Atmospheric Optical Phenomena
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Enhanced Total Internal Reflection Using Low-Index Nanolattice Materials
Letter Vol. 42, No. 20 / October 15 2017 / Optics Letters 4123 Enhanced total internal reflection using low-index nanolattice materials XU A. ZHANG,YI-AN CHEN,ABHIJEET BAGAL, AND CHIH-HAO CHANG* Department of Mechanical and Aerospace Engineering, North Carolina State University, Raleigh, North Carolina 27695, USA *Corresponding author: [email protected] Received 4 August 2017; revised 14 September 2017; accepted 16 September 2017; posted 19 September 2017 (Doc. ID 303972); published 9 October 2017 Low-index materials are key components in integrated Although naturally occurring materials with low refractive photonics and can enhance index contrast and improve per- indices are limited, there are significant research efforts to formance. Such materials can be constructed from porous artificially create low-index materials close to the index of materials, which generally lack mechanical strength and air. These new materials consist of porous structures through are difficult to integrate. Here we demonstrate enhanced to- various conventional fabrication techniques, such as oblique tal internal reflection (TIR) induced by integrating robust deposition [5–9], the sol-gel process [10], and chemical vapor nanolattice materials with periodic architectures between deposition [11]. Due to the air voids, the fabricated porous high-index media. The transmission measurement from structures can have effective refractive indices lower than the the multilayer stack illustrates a cutoff at about a 60° inci- solid material components. However, such materials typically dence angle, indicating an enhanced light trapping effect lack mechanical stability and can induce optical scattering be- through TIR. Light propagation in the nanolattice material cause of the random architectures of the structures. -
Moons Phases and Tides
Moon’s Phases and Tides Moon Phases Half of the Moon is always lit up by the sun. As the Moon orbits the Earth, we see different parts of the lighted area. From Earth, the lit portion we see of the moon waxes (grows) and wanes (shrinks). The revolution of the Moon around the Earth makes the Moon look as if it is changing shape in the sky The Moon passes through four major shapes during a cycle that repeats itself every 29.5 days. The phases always follow one another in the same order: New moon Waxing Crescent First quarter Waxing Gibbous Full moon Waning Gibbous Third (last) Quarter Waning Crescent • IF LIT FROM THE RIGHT, IT IS WAXING OR GROWING • IF DARKENING FROM THE RIGHT, IT IS WANING (SHRINKING) Tides • The Moon's gravitational pull on the Earth cause the seas and oceans to rise and fall in an endless cycle of low and high tides. • Much of the Earth's shoreline life depends on the tides. – Crabs, starfish, mussels, barnacles, etc. – Tides caused by the Moon • The Earth's tides are caused by the gravitational pull of the Moon. • The Earth bulges slightly both toward and away from the Moon. -As the Earth rotates daily, the bulges move across the Earth. • The moon pulls strongly on the water on the side of Earth closest to the moon, causing the water to bulge. • It also pulls less strongly on Earth and on the water on the far side of Earth, which results in tides. What causes tides? • Tides are the rise and fall of ocean water. -
Light, Color, and Atmospheric Optics
Light, Color, and Atmospheric Optics GEOL 1350: Introduction To Meteorology 1 2 • During the scattering process, no energy is gained or lost, and therefore, no temperature changes occur. • Scattering depends on the size of objects, in particular on the ratio of object’s diameter vs wavelength: 1. Rayleigh scattering (D/ < 0.03) 2. Mie scattering (0.03 ≤ D/ < 32) 3. Geometric scattering (D/ ≥ 32) 3 4 • Gas scattering: redirection of radiation by a gas molecule without a net transfer of energy of the molecules • Rayleigh scattering: absorption extinction 4 coefficient s depends on 1/ . • Molecules scatter short (blue) wavelengths preferentially over long (red) wavelengths. • The longer pathway of light through the atmosphere the more shorter wavelengths are scattered. 5 • As sunlight enters the atmosphere, the shorter visible wavelengths of violet, blue and green are scattered more by atmospheric gases than are the longer wavelengths of yellow, orange, and especially red. • The scattered waves of violet, blue, and green strike the eye from all directions. • Because our eyes are more sensitive to blue light, these waves, viewed together, produce the sensation of blue coming from all around us. 6 • Rayleigh Scattering • The selective scattering of blue light by air molecules and very small particles can make distant mountains appear blue. The blue ridge mountains in Virginia. 7 • When small particles, such as fine dust and salt, become suspended in the atmosphere, the color of the sky begins to change from blue to milky white. • These particles are large enough to scatter all wavelengths of visible light fairly evenly in all directions. -
ESSENTIALS of METEOROLOGY (7Th Ed.) GLOSSARY
ESSENTIALS OF METEOROLOGY (7th ed.) GLOSSARY Chapter 1 Aerosols Tiny suspended solid particles (dust, smoke, etc.) or liquid droplets that enter the atmosphere from either natural or human (anthropogenic) sources, such as the burning of fossil fuels. Sulfur-containing fossil fuels, such as coal, produce sulfate aerosols. Air density The ratio of the mass of a substance to the volume occupied by it. Air density is usually expressed as g/cm3 or kg/m3. Also See Density. Air pressure The pressure exerted by the mass of air above a given point, usually expressed in millibars (mb), inches of (atmospheric mercury (Hg) or in hectopascals (hPa). pressure) Atmosphere The envelope of gases that surround a planet and are held to it by the planet's gravitational attraction. The earth's atmosphere is mainly nitrogen and oxygen. Carbon dioxide (CO2) A colorless, odorless gas whose concentration is about 0.039 percent (390 ppm) in a volume of air near sea level. It is a selective absorber of infrared radiation and, consequently, it is important in the earth's atmospheric greenhouse effect. Solid CO2 is called dry ice. Climate The accumulation of daily and seasonal weather events over a long period of time. Front The transition zone between two distinct air masses. Hurricane A tropical cyclone having winds in excess of 64 knots (74 mi/hr). Ionosphere An electrified region of the upper atmosphere where fairly large concentrations of ions and free electrons exist. Lapse rate The rate at which an atmospheric variable (usually temperature) decreases with height. (See Environmental lapse rate.) Mesosphere The atmospheric layer between the stratosphere and the thermosphere. -
Atmospheric Optics Learning Module
Atmospheric Optics Learning Module Everything we see is the reflection of light and without light, everything would be dark. In this learning module, we will discuss the various wavelengths of light and how it is transmitted through Earth’s atmosphere to explain fascinating optical phenomena including why the sky is blue and how rainbows form! To get started, watch this video describing energy in the form of waves. A sundog and halo display in Greenland. Electromagnetic Spectrum (0 – 6:30) Source Electromagnetic Spectrum Electromagnetic (EM) radiation is light. Light you might see in a rainbow, or better yet, a double rainbow such as the one seen in Figure 1. But it is also radio waves, x-rays, and gamma rays. It is incredibly important because there are only two ways we can move energy from place to place. The first is using what is called a particle, or an object moving from place to place. The second way to move energy is through a wave. The interesting thing about EM radiation is that it is both a particle and a wave 1. Figure 1. Double rainbow Source 1 Created by Tyra Brown, Nicole Riemer, Eric Snodgrass and Anna Ortiz at the University of Illinois at Urbana- This work is licensed under a Creative Commons Attribution-ShareAlike 4.0 International License. Champaign. 2015-2016. Supported by the National Science Foundation CAREER Grant #1254428. There are many frequencies of EM radiation that we cannot see. So if we change the frequency, we might have radio waves, which we cannot see, but they are all around us! The same goes for x-rays you might get if you break a bone. -
Atmospheric Optics
53 Atmospheric Optics Craig F. Bohren Pennsylvania State University, Department of Meteorology, University Park, Pennsylvania, USA Phone: (814) 466-6264; Fax: (814) 865-3663; e-mail: [email protected] Abstract Colors of the sky and colored displays in the sky are mostly a consequence of selective scattering by molecules or particles, absorption usually being irrelevant. Molecular scattering selective by wavelength – incident sunlight of some wavelengths being scattered more than others – but the same in any direction at all wavelengths gives rise to the blue of the sky and the red of sunsets and sunrises. Scattering by particles selective by direction – different in different directions at a given wavelength – gives rise to rainbows, coronas, iridescent clouds, the glory, sun dogs, halos, and other ice-crystal displays. The size distribution of these particles and their shapes determine what is observed, water droplets and ice crystals, for example, resulting in distinct displays. To understand the variation and color and brightness of the sky as well as the brightness of clouds requires coming to grips with multiple scattering: scatterers in an ensemble are illuminated by incident sunlight and by the scattered light from each other. The optical properties of an ensemble are not necessarily those of its individual members. Mirages are a consequence of the spatial variation of coherent scattering (refraction) by air molecules, whereas the green flash owes its existence to both coherent scattering by molecules and incoherent scattering -
Einstein's Mirage
Paul L. Schechter Einstein’s Mirage he first prediction of Einstein’s general theoryof relativity T to be verified experimentallywas the deflection of light by a massive body—the Sun. In weak gravitational fields (and for such purposes the Sun’s field is considered weak), light behaves as if there were an index of refraction proportional to the gravitational potential. The stronger the gravitational field, the larger the angu- lar deflection of the light. The Sun is not unique in this regard, and it was quickly appreci- ated that stars in our own galaxy (the MilkyWay) and the combined mass of stars in other galaxies would also, on very rare occasions, produce observable deflections. Variations in the “gravitational” index of refraction would also distort images, stretching them in some directions and shrinking them in others. In the analogous case of terrestrial mirages, the deflections and distortions are due to thermal variations in the index of refraction of air. 36 ) schechter mit physics annual 2003 OTH TERRESTRIAL AND GRAVITATIONAL Bmirages sometimes produce multiple distorted images of the same object. When they do, at least one of the images has the opposite handedness of the object being imaged—it is a mirror image, but distorted. At least one of the other images must have the correct handedness, but it will also be distorted. The French call such distorted images gravitational mirages. In the half century following the confirmation of general relativity, the idea that cosmic mirages might actually be observed was taken seriously byonly a small number of astrophysicists. Most of the papers written on the subject treated them as academic curiosities, far too unlikely to actually be observed. -
Natural Electromagnetic Phenomena and Electromagnetic Theory: a Review
Paper Natural Electromagnetic Phenomena and Electromagnetic Theory: A Review ∗ Masashi Hayakawa Member ∗∗ Katsumi Hattori Member ∗ Yoshiaki Ando Member We review the new findings on natural electromagnetic phenomena in the near-Earth environment and will show the importance of electromagnetic analyses in elucidating the essential points of these phenomena. The topics include (1) atmospheric phenomena related to lightning (e.g. mesospheric optical emissions); (2) seismo-electromagnetic phenomena (electromagnetic phenomena associated with earthquakes and/or volcano eruptions); (3) plasma and wave phenomena in the Earth’s ionosphere and magnetosphere; and (4) electro- magnetic or electrodynamic coupling among different regions. We pay our greatest attention to the unsolved essential problems for each subject, and suggest how electromagnetics would contribute to a solution to those problems. Keywords: Natural electromagnetic phenomena, electromagnetic theory, atmospheric electricity, seismogenic emission, space plasma, computational electromagnetics 1. Introduction We know that the near-Earth environment is occupied by electromagnetic noise over a wide frequency range from DC to VHF (1). Fig. 1 illustrates the frequency spectrum of the terrestrial electromagnetic noise envi- ronment (2). Noises of higher frequency include solar radiation, galactic noise and interplanetary noise, and there are terrestrial noises generated in the near-Earth at lower frequencies. The important electromagnetic phenomena very close to us are summarized as follows: (1) electromagnetic phenomena associated with light- ning discharges in the atmosphere, (2) electromagnetic phenomena in the ionospheric/magnetospheric plasma, and (3) electromagnetic phenomena originating in the lithosphere (1). The first and second phenomena are not so new, but there have been many new discover- ies about them. For example, we have observed a new phenomenon called mesospheric optical emissions asso- ciated with lightning discharges. -
References: Snel's Law and Refraction Index of Refraction For
ESCI 340 - Cloud Physics and Precipitation Processes Lesson 13 - Atmospheric Optical Phenomena Dr. DeCaria References: One of the best sources for information about atmospheric optics is the Atmospheric Optics website, http://www.atoptics.co.uk Snel's Law and Refraction • The index of refraction for a medium is defined as m = c=c;~ (1) where c is the speed of light in a vacuum, andc ~ is the speed of light in the medium.1 • As light passes from one medium into another, there is both reflection and refraction. • Refraction occurs because the wave fronts bend as they cross from one medium into another, causing a ray of light to bend. The ray bends toward the medium that has the slower speed of light (highest index of refraction). • The bending of the ray is quantified by Snel's Law, which is stated mathematically as sin θ m 1 = 2 ; (2) sin θ2 m1 where θ1 is the angle of incidence (and reflection), θ2 is the angle of refraction, and m1 and m2 are the indices of refraction in the two mediums (see Fig. 1). • The amount by which a ray of light is deflected due to refraction can be quantified in one of two ways. { The bending angle, θ0, is the interior angle between the initial and final rays. { The deviation angle, θ00, is the complement of the bending angle, θ00 = 180◦ −θ0. { The relationship between bending angle and deviation angle is illustrated in Fig. 2. Index of Refraction for Air • Light travels faster through warm air than it does through cold air. -
Superior Mirage: Aesthetic Recollections of the Great Lakes
Rochester Institute of Technology RIT Scholar Works Theses 12-2014 Superior Mirage: Aesthetic Recollections of the Great Lakes S Caswell Follow this and additional works at: https://scholarworks.rit.edu/theses Recommended Citation Caswell, S, "Superior Mirage: Aesthetic Recollections of the Great Lakes" (2014). Thesis. Rochester Institute of Technology. Accessed from This Thesis is brought to you for free and open access by RIT Scholar Works. It has been accepted for inclusion in Theses by an authorized administrator of RIT Scholar Works. For more information, please contact [email protected]. Superior Mirage {Aesthetic Recollections of the Great Lakes} By S. Caswell December 2014 A Thesis Submitted in Candidacy for the Degree of Master of Fine Arts-Fine Arts Studio School of Art College of Imaging Arts and Sciences Rochester Institute of Technology Rochester, N.Y. Thesis Approval Superior Mirage By S. Caswell Dr. Tom Lightfoot Date Committee Chair Professor Luvon Sheppard Date Committee Member Professor Elizabeth Kronfield Date Committee Member Acknowledgements I would like to thank the committee of Dr. Tom Lightfoot, Prof. Luvon Sheppard, and Prof. Elizabeth Kronfield for their inspiration, guidance and support in the fruition of this thesis work. Each of your guidance has propelled my work to a higher level due to your individual input and depth of knowledge both artistically and intellectually. This is also the place to thank those who mentored me at Roberts Wesleyan College who were monumental in shaping the way I see as an artist. Thank you to Prof. Scot Bennett, Prof. Douglas Giebel, Prof. Jill Kepler, and Prof Alice Drew. -
Table Talk Succos VOLUME FOUR.Pub
MADE POSSIBLE IN ABLE ALK PART THROUGH A T T GRANT FROM THE STAR-K VAAD OCTOBER 2020 SUCCOS WWW.ACHIM.ORG ISSUE 201 VOLUME 4 HAKASHRUS A MITZVA DILEMMA FOR THE SHABBOS TABLE BALCONY SUCCAH MUSCLE BUILDING We know that everything that happens to us comes from HaShem. When everything in life By Rabbi Yitzi Weiner runs smoothly we ‘understand’ why everything is smooth. However, when life becomes complicated we struggle to understand why HaShem changed His plan. How are we to make sense out of circumstances when they go totally out of control. This question sits on This week is the holiday of Succos. We my mind as we all find ourselves in the middle of Covid and life has spun out of control. all know that on Succos there is a mitz- Although we have no Navi to direct us to the answer, nevertheless, there are clues to vah to live and sleep in a succah in order which we must pay attention. to remember the clouds of glory that pro- Let us leave Covid for a moment and enter the life of a young couple that just had their tected the Jewish people during their trav- third child. Sibling rivalry begins to lift its head and the parents struggle to keep the home els in the desert. This leads us to the fol- peaceful. Nobody is at fault for this challenge; that is how children are programmed. As lowing story. the parents work their way through this challenge, they discover that when they practice Akiva and his family lived in an apart- patience the situation becomes more manageable. -
Analysis of an Infrared Mirage Sequence
Analysis of an infrared mirage sequence Waldemar H. Lehn Infrared observations of seaborne thermal sources are subject to the effects of atmospheric refraction. For low elevation angles at long ranges, out to the limit of visibility, the inevitable atmospheric temper- ature gradients frequently produce mirages. I present an analysis of a 22-min sequence of images recorded on 18 February 1994 at the U.S. Naval Surface Warfare Center at Wallops Island, Virginia. The infrared target is a heat source carried on a ship moving in a straight line toward the camera. The images show a quasi-periodic variation of the horizon elevation, as well as an extended range of visibility. A model that reasonably reproduces the observed features consists of a small temperature inversion in a slightly sloped atmosphere, with an atmospheric gravity wave moving across the line of sight. © 1997 Optical Society of America Key words: Infrared mirage, atmospheric refraction. 1. Introduction ~i! parallel to shore at a nominal bearing angle of 199° All long-range optical observations are affected by toward a fixed station, where the target was a heat refraction in the atmosphere. A well-known exam- source that could be moved up or down a mast ~ele- ple is astronomical refraction that creates a small vations 4.4–26.6 m above mean sea level! and ~ii! apparent vertical displacement of a star or distant directly out to sea at nominal bearing 130°, observing object. Refraction within the surface layer, how- a heat source target on a ship sailing directly toward ever, is not always uniform and on occasion can cause or away from the test site, with two possible target considerable distortion.