope
Journal of Microscopy, Vol. 00, Issue 0 2015, pp. 1–8 doi: 10.1111/jmi.12249 Received 3 December 2014; accepted 24 February 2015 A simple but precise method for quantitative measurement of the quality of the laser focus in a scanning optical microscope J. Trag¨ ardh˚ ∗,K.MacRae∗,†,C.Travis†,R.Amor∗, G. Norris∗, S.H. Wilson∗,†, G.-L. Oppo† & G. McConnell∗ ∗Centre for Biophotonics, Strathclyde Institute for Pharmacy and Biomedical Sciences, University of Strathclyde, Glasgow, U.K †Department of Physics, University of Strathclyde, Glasgow, U.K Key words. Beam characterization, knife-edge measurement, microscopy, resolution. Summary distinguish between fine details of a specimen. According to the Abbe equation, modified by Rayleigh, the lateral resolution We report a method for characterizing the focussing laser r is given by beam exiting the objective in a laser scanning microscope. lat This method provides the size of the optical focus, the diver- 0.61λ r = , (1) gence of the beam, the ellipticity and the astigmatism. We use lat N.A. a microscopic-scale knife edge in the form of a simple trans- mission electron microscopy grid attached to a glass micro- while the axial resolution rax is given by scope slide, and a light-collecting optical fibre and photodiode 2nλ underneath the specimen. By scanning the laser spot from a rax = , (2) (N.A.)2 reflective to a transmitting part of the grid, a beam profile in the form of an error function can be obtained and by repeating where λ is the wavelength, n is the refractive index and N.A. -
Chapter 4 Light and Optics
Chapter 4 Light and Optics Steven M. LaValle University of Oulu Copyright Steven M. LaValle 2019 Available for downloading at http://vr.cs.uiuc.edu/ 98 S. M. LaValle: Virtual Reality Chapter 4 Light and Optics Knowing how light propagates in the physical world is crucial to understanding VR. One reason is the interface between visual displays and our eyes. Light is emitted from displays and arrives on our retinas in a way that convincingly Figure 4.1: Waves and visibility rays emanating from a point light source. reproduces how light arrives through normal vision in the physical world. In the current generation of VR headsets, a system of both engineered and natural lenses (parts of our eyes) guide the light. Another reason to study light propagation is 2. Waves: Ripples through space that are similar to waves propagating on the the construction of virtual worlds. Chapter 3 covered purely geometric aspects surface of water, but are 3D. The wavelength is the distance between peaks. of modeling. The next logical step is to model the physics of light propagation This interpretation is helpful when considering the spectrum of colors. through virtual worlds; this will be continued in Chapter 7, which describes what should be rendered on the visual display. Finally, light propagation is also helpful 3. Rays: A ray traces the motion of a single hypothetical photon. The direction to understanding how cameras work, which provides another way present a virtual is perpendicular to the wavefronts (see Figure 4.1). This interpretation is world: Through panoramic videos. Cameras are also important for tracking, which helpful when explaining lenses and defining the concept of visibility. -
May 2019 OBSERVER
THE OBSERVER OF THE TWIN CITY AMATEUR ASTRONOMERS Volume 44, Number 5 May 2019 INSIDE THIS ISSUE: 1«Editor’s Choice: Image of the Month – Leo Triplet 2«President’s Note 3«Calendar of Celestial Events – May 2019 3«New & Renewing Members/Dues Blues/E-Mail List 4«This Month’s Phases of the Moon 4«This Month’s Solar Phenomena 4«AstroBits – News from Around the TCAA 5«E/PO for April 2019 5«TCAA Image Gallery 9«WentZel and Wenning at NEAF 11«May 2019 with Jeffrey L. Hunt 12«Throwback Thursday 16«Public Viewing Sessions Schedule for 2019 17«TCAA Calendar of Events for 2019 18«TCAA Treasurer’s Report as of April 29, 2019 19«Renewing Your TCAA Membership 19«TCAA Active on Facebook IMAGE OF THE MONTH: EDITOR’S CHOICE – LEO TRIPLET This month’s image was produced by Tim Stone. Tim writes: This famous triplet of galaxies is known as ‘The Leo Trio,’ a catchy name for a wildly unlikely group of three large galaxies: M65, M66, and NGC 3628. All three are interacting with each other, and are quite close to each other, at least as far as large galaxies go. M65 and 66 are about 160,000 light years apart, about the same as the distance between us and the Magellanic Clouds. Imagine the view of each other these two galaxies enjoy! NGC 3628 is a bit farther from the two, about 300,000 years. If we think our view of M31 is unbelievable, suitably positioned astronomers in these galaxies enjoy a vastly superior view of their neighbors! M66 has been deeply disrupted by the interactions with its two neighbors.