Sunlight Bending Through Ice Crystals in Cirriform Clouds
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Atmospheric Optics - II First Midterm Exam Is This Friday!
Atmospheric Optics - II First midterm exam is this Friday! The exam will be in-class, during our regular lecture • this Friday September 28 at 9:30 am The exam will be CLOSED BOOK • ♦ No textbooks ♦ No calculators ♦ No cheat-sheets Alternate seating • The grades will be posted on WebCT • The exam covers Chapters 1,2,3,4,5, and 19. • The sections which are not covered are listed on the • Class Notes web page. RECAP • Human perception of color, white objects, black objects. Light scattering: light is sent in all directions –forward, sideways and • backward ♦ Geometric scattering: R>>λ (all wavelengths equally scattered) ♦ Mie scattering: R~λ (red is scattered more efficiently) ♦ Rayleigh scattering: R<<λ (blue is scattered more efficiently) Phenomena: white clouds, blue skies, hazy skies, crepuscular rays, colorful • sunsets, blue moon. TODAY: Refraction: the bending of the light ray as it travels from one medium to • another. It bends towards the vertical if it enters a more-dense medium and away from the vertical as it enters a less-dense medium. ♦ Phenomena: stars appear higher in the sky, twinkling, twilight. • Reflection: the angle of incidence is equal to the angle of reflection • Total internal reflection: mirages Dispersion: separation of colors when light travels through a medium. • ♦ rainbow Reflection and Refraction of Light The speed of light in vacuum • is c=300,000 km/s Snell’s law: The angle of • incidence is equal to the angle of reflection. Light that enters a more- • dense medium slows down and bends toward the normal. Light that exits a more- • dense medium speeds up and bends away from the normal. -
Light Color and Atmospheric Light, Color, and Atmospheric Optics
Light, Color, and Atmospheric Optics Chapter 19 April 28 and 30, 2009 Colors • Sunlight contains all colors (visible spectrum) Wavelength Ranges in µm UV-C: 0.25 - 0.29 UV-B: 0.29 - 0.32 UV-A: 0.32 - 0.38 Visible: 0.38 - 0.75 Near IR: 0.75 - 4 Mid IR: 4 - 8 Longwave IR: 8 - 100 Colors • If object is white then all colors are reflected • If object is red then only red is reflected and all others are absorbed From Malm (1999). Introduction to Visibility Blue Skies and Hazy days • Selective scattering – Scattering depends on wavelength of light • Rayleigh scattering – Very small particles, gases • Mie scattering – Particles the size of wavelength of visible light • Blue haze • Some particles from plants: terpenes, α- pinene Blue Ridge Mountains • Blue haze caused by scattering of blue light by fine particles Creppyuscular Rays • Scattering of sunlight by dust and haze produces white bands Selective Scattering: Sunset • Notice the effects of scattering on color as sunlight penetrates into the atmosphere Twinkling, Twilight, and the Green Flash • Light that travels from a less dense to a more dense medium loses speed and bends toward the normal, while light that enters a less dense medium increase speed and bends away from the normal. • Apparent position, scintillation, and green flash all depend of density variations in the athtmosphere • Scintillation also indicates the amount of turbulence in the atmosphere Bending of Light Paths from Atmosphere Green Flash • Green flash at top may be seen under circumstances of very cold (dense) air near the surface rapidly changing to warmer (less dense) air aloft Mirages •Miraggyges are caused by refraction of light due to strong density differences in atmospheric layers usually caused by strong temperature differences. -
Photochemically Driven Collapse of Titan's Atmosphere
REPORTS has escaped, the surface temperature again Photochemically Driven Collapse decreases, down to about 86 K, slightly of Titan’s Atmosphere above the equilibrium temperature, because of the slight greenhouse effect resulting Ralph D. Lorenz,* Christopher P. McKay, Jonathan I. Lunine from the N2 opacity below (longward of) 200 cm21. Saturn’s giant moon Titan has a thick (1.5 bar) nitrogen atmosphere, which has a These calculations assume the present temperature structure that is controlled by the absorption of solar and thermal radiation solar constant of 15.6 W m22 and a surface by methane, hydrogen, and organic aerosols into which methane is irreversibly converted albedo of 0.2 and ignore the effects of N2 by photolysis. Previous studies of Titan’s climate evolution have been done with the condensation. As noted in earlier studies assumption that the methane abundance was maintained against photolytic depletion (5), when the atmosphere cools during the throughout Titan’s history, either by continuous supply from the interior or by buffering CH4 depletion, the model temperature at by a surface or near surface reservoir. Radiative-convective and radiative-saturated some altitudes in the atmosphere (here, at equilibrium models of Titan’s atmosphere show that methane depletion may have al- ;10 km for 20% CH4 surface humidity) lowed Titan’s atmosphere to cool so that nitrogen, its main constituent, condenses onto becomes lower than the saturation temper- the surface, collapsing Titan into a Triton-like frozen state with a thin atmosphere. -
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. -
The Texas Manual on Rainwater Harvesting
The Texas Manual on Rainwater Harvesting Texas Water Development Board Third Edition The Texas Manual on Rainwater Harvesting Texas Water Development Board in cooperation with Chris Brown Consulting Jan Gerston Consulting Stephen Colley/Architecture Dr. Hari J. Krishna, P.E., Contract Manager Third Edition 2005 Austin, Texas Acknowledgments The authors would like to thank the following persons for their assistance with the production of this guide: Dr. Hari Krishna, Contract Manager, Texas Water Development Board, and President, American Rainwater Catchment Systems Association (ARCSA); Jen and Paul Radlet, Save the Rain; Richard Heinichen, Tank Town; John Kight, Kendall County Commissioner and Save the Rain board member; Katherine Crawford, Golden Eagle Landscapes; Carolyn Hall, Timbertanks; Dr. Howard Blatt, Feather & Fur Animal Hospital; Dan Wilcox, Advanced Micro Devices; Ron Kreykes, ARCSA board member; Dan Pomerening and Mary Dunford, Bexar County; Billy Kniffen, Menard County Cooperative Extension; Javier Hernandez, Edwards Aquifer Authority; Lara Stuart, CBC; Wendi Kimura, CBC. We also acknowledge the authors of the previous edition of this publication, The Texas Guide to Rainwater Harvesting, Gail Vittori and Wendy Price Todd, AIA. Disclaimer The use of brand names in this publication does not indicate an endorsement by the Texas Water Development Board, or the State of Texas, or any other entity. Views expressed in this report are of the authors and do not necessarily reflect the views of the Texas Water Development Board, or -
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. -
Environmental Systems the Atmosphere and Hydrosphere
Environmental Systems The atmosphere and hydrosphere THE ATMOSPHERE The atmosphere, the gaseous layer that surrounds the earth, formed over four billion years ago. During the evolution of the solid earth, volcanic eruptions released gases into the developing atmosphere. Assuming the outgassing was similar to that of modern volcanoes, the gases released included: water vapor (H2O), carbon monoxide (CO), carbon dioxide (CO2), hydrochloric acid (HCl), methane (CH4), ammonia (NH3), nitrogen (N2) and sulfur gases. The atmosphere was reducing because there was no free oxygen. Most of the hydrogen and helium that outgassed would have eventually escaped into outer space due to the inability of the earth's gravity to hold on to their small masses. There may have also been significant contributions of volatiles from the massive meteoritic bombardments known to have occurred early in the earth's history. Water vapor in the atmosphere condensed and rained down, of radiant energy in the atmosphere. The sun's radiation spans the eventually forming lakes and oceans. The oceans provided homes infrared, visible and ultraviolet light regions, while the earth's for the earliest organisms which were probably similar to radiation is mostly infrared. cyanobacteria. Oxygen was released into the atmosphere by these early organisms, and carbon became sequestered in sedimentary The vertical temperature profile of the atmosphere is variable and rocks. This led to our current oxidizing atmosphere, which is mostly depends upon the types of radiation that affect each atmospheric comprised of nitrogen (roughly 71 percent) and oxygen (roughly 28 layer. This, in turn, depends upon the chemical composition of that percent). -
Why Doesn't the Sky Turn Green?
Why Doesn't The Sky Turn Green? Rushi Shah 09 November 2015 I was leafing through the US Army Corps of Engineers' Manual on Remote Sensing and learned about how Rayleigh scattering creates blue skies during the day and redish-orange sunsets. Well, everybody knows about blue skies and red sunsets, was the title just click-bait, you ask? No, but I'll get to that. 1 The Basics of Rayleigh Scattering Let's start with this whole Rayleigh scattering thing. Basically the idea is that particles in the atmosphere (like Oxygen and Nitrogen particles) scatter rays of light as they enter the atmosphere. How much the light is scattered is heavily dependent on the wavelength of the light. Remember how ROY-G-BIV represents the colors of the rainbow (and thus the spectrum of visible light)? Well that spectrum of light starts with long wavelength rays (reds, oranges, and yellows) and ends with short wavelength rays (blues, indigos, and violets). 1 The amount of light that is scattered (denoted with the variable I) is highly inversely proportional to the wavelength of the light (denoted with the greek letter ). Put simply, as the wavelength goes down, the light waves are scattered more quickly. 1 I / λ4 When sunlight hits the earth directly during mid-day, it travels through a small amount of atmosphere, and thus we see the wavelengths of light that are immediately scattered. Based on the equation above, the blues, indigos, and violets would be scattered first (and they blend together into the blue sky we see). As the sun sets, it goes through more and more particles to reach us. -
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. -
Atmospheric Phenomena by Feist
Atmospheric optical phenomena An introductory guide by Mike Feist Effects caused by water droplets— rainbows and coronae The most well known optical sky effect is the rainbow. This, as most people know, sometimes occurs when the Sun is out and it is raining. To see a rainbow you must stand with your back to the Sun with the raindrops in front of you. It does not have to be raining where you are standing but in the direction that you are looking. The arc of the primary (main) bow is centred on the antisolar point, the spot directly oppo- site the Sun, and has a radius of 42°. The antisolar point is actually centred on the shadow of your head. If the Sun is rising or setting and therefore on the horizon, the primary rainbow will be a complete semi- circle and the top will be 42° up in the sky. If, on the other hand, the Sun is 42° up in the sky, the primary bow will be on the horizon, the top just rising or setting. Con- ventionally the rainbow is said to have John Constable. Hampstead Heath with a Rainbow (1836). seven colours but all we need to remember seen in the spray near waterfalls and artifi- ous forms but with a six-sided shape. They is that, in the primary bow, the red is on cial rainbows can be made using a garden may be as flat hexagonal plates or long the outside and the blue on the inside. Out- hose. Rainbows are one of the easiest opti- hexagonal prisms or as a combination of side the primary bow sometimes there is cal effects to photograph although they the two. -
Mystic Mountain © Mendip Hills AONB
Viewpoint Mystic mountain © Mendip Hills AONB Time: 15 mins Region: South West England Landscape: rural Location: Ebbor Gorge, Somerset, BA5 3BA Grid reference: ST 52649 48742 Getting there: Park at Deer Leap car park and picnic area (on the road between Wookey Hole and Priddy) Keep an eye out for: Buzzards and other birds of prey soaring on the thermals below From this stunning vantage point we have sweeping views south across the flat land of the Somerset Levels. On a clear day, looking east you can see the dark line of hills marking out Exmoor National Park and if you look in a west south-west direction you can even spot the Bristol Channel glistening in the distance. As our eyes pan across the view they rest on a perfectly rounded knoll with a short tower on top. This is Glastonbury Tor. Claimed as the site of the legendary Vale of Avalon and the final resting place of King Arthur, the tor rises up above the flat land surrounding it and is visible for miles around. Why does the mystical Glastonbury Tor rise up out of the surrounding lowlands? First of all look straight ahead and in the middle distance you’ll see three hills which punctuate the flat landscape. From left to right they are Hay Hill, Ben Knowle Hill and Yarley Hill, part of a low ridge just south of the River Axe. Surrounding these hills the Somerset Levels are an area of low-lying farmland. The lowest point is just 0.2 metres above sea level. -
Atmospheric Refraction
Z w o :::> l I ~ <x: '----1-'-1----- WAVE FR ON T Z = -rnX + Zal rn = tan e '----------------------X HORIZONTAL POSITION de = ~~ = (~~) tan8dz v FIG. 1. Origin of atmospheric refraction. DR. SIDNEY BERTRAM The Bunker-Ramo Corp. Canoga Park, Calif. Atmospheric Refraction INTRODUCTION it is believed that the treatment presented herein represents a new and interesting ap T IS WELL KNOWN that the geometry of I aerial photographs may be appreciably proach to the problem. distorted by refraction in the atmosphere at THEORETICAL DISCUSSION the time of exposure, and that to obtain maximum mapping accuracy it is necessary The origin of atmospheric refraction can to compensate this distortion as much as be seen by reference to Figure 1. A light ray knowledge permits. This paper presents a L is shown at an angle (J to the vertical in a solution of the refraction problem, including medium in which the velocity of light v varies a hand calculation for the ARDC Model 1 A. H. Faulds and Robert H. Brock, Jr., "Atmo Atmosphere, 1959. The effect of the curva spheric Refraction and its Distortion of Aerial ture of the earth on the refraction problem is Photography," PSOTOGRAMMETRIC ENGINEERING analyzed separately and shown to be negli Vol. XXX, No.2, March 1964. 2 H. H. Schmid, "A General Analytical Solution gible, except for rays approaching the hori to the Problem of Photogrammetry," Ballistic Re zontal. The problem of determining the re search Laboratories Report No. 1065, July 1959 fraction for a practical situation is also dis (ASTIA 230349). cussed. 3 D. C.