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Kompletní Seznam Halových Jevů a Odkazy Na Příslušné Internetov
List of halo links (by Patrik Trncak) Halos: 6° halo http://www.somerikko.net/old/i_halo/SPF12_32a.jpg 9° halo (Van Buijsen halo) http://www.astro.helsinki.fi/~kahanpaa/halot/ around Moon: http://www.meteoros.de/ee31ee38/ee31_3.htm 12° halo http://www.somerikko.net/old/i_halo/SPF12_32a.jpg 18° halo (Rankin halo) http://www.astro.helsinki.fi/~kahanpaa/halot/ around Moon: http://halo.astronomie.cz/galerie/pyramid/002.jpg 20° halo (Burney halo) http://www.astro.helsinki.fi/~kahanpaa/halot/ around Moon: (in book Atmospheric halos only) 22° halo (small halo) http://www.polarimage.fi/phenom/ha03521a.jpg around Moon: http://www.photoastronomique.net/grand/halo_lune02.jpg 23° halo (Barkow halo) http://www.astro.helsinki.fi/~kahanpaa/halot/ around Moon: (photo not available) 24° halo (Dutheil halo) http://www.meteoros.de/halres/schnee.htm around Moon: http://www.ursa.fi/ursa/jaostot/halot/umi/1999/199page06.gif 28° halo (Scheiner halo) http://www.iki.fi/mika.sillanpaa/ichalos 35° halo (Feuillee halo) http://www.teknofokus.fi/Foto/Haloja/Halo10huhti.htm around Moon: (photo not available) 46° halo (big halo) http://www.somerikko.net/halos/images/sp419.jpg Circumstcribed halo http://www.sundog.clara.co.uk/halo/circim2.htm around Moon: http://www.rfleet.clara.net/gbh/haloes/hal07m.jpg Elliptical halos http://epod.usra.edu/archive/images/ellipse_7.jpg around Moon: http://www.kolumbus.fi/jukka.ruoskanen/Valoilmiot/slides/Elliptical%20halo.jpg Hevel halo http://projekty.astro.cz/ukazy/obr/hevelius_c.jpg Bouguer halo http://www.ursa.fi/ursa/jaostot/halot/havaitseminen/opas/xi_hist.pdf -
View and Print This Publication
@ SOUTHWEST FOREST SERVICE Forest and R U. S.DEPARTMENT OF AGRICULTURE P.0. BOX 245, BERKELEY, CALIFORNIA 94701 Experime Computation of times of sunrise, sunset, and twilight in or near mountainous terrain Bill 6. Ryan Times of sunrise and sunset at specific mountain- ous locations often are important influences on for- estry operations. The change of heating of slopes and terrain at sunrise and sunset affects temperature, air density, and wind. The times of the changes in heat- ing are related to the times of reversal of slope and valley flows, surfacing of strong winds aloft, and the USDA Forest Service penetration inland of the sea breeze. The times when Research NO& PSW- 322 these meteorological reactions occur must be known 1977 if we are to predict fire behavior, smolce dispersion and trajectory, fallout patterns of airborne seeding and spraying, and prescribed burn results. ICnowledge of times of different levels of illumination, such as the beginning and ending of twilight, is necessary for scheduling operations or recreational endeavors that require natural light. The times of sunrise, sunset, and twilight at any particular location depend on such factors as latitude, longitude, time of year, elevation, and heights of the surrounding terrain. Use of the tables (such as The 1 Air Almanac1) to determine times is inconvenient Ryan, Bill C. because each table is applicable to only one location. 1977. Computation of times of sunrise, sunset, and hvilight in or near mountainous tersain. USDA Different tables are needed for each location and Forest Serv. Res. Note PSW-322, 4 p. Pacific corrections must then be made to the tables to ac- Southwest Forest and Range Exp. -
Antarctic Primer
Antarctic Primer By Nigel Sitwell, Tom Ritchie & Gary Miller By Nigel Sitwell, Tom Ritchie & Gary Miller Designed by: Olivia Young, Aurora Expeditions October 2018 Cover image © I.Tortosa Morgan Suite 12, Level 2 35 Buckingham Street Surry Hills, Sydney NSW 2010, Australia To anyone who goes to the Antarctic, there is a tremendous appeal, an unparalleled combination of grandeur, beauty, vastness, loneliness, and malevolence —all of which sound terribly melodramatic — but which truly convey the actual feeling of Antarctica. Where else in the world are all of these descriptions really true? —Captain T.L.M. Sunter, ‘The Antarctic Century Newsletter ANTARCTIC PRIMER 2018 | 3 CONTENTS I. CONSERVING ANTARCTICA Guidance for Visitors to the Antarctic Antarctica’s Historic Heritage South Georgia Biosecurity II. THE PHYSICAL ENVIRONMENT Antarctica The Southern Ocean The Continent Climate Atmospheric Phenomena The Ozone Hole Climate Change Sea Ice The Antarctic Ice Cap Icebergs A Short Glossary of Ice Terms III. THE BIOLOGICAL ENVIRONMENT Life in Antarctica Adapting to the Cold The Kingdom of Krill IV. THE WILDLIFE Antarctic Squids Antarctic Fishes Antarctic Birds Antarctic Seals Antarctic Whales 4 AURORA EXPEDITIONS | Pioneering expedition travel to the heart of nature. CONTENTS V. EXPLORERS AND SCIENTISTS The Exploration of Antarctica The Antarctic Treaty VI. PLACES YOU MAY VISIT South Shetland Islands Antarctic Peninsula Weddell Sea South Orkney Islands South Georgia The Falkland Islands South Sandwich Islands The Historic Ross Sea Sector Commonwealth Bay VII. FURTHER READING VIII. WILDLIFE CHECKLISTS ANTARCTIC PRIMER 2018 | 5 Adélie penguins in the Antarctic Peninsula I. CONSERVING ANTARCTICA Antarctica is the largest wilderness area on earth, a place that must be preserved in its present, virtually pristine state. -
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. -
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. -
Midnight Sun, Part II by PA Lassiter
Midnight Sun, Part II by PA Lassiter . N.B. These chapters are based on characters created by Stephenie Meyer in Twilight, the novel. The title used here, Midnight Sun, some of the chapter titles, and all the non-interior dialogue between Edward and Bella are copyright Stephenie Meyer. The first half of Ms. Meyer’s rough-draft novel, of which this is a continuation, can be found at her website here: http://www.stepheniemeyer.com/pdf/midnightsun_partial_draft4.pdf 12. COMPLICATIONSPart B It was well after midnight when I found myself slipping through Bella’s window. This was becoming a habit that, in the light of day, I knew I should attempt to curb. But after nighttime fell and I had huntedfor though these visits might be irresponsible, I was determined they not be recklessall of my resolve quickly faded. There she lay, the sheet and blanket coiled around her restless body, her feet bound up outside the covers. I inhaled deeply through my nose, welcoming the searing pain that coursed down my throat. As always, Bella’s bedroom was warm and humid and saturated with her scent. Venom flowed into my mouth and my muscles tensed in readiness. But for what? Could I ever train my body to give up this devilish reaction to my beloved’s smell? I feared not. Cautiously, I held my breath and moved to her bedside. I untangled the bedclothes and spread them carefully over her again. She twitched suddenly, her legs scissoring as she rolled to her other side. I froze. “Edward,” she breathed. -
The Golden Hour Refers to the Hour Before Sunset and After Sunrise
TheThe GoldenGolden HourHour The Golden Hour refers to the hour before sunset and after sunrise. Photographers agree that some of the very best times of day to take photos are during these hours. During the Golden Hours, the atmosphere is often permeated with breathtaking light that adds ambiance and interest to any scene. There can be spectacular variations of colors and hues ranging from subtle to dramatic. Even simple subjects take on an added glow. During the Golden Hours, take photos when the opportunity presents itself because light changes quickly and then fades away. 07:14:09 a.m. 07:15:48 a.m. Photographed about 60 seconds after previous photo. The look of a scene can vary greatly when taken at different times of the day. Scene photographed midday Scene photographed early morning SampleSample GoldenGolden HourHour photosphotos Top Tips for taking photos during the Golden Hours Arrive on the scene early to take test shots and adjust camera settings. Set camera to matrix or center-weighted metering. Use small apertures for maximizing depth-of-field. Select the lowest possible ISO. Set white balance to daylight or sunny day. When lighting is low, use a tripod with either a timed shutter release (self-timer) or a shutter release cable or remote. Taking photos during the Golden Hours When photographing the sun Don't stare into the sun, or hold the camera lens towards it for a very long time. Meter for the sky but don't include the sun itself. Composition tips: The horizon line should be above or below the center of the scene. -
George Orwell in His Centenary Year a Catalan Perspective
THE ANNUAL JOAN GILI MEMORIAL LECTURE MIQUEL BERGA George Orwell in his Centenary Year A Catalan Perspective THE ANGLO-CATALAN SOCIETY 2003 © Miquel Berga i Bagué This edition: The Anglo-Catalan Society Produced and typeset by Hallamshire Publications Ltd, Porthmadog. This is the fifth in the regular series of lectures convened by The Anglo-Catalan Society, to be delivered at its annual conference, in commemoration of the figure of Joan Lluís Gili i Serra (1907-1998), founder member of the Society and Honorary Life President from 1979. The object of publication is to ensure wider diffusion, in English, for an address to the Society given by a distinguished figure of Catalan letters whose specialism coincides with an aspect of the multiple interests and achievements of Joan Gili, as scholar, bibliophile and translator. This lecture was given by Miquel Berga at Aberdare Hall, University of Wales (Cardiff), on 16 November 2002. Translation of the text of the lecture and general editing of the publication were the responsibility of Alan Yates, with the cooperation of Louise Johnson. We are grateful to Miquel Berga himself and to Iolanda Pelegrí of the Institució de les Lletres Catalanes for prompt and sympathetic collaboration. Thanks are also due to Pauline Climpson and Jenny Sayles for effective guidance throughout the editing and production stages. Grateful acknowledgement is made of regular sponsorship of The Annual Joan Gili Memorial Lectures provided by the Institució de les Lletres Catalanes, and of the grant towards publication costs received from the Fundació Congrés de Cultura Catalana. The author Miquel Berga was born in Salt (Girona) in 1952. -
Family Portrait Sessions Frequently Asked Questions Before Your Session
kiawahislandphoto.com Family Portrait Sessions Frequently Asked Questions before Your Session When you make an investment in photography, you want it to last a lifetime. Photographics has the expertise to capture the moment and the artistic style and resources to transform your images into works of art you’ll be proud to share and display. We want you to relax and enjoy the experience so all the joy and fun comes through in your portraits. If you have any concerns about your session, just give us a call or pull your photographer aside to discuss any special needs for your group. Relax, enjoy and smile. We’ve got this. Q: What should we wear? A: For outdoor photography on the beach, choose lighter tones and pastel colors for the most pleasing results. Family members don’t have to match exactly, but should stay coordinated with simple, comfortable clothing that blends with the beach environment. Avoid dark tops, busy patterns, graphics/logos, and primary colors that have a tendency to stand out and clash with the environment. Ladies, we’ll be kneeling and sitting in the sand so be wary of low necklines and short skirts. Overall…be comfortable. For great ideas visit our blog online. Q: When is the best time to take beach portraits? A: On the East Coast, the best time is the “golden hour” just before sunset when the light is softer and the temperature is more moderate. We don’t take portraits in the morning and early afternoon hours, because the sun on the beach is too intense which causes harsh shadows and squinting. -
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 -
Exploring Solar Cycle Influences on Polar Plasma Convection
Comparison of Terrestrial and Martian TEC at Dawn and Dusk during Solstices Angeline G. Burrell1 Beatriz Sanchez-Cano2, Mark Lester2, Russell Stoneback1, Olivier Witasse3, Marco Cartacci4 1Center for Space Sciences, University of Texas at Dallas 2Radio and Space Plasma Physics, University of Leicester 3European Space Agency, ESTEC – Scientific Support Office 4Istituto Nazionale di Astrofisica, Istituto di Astrofisica e Planetologia Spaziali 52nd ESLAB Symposium Outline • Motivation • Data and analysis – TEC sources – Data selection – Linear fitting • Results – Martian variations – Terrestrial variations – Similarities and differences • Conclusions Motivation • The Earth and Mars are arguably the most similar of the solar planets - They are both inner, rocky planets - They have similar axial tilts - They both have ionospheres that are formed primarily through EUV and X- ray radiation • Planetary differences can provide physical insights Total Electron Content (TEC) • The Global Positioning System • The Mars Advanced Radar for (GPS) measures TEC globally Subsurface and Ionosphere using a network of satellites and Sounding (MARSIS) measures ground receivers the TEC between the Martian • MIT Haystack provides calibrated surface and Mars Express TEC measurements • Mars Express has an inclination - Available from 1999 onward of 86.9˚ and a period of 7h, - Includes all open ground and allowing observations of all space-based sources locations and times - Specified with a 1˚ latitude by 1˚ • TEC is available for solar zenith longitude resolution with error estimates angles (SZA) greater than 75˚ Picardi and Sorge (2000), In: Proc. SPIE. Eighth International Rideout and Coster (2006) doi:10.1007/s10291-006-0029-5, 2006. Conference on Ground Penetrating Radar, vol. 4084, pp. 624–629. -
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.