Division a / Functional Working Group Time Metrology Standards (Tms) Standards De Metrologie´ Du Temps
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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): -
The Iberoamerican Contribution To
RevMexAA (Serie de Conferencias), 25, 21{23 (2006) THE IBEROAMERICAN CONTRIBUTION TO INTERNATIONAL TIME KEEPING E. F. Arias1,2 RESUMEN Las escalas internacionales de tiempo, Tiempo At´omico Internacional (TAI) y Tiempo Universal Coordinado (UTC), son elaboradas en el Bureau Internacional des Poids et Mesures (BIPM), gracias a la contribuci´on de 57 laboratorios de tiempo nacionales que mantienen controles locales de UTC. La contribuci´on iberoamericana al c´alculo de TAI ha aumentado en los ultimos´ anos.~ Diez laboratorios en las Am´ericas y uno en Espana~ contribuyen a la estabilidad de TAI con el aporte de datos de relojes at´omicos industriales; una fuente de cesio mantenida en uno de ellos contribuye a mejorar la exactitud de TAI. Este art´ıculo resume las caracter´ısticas de las escalas de tiempo de referencia y describe la contribuci´on de los laboratorios iberoamericanos. ABSTRACT The international time scales, International Atomic Time (TAI) and Coordinated Universal Time (UTC), are elaborated at the Bureau International des Poids et Mesures (BIPM), thanks to the contribution of 57 national time laboratories that maintain local realizations of UTC. The Iberoamerican contribution to TAI has increased in the last years. Ten laboratories in America and one in Spain participate to the calculation of TAI , increasing its stability with the data of industrial atomic clocks and improving its accuracy with frequency measurements of a caesium source developed and maintained at one laboratory. This paper summarizes the characteristics of the reference time scales and describes the contributions of the Iberoamerican time laboratories to them. Key Words: TIME | REFERENCE SYSTEMS 1. -
IEEE Standard Definitions of Physical Quantities for Fundamental Frequency and Time Metrology—Random Instabilities
IEEE Standard Definitions of Physical Quantities for Fundamental Frequency and Time Metrology—Random Instabilities IEEE Standards Coordinating Committee 27 Sponsored by the IEEE Standards Coordinating Committee 27 on Time and Frequency TM IEEE 1139 3 Park Avenue IEEE Std 1139™-2008 New York, NY 10016-5997, USA (Revision of IEEE Std 1139-1999) 27 February 2009 Authorized licensed use limited to: Johns Hopkins University. Downloaded on March 07,2019 at 15:29:34 UTC from IEEE Xplore. Restrictions apply. Authorized licensed use limited to: Johns Hopkins University. Downloaded on March 07,2019 at 15:29:34 UTC from IEEE Xplore. Restrictions apply. IEEE Std 1139™-2008 (Revision of IEEE Std 1139-1999) IEEE Standard Definitions of Physical Quantities for Fundamental Frequency and Time Metrology—Random Instabilities Sponsor IEEE Standards Coordinating Committee 27 on Time and Frequency Approved 26 September 2008 IEEE-SA Standards Board Authorized licensed use limited to: Johns Hopkins University. Downloaded on March 07,2019 at 15:29:34 UTC from IEEE Xplore. Restrictions apply. Abstract: Methods of describing random instabilities of importance to frequency and time metrology are covered. Quantities covered include frequency, amplitude, and phase instabilities; spectral densities of frequency, amplitude, and phase fluctuations; and time-domain deviations of frequency fluctuations. In addition, recommendations are made for the reporting of measurements of frequency, amplitude, and phase instabilities, especially in regard to the recording of experimental parameters, experimental conditions, and calculation techniques. Keywords: AM noise, amplitude instability, FM noise, frequency domain, frequency instability, frequency metrology, frequency modulation, noise, phase instability, phase modulation, phase noise, PM noise, time domain, time metrology • The Institute of Electrical and Electronics Engineers, Inc. -
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. -
Governing the Time of the World Written by Tim Stevens
Governing the Time of the World Written by Tim Stevens This PDF is auto-generated for reference only. As such, it may contain some conversion errors and/or missing information. For all formal use please refer to the official version on the website, as linked below. Governing the Time of the World https://www.e-ir.info/2016/08/07/governing-the-time-of-the-world/ TIM STEVENS, AUG 7 2016 This is an excerpt from Time, Temporality and Global Politics – an E-IR Edited Collection. Available now on Amazon (UK, USA, Ca, Ger, Fra), in all good book stores, and via a free PDF download. Find out more about E-IR’s range of open access books here Recent scholarship in International Relations (IR) is concerned with how political actors conceive of time and experience temporality and, specifically, how these ontological and epistemological considerations affect political theory and practice (Hutchings 2008; Stevens 2016). Drawing upon diverse empirical and theoretical resources, it emphasises both the political nature of ‘time’ and the temporalities of politics. This chronopolitical sensitivity augments our understanding of international relations as practices whose temporal dimensions are as fundamental to their operations as those revealed by more established critiques of spatiality, materiality and discourse (see also Klinke 2013). This transforms our understanding of time as a mere backdrop to ‘history’ and other core concerns of IR (Kütting 2001) and provides opportunities to reflect upon the constitutive role of time in IR theory itself (Berenskoetter 2011; Hom and Steele 2010; Hutchings 2007; McIntosh 2015). One strand of IR scholarship problematises the historical emergence of a hegemonic global time that subsumed within it local and indigenous times to become the time by which global trade and communications are transacted (Hom 2010, 2012). -
Mutual Benefits of Timekeeping and Positioning
Tavella and Petit Satell Navig (2020) 1:10 https://doi.org/10.1186/s43020-020-00012-0 Satellite Navigation https://satellite-navigation.springeropen.com/ REVIEW Open Access Precise time scales and navigation systems: mutual benefts of timekeeping and positioning Patrizia Tavella* and Gérard Petit Abstract The relationship and the mutual benefts of timekeeping and Global Navigation Satellite Systems (GNSS) are reviewed, showing how each feld has been enriched and will continue to progress, based on the progress of the other feld. The role of GNSSs in the calculation of Coordinated Universal Time (UTC), as well as the capacity of GNSSs to provide UTC time dissemination services are described, leading now to a time transfer accuracy of the order of 1–2 ns. In addi- tion, the fundamental role of atomic clocks in the GNSS positioning is illustrated. The paper presents a review of the current use of GNSS in the international timekeeping system, as well as illustrating the role of GNSS in disseminating time, and use the time and frequency metrology as fundamentals in the navigation service. Keywords: Atomic clock, Time scale, Time measurement, Navigation, Timekeeping, UTC Introduction information. Tis is accomplished by a precise connec- Navigation and timekeeping have always been strongly tion between the GNSS control centre and some of the related. Te current GNSSs are based on a strict time- national laboratories that participate to UTC and realize keeping system and the core measure, the pseudo-range, their real-time local approximation of UTC. is actually a time measurement. To this aim, very good Tese features are reviewed in this paper ofering an clocks are installed on board GNSS satellites, as well as in overview of the mutual advantages between navigation the ground stations and control centres. -
Time Metrology in Galileo.Pdf
Time Metrology in the Galileo Navigation System The Experience of the Italian National Metrology Institute I.Sesia, G.Signorile, G.Cerretto, E.Cantoni, P.Tavella A.Cernigliaro, A.Samperi Optics Division, INRiM, Turin, Italy DASS Division, aizoOn, Turin, Italy [email protected] [email protected], [email protected] Abstract—Timekeeping is crucial in Global Navigation system, the research on new clock technologies, calibrations, Satellite Systems (GNSS), being the positioning accuracy directly evaluation of uncertainty, and dissemination of accurate time. related to a time measurement. As a consequence, the typical expertise of time metrology laboratories is necessary in many This paper presents the experience of the Italian National different aspects of a navigation system. This paper presents the Institute of Metrological Research (INRiM) time laboratory in experience of INRIM in the development of the Galileo the Galileo experimental and validation phases. navigation system from the earlier studies till the very recent In Orbit Validation phase showing how the time metrology practice II. THE GALILEO EXPERIENCE has been useful in the understanding of time aspects of INRiM has been involved in the Galileo system since 1999 navigation and showing as well how the navigation service and participated to different phases of the project. perspective has stimulated new ideas and better understanding of time measures. The first experimental phase was the Galileo System Test Bed Version 1 (GSTB V1) in 2002 in which INRiM participated, Keywords—time metrology; atomic clocks; steering; time together with the British NPL and the German PTB scales; GNSS timing; timekeeping; space clocks; system noise laboratories, to generate the experimental Galileo System Time, the reference time scale of the system, obtained from the I. -
TIME 1. Introduction 2. Time Scales
TIME 1. Introduction The TCS requires access to time in various forms and accuracies. This document briefly explains the various time scale, illustrate the mean to obtain the time, and discusses the TCS implementation. 2. Time scales International Atomic Time (TIA) is a man-made, laboratory timescale. Its units the SI seconds which is based on the frequency of the cesium-133 atom. TAI is the International Atomic Time scale, a statistical timescale based on a large number of atomic clocks. Coordinated Universal Time (UTC) – UTC is the basis of civil timekeeping. The UTC uses the SI second, which is an atomic time, as it fundamental unit. The UTC is kept in time with the Earth rotation. However, the rate of the Earth rotation is not uniform (with respect to atomic time). To compensate a leap second is added usually at the end of June or December about every 18 months. Also the earth is divided in to standard-time zones, and UTC differs by an integral number of hours between time zones (parts of Canada and Australia differ by n+0.5 hours). You local time is UTC adjusted by your timezone offset. Universal Time (UT1) – Universal time or, more specifically UT1, is counted from 0 hours at midnight, with unit of duration the mean solar day, defined to be as uniform as possible despite variations in the rotation of the Earth. It is observed as the diurnal motion of stars or extraterrestrial radio sources. It is continuous (no leap second), but has a variable rate due the Earth’s non-uniform rotational period. -
Earth Rotation Changes Since −500 CE Driven by Ice Mass Variations ∗ Carling Hay A,B, , Jerry X
Earth and Planetary Science Letters 448 (2016) 115–121 Contents lists available at ScienceDirect Earth and Planetary Science Letters www.elsevier.com/locate/epsl Earth rotation changes since −500 CE driven by ice mass variations ∗ Carling Hay a,b, , Jerry X. Mitrovica b, Eric Morrow a, Robert E. Kopp a,c, Peter Huybers b, Richard B. Alley d a Department of Earth and Planetary Sciences and Institute of Earth, Ocean, and Atmospheric Sciences, Rutgers University, Piscataway, NJ, 08854, USA b Department of Earth and Planetary Sciences, Harvard University, 20 Oxford Street, Cambridge, MA, 02138, USA c Rutgers Energy Institute, Rutgers University, New Brunswick, NJ, 08901, USA d Department of Geosciences and Earth and Environmental Systems Institute, Pennsylvania State University, University Park, PA, 16802, USA a r t i c l e i n f o a b s t r a c t Article history: We predict the perturbation to the Earth’s length-of-day (LOD) over the Common Era using a recently Received 1 October 2015 derived estimate of global sea-level change for this time period. We use this estimate to derive a time Received in revised form 24 March 2016 series of “clock error”, defined as the difference in timing of two clocks, one based on a theoretically Accepted 13 May 2016 invariant time scale (terrestrial time) and one fixed to Earth rotation (universal time), and compare this Available online 30 May 2016 time series to millennial scale variability in clock error inferred from ancient eclipse records. Under the Editor: B. Buffett assumption that global sea-level change over the Common Era is driven by ice mass flux alone, we Keywords: find that this flux can reconcile a significant fraction of the discrepancies between clock error computed sea level assuming constant slowing of Earth’s rotation and that inferred from eclipse records since 700 CE. -
Chapter I. Solar and Lunar Eclipses 6 1.1
1 ANCIENT RIDDLES OF SOLAR ECLIPSES. Asymmetric Astronomy Second Edition By IGOR N. TAGANOV and VILLE-V.E. SAARI Russian Academy of Sciences Saint Petersburg 2016 2 Taganov, Igor N., Saari, Ville-V.E. Ancient Riddles of Solar Eclipses. Asymmetric Astronomy. Second Edition – Saint Petersburg: TIN, 2016. – 110 p., 53 ill. Electronic Edition ISBN 978-5-902632-28-3 © Taganov, Igor N.; Saari, Ville-V.E. 2016 The book examines some of the mysteries of ancient astronomical treatises, for example, known since the Middle Ages the “Wednesday paradox”, and the history of the emergence and spread in the East of the belief that the eclipses of the Sun and the Moon, as well as all the Universe geometry are defined by a single sacred number 108. The calendar cycles of solar eclipses, considered in the book, confirming the old assumption of Indian and Chinese astronomers in 6-8 centuries, show that the probability of a total solar eclipse is larger in the spring and summer months, and the probability of annular eclipse, on the contrary, is larger in the autumn and winter months. Analysis of ancient chronicles of solar and lunar eclipses discovers evidence of gradual deceleration of time, which is confirmed by modern astronomical observations of the orbital movement of the Earth, the Moon, Mercury and Venus. The cosmological deceleration of time is a consequence of the irreversibility of “physical” time, which leads to the fact that all the characteristic time intervals are shorter in the past than in the future. In theoretical cosmology, the use of the concept of decelerating physical time allows to represent the key cosmological parameters of the observable Universe in the form of simple functions of the fundamental physical constants. -
IAU) and Time
The relationships between The International Astronomical Union (IAU) and time Nicole Capitaine IAU Representative in the CCU Time and astronomy: a few historical aspects Measurements of time before the adoption of atomic time - The time based on the Earth’s rotation was considered as being uniform until 1935. - Up to the middle of the 20th century it was determined by astronomical observations (sidereal time converted to mean solar time, then to Universal time). When polar motion within the Earth and irregularities of Earth’s rotation have been known (secular and seasonal variations), the astronomers: 1) defined and realized several forms of UT to correct the observed UT0, for polar motion (UT1) and for seasonal variations (UT2); 2) adopted a new time scale, the Ephemeris time, ET, based on the orbital motion of the Earth around the Sun instead of on Earth’s rotation, for celestial dynamics, 3) proposed, in 1952, the second defined as a fraction of the tropical year of 1900. Definition of the second based on astronomy (before the 13th CGPM 1967-1968) definition - Before 1960: 1st definition of the second The unit of time, the second, was defined as the fraction 1/86 400 of the mean solar day. The exact definition of "mean solar day" was left to astronomers (cf. SI Brochure). - 1960-1967: 2d definition of the second The 11th CGPM (1960) adopted the definition given by the IAU based on the tropical year 1900: The second is the fraction 1/31 556 925.9747 of the tropical year for 1900 January 0 at 12 hours ephemeris time. -
Metrology with Trapped Atoms on a Chip Using Non-Degenerate and Degenerate Quantum Gases Vincent Dugrain
Metrology with trapped atoms on a chip using non-degenerate and degenerate quantum gases Vincent Dugrain To cite this version: Vincent Dugrain. Metrology with trapped atoms on a chip using non-degenerate and degenerate quantum gases. Quantum Gases [cond-mat.quant-gas]. Université Pierre & Marie Curie - Paris 6, 2012. English. tel-02074807 HAL Id: tel-02074807 https://hal.archives-ouvertes.fr/tel-02074807 Submitted on 20 Mar 2019 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. LABORATOIRE KASTLER BROSSEL LABORATOIRE DES SYSTEMES` DE REF´ ERENCE´ TEMPS{ESPACE THESE` DE DOCTORAT DE L'UNIVERSITE´ PIERRE ET MARIE CURIE Sp´ecialit´e: Physique Quantique Ecole´ doctorale de Physique de la R´egionParisienne - ED 107 Pr´esent´eepar Vincent Dugrain Pour obtenir le grade de DOCTEUR de l'UNIVERSITE´ PIERRE ET MARIE CURIE Sujet : Metrology with Trapped Atoms on a Chip using Non-degenerate and Degenerate Quantum Gases Soutenue le 21 D´ecembre 2012 devant le jury compos´ede: M. Djamel ALLAL Examinateur M. Denis BOIRON Rapporteur M. Fr´ed´eric CHEVY Pr´esident du jury M. Jozsef FORTAGH Rapporteur M. Jakob REICHEL Membre invit´e M Peter ROSENBUSCH Examinateur Remerciements Mes premiers remerciements s'adressent `ames deux encadrants de th`ese,Jakob Reichel et Peter Rosenbusch.