The Min Min Light and the Fata Morgana Pettigrew
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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. -
Report to Office of Water Science, Department of Science, Information Technology and Innovation, Brisbane
Lake Eyre Basin Springs Assessment Project Hydrogeology, cultural history and biological values of springs in the Barcaldine, Springvale and Flinders River supergroups, Galilee Basin and Tertiary springs of western Queensland 2016 Department of Science, Information Technology and Innovation Prepared by R.J. Fensham, J.L. Silcock, B. Laffineur, H.J. MacDermott Queensland Herbarium Science Delivery Division Department of Science, Information Technology and Innovation PO Box 5078 Brisbane QLD 4001 © The Commonwealth of Australia 2016 The Queensland Government supports and encourages the dissemination and exchange of its information. The copyright in this publication is licensed under a Creative Commons Attribution 3.0 Australia (CC BY) licence Under this licence you are free, without having to seek permission from DSITI or the Commonwealth, to use this publication in accordance with the licence terms. You must keep intact the copyright notice and attribute the source of the publication. For more information on this licence visit http://creativecommons.org/licenses/by/3.0/au/deed.en Disclaimer This document has been prepared with all due diligence and care, based on the best available information at the time of publication. The department holds no responsibility for any errors or omissions within this document. Any decisions made by other parties based on this document are solely the responsibility of those parties. Information contained in this document is from a number of sources and, as such, does not necessarily represent government or departmental policy. If you need to access this document in a language other than English, please call the Translating and Interpreting Service (TIS National) on 131 450 and ask them to telephone Library Services on +61 7 3170 5725 Citation Fensham, R.J., Silcock, J.L., Laffineur, B., MacDermott, H.J. -
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. -
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. -
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 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 -
The Antarctic Sun, December 17, 2006
December 17, 2006 New fi nds in Dry Valleys indicate ancient tundra By Peter Rejcek Sun staff Flannel shirts and jeans – or perhaps a light fleece – may have been the norm in the McMurdo Dry Valleys of Antarctica about 14 mil- lion years ago. Fossil records and glacial history in an area of the western Olympus Range near Mount Boreas indi- cate that during the middle of the Miocene epoch (about 14 million years ago) climatic conditions were warm and wet enough to support plant and insect life, according to a team of scientists that returned this season to continue its research. The story began when Adam Lewis, a post-doctoral fellow at The Antarctic The Sun Byrd Polar Research Center at The Ohio State University, traversed a roughly 100-square-kilometer Allan Ashworth picks through a pile of area of the Olympus Range sev- Peter Rejcek / eral years ago while working on shale looking for fossils and other his doctorate. His thesis involved fleshing out the glacial history evidence of a tundra environment that he and of eight valleys between various mountain peaks. others believe disappeared in the McMurdo Dry “In the process of doing that, I discovered these lake deposits,” Valleys about 14 million years ago. explained Lewis shortly before he headed into the field via helicop- See related story on page 8 See CLIMATE on page 9 Blowin’ in the Wind Quote of the Week USAP looks to harness alternative energy for McMurdo, South Pole “So, are you originally from By Steve Martaindale Programs for the National Science Foundation. -
The Fata Morgana. by Professor FA Forel, Morges
1911-12.] The Fata Morgana. 175 XV.—The Fata Morgana. By Professor F. A. Forel, Morges, Switzerland. Abstract of an Address delivered before the Society on July II,., 1911; translated by Professor C. G. Knott. AMONG optical phenomena which originate over the surface of water there is one so ill-defined and ill-observed as to be still mysterious; till now it has received no valid explanation. The Italians call it the Fata Morgana. Under conditions still lacking precise description, there appear on the far side of the Straits of Messina certain fantastic visions, fortresses and castles of unknown cities, which seem to emerge from the sea, soon to vanish again. These are the "palaces" of the "fairy Morgana," which appear and dis- appear at the capricious stroke of the magician's wand. Most of the accounts of the phenomenon are founded on the extravagant description and the amazing picture published in 1773 by the Dominican friar Don Antonio Minasi, professor of botany at the Roman College of Sapienzia. This drawing, with its incoherent groupings of castles and boats, reflected and refracted at random in a manner quite inconsistent with physical possibilities, was largely the creation of the distorted imagination of an artist who did not understand in the least the wonderful illusion. To appreciate the confusion which reigns in the scientific world in regard to this phenomenon, the reader need only refer to the chapter on the Fata Morgana in Pernter's admirable work on Meteorological Optics (Vienna, 1910). There he will be impressed with the uncertainty of the conclusions reached by the author after a study of the insufficient and contradictory documents to which he had access. -
How to Format a SCCG Papaer
Chasing the Green Flash: a Global Illumination Solution for Inhomogeneous Media D. Gutierrez F.J. Seron O. Anson A. Muñoz University of Zaragoza University of Zaragoza University of Zaragoza University of Zaragoza [email protected] [email protected] [email protected] [email protected] restrictions on the scenes and effects that can be Abstract reproduced, including some of the phenomena that occur in our atmosphere. Several natural phenomena, such as mirages or the Most of the media are in fact inhomogeneous to one green flash, are owed to inhomogeneous media in degree or another, with properties varying continuously which the index of refraction is not constant. This from point to point. The atmosphere, for instance, is in makes the light rays travel a curved path while going fact inhomogeneous since pressure, temperature and through those media. One way to simulate global other properties do vary from point to point, and illumination in inhomogeneous media is to use a therefore its optic characterization, given by the index curved ray tracing algorithm, but this approach of refraction, is not constant. presents some problems that still need to be solved. A light ray propagating in a straight line would then be This paper introduces a full solution to the global accurate only in two situations: either there is no media illumination problem, based on what we have called through which the light travels (as in outer space, for curved photon mapping, that can be used to simulate instance), or the media are homogeneous. But with several natural atmospheric phenomena. We also inhomogeneous media, new phenomena occur. -
Evaluating the Effectiveness of Current Atmospheric Refraction Models in Predicting Sunrise and Sunset Times
Michigan Technological University Digital Commons @ Michigan Tech Dissertations, Master's Theses and Master's Reports 2018 Evaluating the Effectiveness of Current Atmospheric Refraction Models in Predicting Sunrise and Sunset Times Teresa Wilson Michigan Technological University, [email protected] Copyright 2018 Teresa Wilson Recommended Citation Wilson, Teresa, "Evaluating the Effectiveness of Current Atmospheric Refraction Models in Predicting Sunrise and Sunset Times", Open Access Dissertation, Michigan Technological University, 2018. https://doi.org/10.37099/mtu.dc.etdr/697 Follow this and additional works at: https://digitalcommons.mtu.edu/etdr Part of the Atmospheric Sciences Commons, Other Astrophysics and Astronomy Commons, and the Other Physics Commons EVALUATING THE EFFECTIVENESS OF CURRENT ATMOSPHERIC REFRACTION MODELS IN PREDICTING SUNRISE AND SUNSET TIMES By Teresa A. Wilson A DISSERTATION Submitted in partial fulfillment of the requirements for the degree of DOCTOR OF PHILOSOPHY In Physics MICHIGAN TECHNOLOGICAL UNIVERSITY 2018 © 2018 Teresa A. Wilson This dissertation has been approved in partial fulfillment of the requirements for the Degree of DOCTOR OF PHILOSOPHY in Physics. Department of Physics Dissertation Co-advisor: Dr. Robert J. Nemiroff Dissertation Co-advisor: Dr. Jennifer L. Bartlett Committee Member: Dr. Brian E. Fick Committee Member: Dr. James L. Hilton Committee Member: Dr. Claudio Mazzoleni Department Chair: Dr. Ravindra Pandey Dedication To my fellow PhD students and the naive idealism with which we started this adventure. Like Frodo, we will never be the same. Contents List of Figures ................................. xi List of Tables .................................. xvii Acknowledgments ............................... xix List of Abbreviations ............................. xxi Abstract ..................................... xxv 1 Introduction ................................. 1 1.1 Introduction . 1 1.2 Effects of Refraction on Horizon . -
Storms, Swells, Snowand Ice (Topped with Polar Bears)
travel at home travel at home INTO THE NORTH Storms, swells, snow and ICE and OUT OF THE (topped with polar bears) are NORTHWEST PASSAGE all part of this EPIC voyage STORY + PHOTOGRAPHY BY Barb Sligl Iceberg at sunset, 250 km north of the Arctic Circle in Ilulissat Icefjord in Greenland, a UNESCO World Heritage Site 36 JUST FOR CANADIAN DENTISTS November/December 2016 travel at home travel at home omewhere above the Arctic Circle, I see a fata morgana. Low-lying, barren islands—like so many sperm whales with their broad, sloping foreheads—float above the horizon in Coronation Gulf. As if I’m a long-lost sea captain of yore, it’s a glimpse of what’s called a superior mirage. In 1818, on his search for the long-sought Northwest Passage, captain John Ross’s route was barred by an insurmountable range he called Croker’s Mountains. Yet there was no such thing. A year later, another explorer sailed right through the same spot in Lancaster Sound, as did doomed Franklin in 1845 and then the first man to make it through the SNorthwest Passage in 1906, Roald Amundsen. Today, this storied route is often still blocked—by sea ice. It’s what makes it one of the last untouched places on earth. I’m on Adventure Canada’s Out of the Northwest Passage voyage, and after my fata morgana sighting, I continue to see fantastical things over the next 16 days of this historic- yet-still-novel voyage. From a strip of pink on the horizon that hovers between inky sea and dark swathe of clouds like a Rothko painting to storms and swells, snow and ice—all High Arctic sunset, like a Rothko painting Touring Ilulissat Icefjord by zodiac with the seductive whisper of peril.