Extending Coordinated Universal Time to Dates Before 1972∗
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Ast 443 / Phy 517
AST 443 / PHY 517 Astronomical Observing Techniques Prof. F.M. Walter I. The Basics The 3 basic measurements: • WHERE something is • WHEN something happened • HOW BRIGHT something is Since this is science, let’s be quantitative! Where • Positions: – 2-dimensional projections on celestial sphere (q,f) • q,f are angular measures: radians, or degrees, minutes, arcsec – 3-dimensional position in space (x,y,z) or (q, f, r). • (x,y,z) are linear positions within a right-handed rectilinear coordinate system. • R is a distance (spherical coordinates) • Galactic positions are sometimes presented in cylindrical coordinates, of galactocentric radius, height above the galactic plane, and azimuth. Angles There are • 360 degrees (o) in a circle • 60 minutes of arc (‘) in a degree (arcmin) • 60 seconds of arc (“) in an arcmin There are • 24 hours (h) along the equator • 60 minutes of time (m) per hour • 60 seconds of time (s) per minute • 1 second of time = 15”/cos(latitude) Coordinate Systems "What good are Mercator's North Poles and Equators Tropics, Zones, and Meridian Lines?" So the Bellman would cry, and the crew would reply "They are merely conventional signs" L. Carroll -- The Hunting of the Snark • Equatorial (celestial): based on terrestrial longitude & latitude • Ecliptic: based on the Earth’s orbit • Altitude-Azimuth (alt-az): local • Galactic: based on MilKy Way • Supergalactic: based on supergalactic plane Reference points Celestial coordinates (Right Ascension α, Declination δ) • δ = 0: projection oF terrestrial equator • (α, δ) = (0,0): -
Programme Book COLOPHON
tolkien society UNQUENDOR lustrum day saturday 19 june 2021 celebrating unquendor's 40th anniversary theme: númenor 1 programme book COLOPHON This programme book is offered to you by the Lustrum committee 2021. Bram Lagendijk and Jan Groen editors Bram Lagendijk design and lay out For the benefit of the many international participants, this programme book is in English. However, of the activities, only the lectures are all in English. The other activities will be in Dutch, occasionally interspersed with English. tolkien society unquendor E-mail: [email protected] Internet: www.unquendor.nl Instagram: www.instagram.com/unquendor Facebook: www.facebook.com/groups/unquendor Twitter: www.twitter.com/unquendor Youtube: www.youtube.com/user/tolkiengenootschap Discord: www.discord.gg/u3wwqHt9RE June 2021 CONTENTS Getting started ... 4 A short history of Unquendor 5 Things you need to know 6 Númenor: The very short story 7 Programme and timetable 8 y Lectures 9 Denis Bridoux Tall ships and tall kings Númenor: From Literary Conception y to Geographical Representation 9 Renée Vink Three times three, The Uncharted Consequences of y the Downfall of Númenor 9 What brought they from Hedwig SlembrouckThe Lord of the Rings Has the history of the Fall of Númenor y been told in ?? 9 the foundered land José Maria Miranda y Law in Númenor 9 Paul Corfield Godfrey, Simon Crosby Buttle Over the flowing sea? WorkshopsThe Second Age: A Beginning and an End 910 y Seven stars and seven stones Nathalie Kuijpers y Drabbles 10 QuizJonne Steen Redeker 10 And one white tree. Caroline en Irene van Houten y Jan Groen Gandalf – The Two Towers y Poem in many languages 10 Languages of Númenor 10 Peter Crijns, Harm Schelhaas, Dirk Trappers y Dirk Flikweert IntroducingLive cooking: the presentersNúmenórean fish pie 1011 Festive toast and … 14 Participants 15 Númenórean fish pie 16 Númenóreaanse vispastei 17 GETTING STARTED… p deze Lustrumdag vieren we het 40-jarig Obestaan van Unquendor! Natuurlijk, we had- den een groot Lustrumfeest voor ogen, ons achtste. -
What Time Is It?
The Astronomical League A Federation of Astronomical Societies Astro Note E3 – What Time Is It? Introduction – There are many methods used to keep time, each having its own special use and advantage. Until recently, when atomic clocks became available, time was reckoned by the Earth's motions: one rotation on its axis was a "day" and one revolution about the Sun was a "year." An hour was one twenty-fourth of a day, and so on. It was convenient to use the position of the Sun in the sky to measure the various intervals. Apparent Time This is the time kept by a sundial. It is a direct measure of the Sun's position in the sky relative to the position of the observer. Since it is dependent on the observer's location, it is also a local time. Being measured according to the true solar position, it is subject to all the irregularities of the Earth's motion. The reference time is 12:00 noon when the true Sun is on the observer's meridian. Mean Time Many of the irregularities in the Earth's motion are due to its elliptical orbit. In order to add some consistency to the measure of time, we use the concept of mean time. Mean time uses the position of a fictitious "mean Sun" which moves smoothly and uniformly across the sky and is insensitive to the irregularities of the Earth’s motion. A mean solar day is 24 hours long. The "Equation of Time," tabulated in almanacs and represented on maps by the analemma, provides the correction between mean and apparent time to allow for the eccentricity of the Earth's orbit. -
An Atomic Physics Perspective on the New Kilogram Defined by Planck's Constant
An atomic physics perspective on the new kilogram defined by Planck’s constant (Wolfgang Ketterle and Alan O. Jamison, MIT) (Manuscript submitted to Physics Today) On May 20, the kilogram will no longer be defined by the artefact in Paris, but through the definition1 of Planck’s constant h=6.626 070 15*10-34 kg m2/s. This is the result of advances in metrology: The best two measurements of h, the Watt balance and the silicon spheres, have now reached an accuracy similar to the mass drift of the ur-kilogram in Paris over 130 years. At this point, the General Conference on Weights and Measures decided to use the precisely measured numerical value of h as the definition of h, which then defines the unit of the kilogram. But how can we now explain in simple terms what exactly one kilogram is? How do fixed numerical values of h, the speed of light c and the Cs hyperfine frequency νCs define the kilogram? In this article we give a simple conceptual picture of the new kilogram and relate it to the practical realizations of the kilogram. A similar change occurred in 1983 for the definition of the meter when the speed of light was defined to be 299 792 458 m/s. Since the second was the time required for 9 192 631 770 oscillations of hyperfine radiation from a cesium atom, defining the speed of light defined the meter as the distance travelled by light in 1/9192631770 of a second, or equivalently, as 9192631770/299792458 times the wavelength of the cesium hyperfine radiation. -
Building the Bridge Between the First and Second Year Experience: a Collaborative Approach to Student Learning and Development STEP
Building the bridge between the first and second year experience: A collaborative approach to student learning and development STEP Introductions STEP Agenda for Today • Share research and theory that shapes first and second year programs • Differentiate programs, interventions, and support that should be targeted at first year students, second year students, or both • Think about your own department and how to work differently with first and second-year students • Review structure of FYE and STEP at Ohio State and where your office can support existing efforts STEP Learning Outcomes • Participants will reflect on and articulate what services, resources, and programming currently exist in their department for first and/or second year students. • Participants will articulate the key salient needs and developmental milestones that often distinguish the second year experience from the first. • Participants will be able to utilize at least one strategy for curriculum differentiation that will contribute to a more seamless experiences for students between their first and second year. Foundational Research that Informs FYE and STEP STEP Developmental Readiness and Sequencing • Developmental Readiness: “The ability and motivation to attend to, make meaning of, and appropriate new knowledge into one’s long term memory structures” (Hannah & Lester, 2009). • Sequencing: The order and structure in which people learn new skill sets (Hannah & Avolio, 2010). • Scaffolding: Support given during the learning process which is tailored to the needs of an -
Second Time Moms & the Truth About Parenting
Second Time Moms & The Truth About Parenting Summary Why does our case deserve an award? In the US, and globally, every diaper brand obsesses about the emotion and joy experienced by new parents. Luvs took the brave decision to focus exclusively on an audience that nobody was talking to: second time moms. Planning made Luvs the official diaper brand of experienced moms. The depth of insights Planning uncovered about this target led to creative work that did a very rare thing for the diaper category: it was funny, entertaining and sparked a record amount of debate. For the first time these moms felt that someone was finally standing up for them and Luvs was applauded for not being afraid to show motherhood in a more realistic way. And in doing so, we achieved the highest volume and value sales in the brand’s history. 2 Luvs: A Challenger Facing A Challenge Luvs is a value priced diaper brand that ranks a distant fourth in terms of value share within the US diaper category at 8.9%. Pampers and Huggies are both premium priced diapers that make up most of the category, with value share at 31, and 41 respectively. Private Label is the third biggest player with 19% value share. We needed to generate awareness to drive trial for Luvs in order to grow the brand, but a few things stood in our way. Low Share Of Voice Huggies spends $54 million on advertising and Pampers spends $48 million. In comparison, Luvs spends only $9 million in media support. So the two dominant diaper brands outspend us 9 to 1, making our goal of increased awareness very challenging. -
Debates in the Digital Humanities This Page Intentionally Left Blank DEBATES in the DIGITAL HUMANITIES
debates in the digital humanities This page intentionally left blank DEBATES IN THE DIGITAL HUMANITIES Matthew K. Gold editor University of Minnesota Press Minneapolis London Chapter 1 was previously published as “What Is Digital Humanities and What’s It Doing in English Departments?” ADE Bulletin, no. 150 (2010): 55– 61. Chap- ter 2 was previously published as “The Humanities, Done Digitally,” The Chron- icle of Higher Education, May 8, 2011. Chapter 17 was previously published as “You Work at Brown. What Do You Teach?” in #alt- academy, Bethany Nowviskie, ed. (New York: MediaCommons, 2011). Chapter 28 was previously published as “Humanities 2.0: Promises, Perils, Predictions,” PMLA 123, no. 3 (May 2008): 707– 17. Copyright 2012 by the Regents of the University of Minnesota all rights reserved. No part of this publication may be reproduced, stored in a retrieval system, or transmitted, in any form or by any means, electronic, mechanical, photocopying, recording, or otherwise, without the prior written permission of the publisher. Published by the University of Minnesota Press 111 Third Avenue South, Suite 290 Minneapolis, MN 55401- 2520 http://www.upress.umn.edu library of congress cataloging-in-publication data Debates in the digital humanities / [edited by] Matthew K. Gold. ISBN 978-0-8166-7794-8 (hardback)—ISBN 978-0-8166-7795-5 (pb) 1. Humanities—Study and teaching (Higher)—Data processing. 2. Humanities —Technological innovations. 3. Digital media. I. Gold, Matthew K.. AZ182.D44 2012 001.3071—dc23 2011044236 Printed in the United States of America on acid- free paper The University of Minnesota is an equal- opportunity educator and employer. -
How Long Is a Year.Pdf
How Long Is A Year? Dr. Bryan Mendez Space Sciences Laboratory UC Berkeley Keeping Time The basic unit of time is a Day. Different starting points: • Sunrise, • Noon, • Sunset, • Midnight tied to the Sun’s motion. Universal Time uses midnight as the starting point of a day. Length: sunrise to sunrise, sunset to sunset? Day Noon to noon – The seasonal motion of the Sun changes its rise and set times, so sunrise to sunrise would be a variable measure. Noon to noon is far more constant. Noon: time of the Sun’s transit of the meridian Stellarium View and measure a day Day Aday is caused by Earth’s motion: spinning on an axis and orbiting around the Sun. Earth’s spin is very regular (daily variations on the order of a few milliseconds, due to internal rearrangement of Earth’s mass and external gravitational forces primarily from the Moon and Sun). Synodic Day Noon to noon = synodic or solar day (point 1 to 3). This is not the time for one complete spin of Earth (1 to 2). Because Earth also orbits at the same time as it is spinning, it takes a little extra time for the Sun to come back to noon after one complete spin. Because the orbit is elliptical, when Earth is closest to the Sun it is moving faster, and it takes longer to bring the Sun back around to noon. When Earth is farther it moves slower and it takes less time to rotate the Sun back to noon. Mean Solar Day is an average of the amount time it takes to go from noon to noon throughout an orbit = 24 Hours Real solar day varies by up to 30 seconds depending on the time of year. -
September 2019
JUDICIAL COUNCIL OF CALIFORNIA 455 Golden Gate Avenue . San Francisco, California 94102-3688 www.courts.ca.gov REPORT TO THE JUDICI AL COUNCIL For business meeting on: September 23–24, 2019 Title Agenda Item Type Judicial Workload Assessment: 2018 Judicial Action Required Workload Study Updated Caseweights Effective Date Rules, Forms, Standards, or Statutes Affected September 24, 2019 None Date of Report Recommended by September 10, 2019 Workload Assessment Advisory Committee Hon. Lorna A. Alksne, Chair Contact Judicial Council staff Kristin Greenaway, 415-865-7832 Kristin Greenaway, Supervising Research [email protected] Analyst Office of Court Research Executive Summary The Workload Assessment Advisory Committee (WAAC) recommends that the Judicial Council adopt the proposed Judicial Workload Study updated model parameters that are used as part of the formula for assessing judicial need in the trial courts. The council previously approved the Judicial Workload Study in 2001 and 2011; the current update accounts for changes in the law and practice that have affected judicial workload since the last study update in 2011. The recommendation also reflects direction from the Judicial Council, at its July 18, 2019 meeting, to perform additional analysis to ensure the model best represents courts of all sizes. Further, WAAC recommends that the council approve an updated Judicial Needs Assessment per Government Code section 69614(c)(1) based on the new judicial workload measures and the established methodology for prioritization of judgeships. The updated needs assessment would replace a preliminary version that was completed in 2018 using workload measures developed in 2011. Recommendation The Workload Assessment Advisory Committee recommends that the Judicial Council: 1. -
Before the Washington Utilities and Transportation Commission
BEFORE THE WASHINGTON UTILITIES AND TRANSPORTATION COMMISSION In the Matter of Puget Sound Energy DOCKET UE-171087 2018-2019 Biennial Conservation Plan ____________________________________ In the Matter of Avista Corporation 2018- DOCKET UE-171091 2019 Biennial Conservation Plan ____________________________________ In the Matter of Pacific Power and Light Company 2018-2019 Biennial DOCKET UE-171092 Conservation Plan COMMISSION STAFF COMMENTS REGARDING ELECTRIC UTILITY CONSERVATION PLANS UNDER THE ENERGY INDEPENDENCE ACT, RCW 19.285 and WAC 480-109 (2018-2019 BIENNIAL CONSERVATION PLANS) December 1, 2017 Dockets UE-171087, UE-171091, UE-171092 Staff Comments on 2018-2019 Biennial Conservation Plans Page i Contents Introduction ..................................................................................................................................... 3 Target Setting and Implementation Plans ....................................................................................... 4 NEEA........................................................................................................................................... 4 Decoupling Calculation .............................................................................................................. 6 Rebate Incentive Level ................................................................................................................ 7 Hard to Reach Markets ............................................................................................................... 7 Additional -
Sidereal Time 1 Sidereal Time
Sidereal time 1 Sidereal time Sidereal time (pronounced /saɪˈdɪəri.əl/) is a time-keeping system astronomers use to keep track of the direction to point their telescopes to view a given star in the night sky. Just as the Sun and Moon appear to rise in the east and set in the west, so do the stars. A sidereal day is approximately 23 hours, 56 minutes, 4.091 seconds (23.93447 hours or 0.99726957 SI days), corresponding to the time it takes for the Earth to complete one rotation relative to the vernal equinox. The vernal equinox itself precesses very slowly in a westward direction relative to the fixed stars, completing one revolution every 26,000 years approximately. As a consequence, the misnamed sidereal day, as "sidereal" is derived from the Latin sidus meaning "star", is some 0.008 seconds shorter than the earth's period of rotation relative to the fixed stars. The longer true sidereal period is called a stellar day by the International Earth Rotation and Reference Systems Service (IERS). It is also referred to as the sidereal period of rotation. The direction from the Earth to the Sun is constantly changing (because the Earth revolves around the Sun over the course of a year), but the directions from the Earth to the distant stars do not change nearly as much. Therefore the cycle of the apparent motion of the stars around the Earth has a period that is not quite the same as the 24-hour average length of the solar day. Maps of the stars in the night sky usually make use of declination and right ascension as coordinates. -
Astronomical Time Keeping file:///Media/TOSHIBA/Times.Htm
Astronomical Time Keeping file:///media/TOSHIBA/times.htm Astronomical Time Keeping Introduction Siderial Time Solar Time Universal Time (UT), Greenwich Time Timezones Atomic Time Ephemeris Time, Dynamical Time Scales (TDT, TDB) Julian Day Numbers Astronomical Calendars References Introduction: Time keeping and construction of calendars are among the oldest branches of astronomy. Up until very recently, no earth-bound method of time keeping could match the accuracy of time determinations derived from observations of the sun and the planets. All the time units that appear natural to man are caused by astronomical phenomena: The year by Earth's orbit around the Sun and the resulting run of the seasons, the month by the Moon's movement around the Earth and the change of the Moon phases, the day by Earth's rotation and the succession of brightness and darkness. If high precision is required, however, the definition of time units appears to be problematic. Firstly, ambiguities arise for instance in the exact definition of a rotation or revolution. Secondly, some of the basic astronomical processes turn out to be uneven and irregular. A problem known for thousands of years is the non-commensurability of year, month, and day. Neither can the year be precisely expressed as an integer number of months or days, nor does a month contain an integer number of days. To solves these problems, a multitude of time scales and calenders were devised of which the most important will be described below. Siderial Time The siderial time is deduced from the revolution of the Earth with respect to the distant stars and can therefore be determined from nightly observations of the starry sky.