The Marine Chronometer (Edited from Wikipedia)
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Measurement of Time
Measurement of Time M.Y. ANAND, B.A. KAGALI* Department of Physics, Bangalore University, Bangalore 560056 *email: [email protected] ABSTRACT Time was historically measured using the periodic motions of the sun and stars. Various types of sun clocks were devised in Egypt, Greece and Europe. Different types of water clocks were assembled with ever greater accuracy. Only in the seventeenth century did the mechanical clock with pendulums and springs appeared. Accurate quartz clocks and atomic clocks were developed in the first half of the twentieth century. Now we have clocks that have better than microsecond accuracy. This article gives a brief account of all these topics. Keywords: Sun clocks, Water clocks, Mechanical clocks, Quartz clocks, Atomic clocks, World Time, Indian Standard time We all know intuitively what time is. It can be civilizations relied upon the apparent motion of roughly equated with change or motions. From these bodies through the sky to determine the very beginning man has been interested in seasons, months, and years. understanding and measuring time. More We know little about the details of recently, he has been looking for ways to limit timekeeping in prehistoric eras, but we find the “damaging” effects of time and going that in every culture, some people were backward in time! preoccupied with measuring and recording the Celestial bodies—the Sun, Moon, planets, passage of time. Ice-age hunters in Europe over and stars—have provided us a reference for 20,000 years ago scratched lines and gouged measuring the passage of time. Ancient holes in sticks and bones, possibly counting the Physics Education • January − March 2007 277 days between phases of the moon. -
Floating and Platform Balances an Introduction
Floating and Platform Balances An introduction ©Darrah Artzner 3/2018 Floating and Platform Balances • Introduce main types • Discuss each in some detail including part identification and function • Testing and Inspecting • Cleaning tips • Lubrication • Performing repairs Balance Assembly Type Floating Platform Floating Balance Frame Spring stud Helicoid spring Hollow Tube Mounting Post Regulator Balance wheel Floating Balance cont. Jewel Roller Pin Paired weight Hollow Tube Safety Roller Pivot Wire Floating Balance cont. Example Retaining Hermle screws Safety Roller Note: moving fork Jewel cover Floating Balance cont. Inspecting and Testing (Balance assembly is removed from movement) • Inspect pivot (suspension) wire for distortion, corrosion, breakage. • Balance should appear to float between frame. Top and bottom distance. • Balance spring should be proportional and not distorted in any way. • Inspect jewels for cracks and or breakage. • Roller pin should be centered when viewed from front. (beat) • Rotate balance wheel three quarters of a turn (270°) and release. It should rotate smoothly with no distortion and should oscillate for several (3) minutes. Otherwise it needs attention. Floating Balance cont. Cleaning • Make sure the main spring has been let down before working on movement. • Use non-aqueous watch cleaner and/or rinse. • Agitate in cleaner/rinse by hand or briefly in ultrasonic. • Rinse twice and final in naphtha, Coleman fuel (or similar) or alcohol. • Allow to dry. (heat can be used with caution – ask me how I would do it.) Lubrication • There are two opinions. To lube or not to lube. • Place a vary small amount of watch oil on to the upper and lower jewel where the pivot wire passed through the jewel holes. -
QUICK REFERENCE GUIDE Latitude, Longitude and Associated Metadata
QUICK REFERENCE GUIDE Latitude, Longitude and Associated Metadata The Property Profile Form (PPF) requests the property name, address, city, state and zip. From these address fields, ACRES interfaces with Google Maps and extracts the latitude and longitude (lat/long) for the property location. ACRES sets the remaining property geographic information to default values. The data (known collectively as “metadata”) are required by EPA Data Standards. Should an ACRES user need to be update the metadata, the Edit Fields link on the PPF provides the ability to change the information. Before the metadata were populated by ACRES, the data were entered manually. There may still be the need to do so, for example some properties do not have a specific street address (e.g. a rural property located on a state highway) or an ACRES user may have an exact lat/long that is to be used. This Quick Reference Guide covers how to find latitude and longitude, define the metadata, fill out the associated fields in a Property Work Package, and convert latitude and longitude to decimal degree format. This explains how the metadata were determined prior to September 2011 (when the Google Maps interface was added to ACRES). Definitions Below are definitions of the six data elements for latitude and longitude data that are collected in a Property Work Package. The definitions below are based on text from the EPA Data Standard. Latitude: Is the measure of the angular distance on a meridian north or south of the equator. Latitudinal lines run horizontal around the earth in parallel concentric lines from the equator to each of the poles. -
Latitude/Longitude Data Standard
LATITUDE/LONGITUDE DATA STANDARD Standard No.: EX000017.2 January 6, 2006 Approved on January 6, 2006 by the Exchange Network Leadership Council for use on the Environmental Information Exchange Network Approved on January 6, 2006 by the Chief Information Officer of the U. S. Environmental Protection Agency for use within U.S. EPA This consensus standard was developed in collaboration by State, Tribal, and U. S. EPA representatives under the guidance of the Exchange Network Leadership Council and its predecessor organization, the Environmental Data Standards Council. Latitude/Longitude Data Standard Std No.:EX000017.2 Foreword The Environmental Data Standards Council (EDSC) identifies, prioritizes, and pursues the creation of data standards for those areas where information exchange standards will provide the most value in achieving environmental results. The Council involves Tribes and Tribal Nations, state and federal agencies in the development of the standards and then provides the draft materials for general review. Business groups, non- governmental organizations, and other interested parties may then provide input and comment for Council consideration and standard finalization. Standards are available at http://www.epa.gov/datastandards. 1.0 INTRODUCTION The Latitude/Longitude Data Standard is a set of data elements that can be used for recording horizontal and vertical coordinates and associated metadata that define a point on the earth. The latitude/longitude data standard establishes the requirements for documenting latitude and longitude coordinates and related method, accuracy, and description data for all places used in data exchange transaction. Places include facilities, sites, monitoring stations, observation points, and other regulated or tracked features. 1.1 Scope The purpose of the standard is to provide a common set of data elements to specify a point by latitude/longitude. -
Collectable POCKET Watches 1750-1920
cOLLECTABLE POCKET watches 1750-1920 Ian Beilby Clocks Magazine Beginner’s Guide Series No 5 cOLLECTABLE POCKET watches 1750-1920 Ian Beilby Clocks Magazine Beginner’s Guide Series No 5 Published by Splat Publishing Ltd. 141b Lower Granton Road Edinburgh EH5 1EX United Kingdom www.clocksmagazine.com © 2017 Ian Beilby World copyright reserved ISBN: 978-0-9562732-4-6 The right of Ian Beilby to be identified as author of this work has been asserted in accordance with the Copyright, Designs and Patents Act 1988. 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 permission of the publisher. 2 4 6 8 10 9 7 5 3 1 Printed by CBF Cheltenham Business Forms Ltd, 67 Hatherley Road, Cheltenham GL51 6EG CONTENTS Introduction 7 Chapter 1. The eighteenth century verge watch 13 Chapter 2. The nineteenth century verge watch 22 Chapter 3. The English cylinder and rack lever watch 36 Chapter 4. The English lever watch 42 Chapter 5. The Swiss lever watch 54 Chapter 6. The American lever watch 62 Chapter 7. The Swiss cylinder ladies’ fob watch 72 Chapter 8. Advice on collecting and maintenance 77 Appendix 1. Glossary 82 Appendix 2. Further reading 86 CLOCKS MAGAZINE BEGINNER’S GUIDE SERIES No. 1. Clock Repair, A Beginner’s Guide No. 2. Beginner’s Guide to Pocket Watches No. 3. American Clocks, An Introduction No. 4. What’s it Worth, Price Guide to Clocks 2014 No. -
Physics 2305 Lab 11: Torsion Pendulum
Name___________________ ID number_________________________ Date____________________ Lab partner_________________________ Lab CRN________________ Lab instructor_______________________ Physics 2305 Lab 11: Torsion Pendulum Objective 1. To demonstrate that the motion of the torsion pendulum satisfies the simple harmonic form in equation (3) 2. To show that the period (or angular frequency) of the simple harmonic motion of the torsion pendulum is independent of the amplitude of the motion 3. To make measurements to demonstrate the validity of equation (6), which relates the angular frequency of motion to the torsion constant and the moment of inertia of the torsion pendulum Useful background reading Young and Freedman, section 13.1, 13.2, 13.4 (the “angular SHM” section, specifically) Introduction A torsion pendulum is shown schematically to the right. A disk with moment of inertia I0 is fastened near the center of a long straight wire stretched between two fixed mounts. If the disk is rotated through an angle θ and released, the twist in the wire rotates the disk back toward equilibrium. It overshoots and I 0 oscillates back and forth like a pendulum, hence the name. Torsion pendulums are used for the timing element in some θ clocks. The most common variety is a decorative polished brass mechanism under a glass dome. You may have seen one. The balance wheel in an old fashioned mechanical watch is a kind of torsion pendulum, though the restoring force is provided by a flat coiled spring rather than a long twisted wire. Torsion pendulums can be made very accurate and have been used in numerous precision experiments in 1 physics. -
A Stability Analysis of Divergence Damping on a Latitude–Longitude Grid
2976 MONTHLY WEATHER REVIEW VOLUME 139 A Stability Analysis of Divergence Damping on a Latitude–Longitude Grid JARED P. WHITEHEAD Department of Mathematics, University of Michigan, Ann Arbor, Ann Arbor, Michigan CHRISTIANE JABLONOWSKI AND RICHARD B. ROOD Department of Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, Ann Arbor, Michigan PETER H. LAURITZEN Climate and Global Dynamics Division, National Center for Atmospheric Research,* Boulder, Colorado (Manuscript received 24 August 2010, in final form 25 March 2011) ABSTRACT The dynamical core of an atmospheric general circulation model is engineered to satisfy a delicate balance between numerical stability, computational cost, and an accurate representation of the equations of motion. It generally contains either explicitly added or inherent numerical diffusion mechanisms to control the buildup of energy or enstrophy at the smallest scales. The diffusion fosters computational stability and is sometimes also viewed as a substitute for unresolved subgrid-scale processes. A particular form of explicitly added diffusion is horizontal divergence damping. In this paper a von Neumann stability analysis of horizontal divergence damping on a latitude–longitude grid is performed. Stability restrictions are derived for the damping coefficients of both second- and fourth- order divergence damping. The accuracy of the theoretical analysis is verified through the use of idealized dynamical core test cases that include the simulation of gravity waves and a baroclinic wave. The tests are applied to the finite-volume dynamical core of NCAR’s Community Atmosphere Model version 5 (CAM5). Investigation of the amplification factor for the divergence damping mechanisms explains how small-scale meridional waves found in a baroclinic wave test case are not eliminated by the damping. -
RAMP: a Computer System for Mapping Regional Areas
RAMP: a computer system for mapping regional areas Bradley B. Nickey PACIFIC SOUTHWEST Forest and Range Experiment Station FOREST SERVICE lJ S DEPARTMENT OF AGRICULTURE P.O. BOX 245, BERKELEY, CALIFORNIA 94701 USDA FOREST SERVICE GENERAL TECHNICAL REPORT PSW-12 11975 CONTENTS Page Introduction ........................................... 1 Individual Fire Reports ................................... 1 RAMP ................................................ 2 Digitization Requirements ................................. 2 Accuracy .............................................. 2 Computer Software ...................................... 2 Computer Operations .................................... 4 Converting Coordinates ................................ 4 Aligning Coordinates .................................. 4 Mapping Sections ..................................... 6 Application ............................................ 8 Literature Cited ......................................... 9 Nickey, Bradley B. 1975. RAMP: a computer system for mapping regional areas. USDA Forest Serv. Gen. Tech. Rep. PSW-12, 9 p., illus. Pacific Southwest Forest and Range Exp. Stn., Berkeley, Calif. Until 1972, the U.S. Forest Service's Individual Fire Reports recorded locations by the section-township-range system..These earlier fire reports, therefore, lacked congruent locations. RAMP (Regional Area Mapping Pro- cedure) was designed to make the reports more useful for quantitative analysis. This computer-based technique converts locations expressed in section-township-range -
GMT and Longitude by Lunar Distance: Two Methods Compared from a Practitioner’S Point of View
THE JOURNAL OF NAVIGATION (2019), 72, 1660–1664. c The Royal Institute of Navigation 2019 doi:10.1017/S0373463319000341 FORUM GMT and Longitude by Lunar Distance: Two Methods Compared From a Practitioner’s Point of View Eric Romelczyk (E-mail: [email protected]) This article discusses the technique of observing lunar distance - that is, angular distance between the moon and another celestial body - to establish universal time and longitude, from a practitioner’s point of view. The article presents a brief overview of the principles underlying the lunar distance observation and its use in celestial navigation. A discussion follows of two different methods for finding universal time by observing lunar distance, Dr. Wendel Brunner’s calculator-based method and the specialised inspection tables created by Bruce Stark. The article compares the two methods against each other for ease of use and accuracy. The author concludes that either method will provide satisfactory results, but that the technique of observing lunar dis- tance is unlikely to regain relevance in the modern-day practice of navigation and is primarily useful as a skill-building exercise in making sextant observations. KEYWORDS 1. Navigation. 2. History. 3. Nautical. 4. Time. Submitted: 8 August 2018. Accepted: 14 April 2019. First published online: 2 May 2019. 1. INTRODUCTION. 1.1. History of the lunar distance method. For centuries of seafaring history, a method for accurately measuring time to the degree of precision necessary to establish the navigator’s longitude was out of reach for practical purposes. It had been understood since the mid-16th century that the navigator’s longitude could be established either by reference to the moon’s angular distance from other celestial bodies - the “lunar distance”, measured by careful sextant observations - or by reference to a timepiece of sufficient accuracy. -
Spherical Coordinate Systems
Spherical Coordinate Systems Exploring Space Through Math Pre-Calculus let's examine the Earth in 3-dimensional space. The Earth is a large spherical object. In order to find a location on the surface, The Global Pos~ioning System grid is used. The Earth is conventionally broken up into 4 parts called hemispheres. The North and South hemispheres are separated by the equator. The East and West hemispheres are separated by the Prime Meridian. The Geographic Coordinate System grid utilizes a series of horizontal and vertical lines. The horizontal lines are called latitude lines. The equator is the center line of latitude. Each line is measured in degrees to the North or South of the equator. Since there are 360 degrees in a circle, each hemisphere is 180 degrees. The vertical lines are called longitude lines. The Prime Meridian is the center line of longitude. Each hemisphere either East or West from the center line is 180 degrees. These lines form a grid or mapping system for the surface of the Earth, This is how latitude and longitude lines are represented on a flat map called a Mercator Projection. Lat~ude , l ong~ude , and elevalion allows us to uniquely identify a location on Earth but, how do we identify the pos~ion of another point or object above Earth's surface relative to that I? NASA uses a spherical Coordinate system called the Topodetic coordinate system. Consider the position of the space shuttle . The first variable used for position is called the azimuth. Azimuth is the horizontal angle Az of the location on the Earth, measured clockwise from a - line pointing due north. -
Observed Time Difference of Arrival (OTDOA) Positioning in 3GPP LTE
Observed Time Difference Of Arrival (OTDOA) Positioning in 3GPP LTE by Sven Fischer June 6, 2014 © 2014 Qualcomm Technologies, Inc. Contents 1 Scope ................................................................................................................ 7 2 References ....................................................................................................... 8 3 Definitions and Abbreviations ........................................................................ 9 3.1 Definitions .................................................................................................................... 9 3.2 Abbreviations .............................................................................................................. 10 4 Multilateration in OTDOA Positioning ......................................................... 12 4.1 Introduction ................................................................................................................. 12 4.2 Reference Signal Time Difference Measurement (RSTD) ......................................... 13 4.2.1 Definition ......................................................................................................... 13 4.2.2 RSTD Measurement Report Mapping ............................................................. 13 4.3 Basic OTDOA Navigation Equations ......................................................................... 13 5 Positioning Reference Signals (PRS) .......................................................... 15 5.1 Overview .................................................................................................................... -
A Short Guide to Celestial Navigation5.16 MB
A Short Guide to elestial Na1igation Copyright A 1997 2011 (enning -mland Permission is granted to copy, distribute and/or modify this document under the terms of the G.2 Free Documentation -icense, 3ersion 1.3 or any later version published by the Free 0oftware Foundation% with no ,nvariant 0ections, no Front Cover 1eIts and no Back Cover 1eIts. A copy of the license is included in the section entitled "G.2 Free Documentation -icense". ,evised October 1 st , 2011 First Published May 20 th , 1997 .ndeB 1reface Chapter 1he Basics of Celestial ,aEigation Chapter 2 Altitude Measurement Chapter 3 )eographic .osition and 1ime Chapter 4 Finding One's .osition 0ight Reduction) Chapter 5 Finding the .osition of an Advancing 2essel Determination of Latitude and Longitude, Direct Calculation of Chapter 6 .osition Chapter 7 Finding 1ime and Longitude by Lunar Distances Chapter 8 Rise, 0et, 1wilight Chapter 9 )eodetic Aspects of Celestial ,aEigation Chapter 0 0pherical 1rigonometry Chapter 1he ,aEigational 1riangle Chapter 12 )eneral Formulas for ,aEigation Chapter 13 Charts and .lotting 0heets Chapter 14 Magnetic Declination Chapter 15 Ephemerides of the 0un Chapter 16 ,aEigational Errors Chapter 17 1he Marine Chronometer AppendiB -02 ,ree Documentation /icense Much is due to those who first bro-e the way to -now.edge, and .eft on.y to their successors the tas- of smoothing it Samue. Johnson Prefa e Why should anybody still practice celestial naRigation in the era of electronics and 18S? 7ne might as Sell ask Shy some photographers still develop black-and-Shite photos in their darkroom instead of using a digital camera.