Sunset/Sunrise Phenomena
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How the Sun Paints the Sky the Generation of Its Colour and Luminosity Bob Fosbury European Southern Observatory and University College London
How the Sun Paints the Sky The generation of its colour and luminosity Bob Fosbury European Southern Observatory and University College London Introduction: the 19th century context — science and painting The appearance of a brilliantly clear night sky must surely have stimulated the curiosity of our earliest ancestors and provided them with the foundation upon which their descendants built the entire edifice of science. This is a conclusion that would be dramatically affirmed if any one of us were to look upwards in clear weather from a location that is not polluted by artificial light: an increasingly rare possibility now, but one that provides a welcome regeneration of the sense of wonder. What happened when our ancient ancestors gazed instead at the sky in daylight or twilight? It is difficult to gauge from written evidence as there was such variation in the language of description among different cultures (see “Sky in a bottle” by Peter Pesic. MIT Press, 2005. ISBN 0-262-16234-2). The blue colour of a cloudless sky was described in a remarkable variety of language, but the question of its cause most often remained in the realm of a superior being. Its nature did concern the Greek philosophers but they appeared to describe surfaces and objects in the language of texture rather than colour: they did not have a word for blue. It was only during the last millennium that thinkers really tried to get to grips with the problem, with Leonardo da Vinci, Isaac Newton and Johann Wolfgang von Goethe all applying themselves. It was not easy however, and no real progress was made until the mid-19th century when there was a focus of the greatest scientific minds of the time on the problem of both the colour and the what was then the novel property of polarisation of the light. -
Rare Astronomical Sights and Sounds
Jonathan Powell Rare Astronomical Sights and Sounds The Patrick Moore The Patrick Moore Practical Astronomy Series More information about this series at http://www.springer.com/series/3192 Rare Astronomical Sights and Sounds Jonathan Powell Jonathan Powell Ebbw Vale, United Kingdom ISSN 1431-9756 ISSN 2197-6562 (electronic) The Patrick Moore Practical Astronomy Series ISBN 978-3-319-97700-3 ISBN 978-3-319-97701-0 (eBook) https://doi.org/10.1007/978-3-319-97701-0 Library of Congress Control Number: 2018953700 © Springer Nature Switzerland AG 2018 This work is subject to copyright. All rights are reserved by the Publisher, whether the whole or part of the material is concerned, specifically the rights of translation, reprinting, reuse of illustrations, recitation, broadcasting, reproduction on microfilms or in any other physical way, and transmission or information storage and retrieval, electronic adaptation, computer software, or by similar or dissimilar methodology now known or hereafter developed. The use of general descriptive names, registered names, trademarks, service marks, etc. in this publication does not imply, even in the absence of a specific statement, that such names are exempt from the relevant protective laws and regulations and therefore free for general use. The publisher, the authors, and the editors are safe to assume that the advice and information in this book are believed to be true and accurate at the date of publication. Neither the publisher nor the authors or the editors give a warranty, express or implied, with respect to the material contained herein or for any errors or omissions that may have been made. -
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. -
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. -
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. -
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. -
Insider Tips
It’s no secret that North Lake Tahoe has some of the most gorgeous sunsets on the west coast, but did you know that winter is actually the best time to watch the sunset? The shoreline of North Lake Tahoe is the perfect place to watch the sky light up, so follow along and get your cameras ready! What Is It? Fun Facts Year-round, North Lake Tahoe is home to the most awe- • Alpenglow happens when light is reflected off airborne inspiring sunsets featuring breathtaking cotton candy colored precipitation and ice crystals in the lower atmosphere skies. In winter, the signature snowy scenery and glittering and technically is only visible after sunset or before waters add even more beauty to the region’s sunsets for a sunrise. The term “alpenglow” dates back to 19th can’t-miss viewing experience. century Germany to describe this unique phenomenon. Where Can I Find It? If You Like This, You’ll Love: North Lake Tahoe’s beaches are some of the best places to Other great spots for winter lakeside sunsets in North Lake catch stunning sunsets in the winter, from Commons Beach Tahoe include: in Tahoe City to The Hyatt Regency Lake Tahoe’s beach in • Hidden Beach in Incline Village Incline Village and everywhere in between. • Donner Summit in Truckee Because sunsets happen earlier during winter months, these beaches also offer the perfect jumping off point to enjoy • Moon Dunes Beach in Tahoe Vista dinner during or after a sunset. Try these different restaurants • Speedboat Beach in Crystal Bay for the perfect post-sunset meal: In Tahoe City and Commons Beach Insider Tips • Christy Hill, Sunnyside Restaurant & Lodge, Jake’s On • Because the sun goes down earlier in the winter, visitors The Lake, or Wolfdale’s Cuisine Unique can enjoy the sunset before, or during, dinner without In Kings Beach and Carnelian Bay having to stay up late. -
Planit! User Guide
ALL-IN-ONE PLANNING APP FOR LANDSCAPE PHOTOGRAPHERS QUICK USER GUIDES The Sun and the Moon Rise and Set The Rise and Set page shows the 1 time of the sunrise, sunset, moonrise, and moonset on a day as A sunrise always happens before a The azimuth of the Sun or the well as their azimuth. Moon is shown as thick color sunset on the same day. However, on lines on the map . some days, the moonset could take place before the moonrise within the Confused about which line same day. On those days, we might 3 means what? Just look at the show either the next day’s moonset or colors of the icons and lines. the previous day’s moonrise Within the app, everything depending on the current time. In any related to the Sun is in orange. case, the left one is always moonrise Everything related to the Moon and the right one is always moonset. is in blue. Sunrise: a lighter orange Sunset: a darker orange Moonrise: a lighter blue 2 Moonset: a darker blue 4 You may see a little superscript “+1” or “1-” to some of the moonrise or moonset times. The “+1” or “1-” sign means the event happens on the next day or the previous day, respectively. Perpetual Day and Perpetual Night This is a very short day ( If further north, there is no Sometimes there is no sunrise only 2 hours) in Iceland. sunrise or sunset. or sunset for a given day. It is called the perpetual day when the Sun never sets, or perpetual night when the Sun never rises. -
Atmospheric Refraction
International Young Naturalists’ Tournament 4. Sunset Serbian team Regional Center For Talented Youth 4. Sunset The visible Sun disk touches the horizon and after a particular time interval disappears behind the horizon. What is the duration of this time interval? Explain the optical phenomena observed during a sunset. SUNSET Sunset (sundown) - daily disappearance of the Sun below the western horizon, as a result of Earth's rotation In astronomy : the time of sunset - moment when the trailing edge of the Sun's disk disappears below the horizon ANGULAR VELOCITY OF THE SUN • angularthe angle speed by which for one an complete object spins rotation in a certain is given time as: - its rotation rate t = 23h 54 min 4s ANGULAR VELOCITY - orthogonal component- ω ϕ DURATION OF SUNSET •equation for the duration of sunset: DURATION OF SUNSET • The fastest sunset at the time of the equinoxes (March 21 and September 23 • The slowest sunset at the time of solstice (around 21 June and 21 December) DURATION OF SUNSET • The fastest sunset - 2 minutes 47 sec • The slowest sunset - 3 min 23 sec • At the equator, between 128 and 142 sec (2 min. 8 sec and 2 min. 22 sec) DURATION OF SUNSET City Duration of sunset Latitude Beijing 167 s 39.92° Belgrade 183.6 s 44.82° Paris 198 s 48.86° London 209.3 s 51.51° Moscow 231.5 s 55.75 ° Light scattering Reflection Refraction LIGHT SCATTERING • caused by small particles and molecules in the atmosphere • scattered rays go off in many directions RAYLEIGH SCATTERING • Rayleigh scattering - elastic scattering of light • Blue light from the sun is scattered more than red LAW OF REFLECTION DIFFUSE REFLECTION • It occurs when a rough surface causes reflected rays to travel in different directions ATMOSPHERIC REFRACTION • the shift in apparent direction of a celestial object caused by the refraction of light rays as they pass through Earth’s atmosphere MORE OPTICAL PHENOMENA Twilight Wedge Belt of Venus Earth’s shadow Afterglow Alpenglow CONCLUSION During the sunset: 1. -
The Blue Hour‐ by Dennis Arculeo
THE April 2019 May 16th‐ End of Year Compeon Building G Sung Harbor 8 PM th May 4 ‐ Model Shoot ‐ Mayr Studio ‐ Staten Island Camera Club Meet‐Up reserve a seat @: hps://www.meetup.com/ Staten‐Island‐camera‐club/events/259170884/ spaces are limited. May 16th‐ End of Year Compeon ‐ Harbor Room 8:00PM Image of the Year Selecon ‐ Judge Al Brown. June 6th - Annual Awards Dinner - Real Madrid Restaurant - All are welcome - Bring a Friend - Paid Reservation is a must! June 8th Saturday Governors House Meet‐Up reserve a seat @: reserve a seat @: hps://www.meetup.com/Staten‐Island‐camera‐ club/events/ spaces are limited. Well, the End of Year Compeon is almost here. On that For those who aended in the past the menu is the same. night we will decide the Images of the Year. So come on down on May 16th.. Color and Mono Digital Images and You can secure your reservaon with a $45.00 per person pay‐ Prints will compete for the coveted awards in each of their ment on May 16that this month’s End of the Year Compe‐ respecve categories. You can enter any 4 Color or Mono on. Please bring a check payable to Staten Island Camera Club. Digital and or Print that you competed with this season. If you are not aending the End of Year Compeon, but would Here is the low down on the Awards Dinner being held on like to aend the dinner please mail your check to: Thursday June 6th, 2019. Barbara M. Hoffman at 323 Stobe Avenue, SI, NY 10306. -
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.