It's About Time Notes
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
PHYS 633: Introduction to Stellar Astrophysics Spring Semester 2006 Rich Townsend ([email protected])
PHYS 633: Introduction to Stellar Astrophysics Spring Semester 2006 Rich Townsend ([email protected]) Governing Equations In the foregoing analysis, we have seen how a star usually maintains a state of hydrostatic equilibrium. We have seen how the energy created in the star through nuclear reactions, or released through contraction, makes its way out in the form of the star’s luminosity. We have seen how the physical processes responsible for transporting this energy can either be radiation or convection. And, finally, we have seen how nuclear reactions within the star, and transport processes such as convective mixing, can alter the stars chemical composition. These four key pieces of physics lead to 3 + I of the differential equations governing stellar structure (here, I is the number of elements whose evolution we are following). Let’s quickly review these equations. First, we have the most general (spherically-symmetric) form for the equation governing momen- tum conservation, ∂P Gm 1 ∂2r = − − . (1) ∂m 4πr2 4πr2 ∂t2 If the second term on the right-hand side vanishes, then we recover the equation of hydrostatic equilibrium, expressed in Lagrangian form (i.e., derivatives with respect to the mass coordinate m, rather than the radial coordinate r). If this term does not vanish at some point in the star, then the mass shells at that point will being to expand or contract, with an acceleration given by ∂2r/∂t2. Second, we have the most general form for the energy conservation equation, ∂l ∂T δ ∂P = − − c + . (2) ∂m ν P ∂t ρ ∂t The first and second terms on the right-hand side come from nuclear energy gen- eration and neutrino losses, respectively. -
Used Time Scales GEORGE E
PROCEEDINGS OF THE IEEE, VOL. 55, NO. 6, JIJNE 1967 815 Reprinted from the PROCEEDINGS OF THE IEEI< VOL. 55, NO. 6, JUNE, 1967 pp. 815-821 COPYRIGHT @ 1967-THE INSTITCJTE OF kECTRITAT. AND ELECTRONICSEN~INEERS. INr I’KINTED IN THE lT.S.A. Some Characteristics of Commonly Used Time Scales GEORGE E. HUDSON A bstract-Various examples of ideally defined time scales are given. Bureau of Standards to realize one international unit of Realizations of these scales occur with the construction and maintenance of time [2]. As noted in the next section, it realizes the atomic various clocks, and in the broadcast dissemination of the scale information. Atomic and universal time scales disseminated via standard frequency and time scale, AT (or A), with a definite initial epoch. This clock time-signal broadcasts are compared. There is a discussion of some studies is based on the NBS frequency standard, a cesium beam of the associated problems suggested by the International Radio Consultative device [3]. This is the atomic standard to which the non- Committee (CCIR). offset carrier frequency signals and time intervals emitted from NBS radio station WWVB are referenced ; neverthe- I. INTRODUCTION less, the time scale SA (stepped atomic), used in these emis- PECIFIC PROBLEMS noted in this paper range from sions, is only piecewise uniform with respect to AT, and mathematical investigations of the properties of in- piecewise continuous in order that it may approximate to dividual time scales and the formation of a composite s the slightly variable scale known as UT2. SA is described scale from many independent ones, through statistical in Section 11-A-2). -
Prague & Munich
Prague & Munich combo weekend! A chance to enjoy two of the most beauful, historic and largest beer consuming places on the planet in one weekend! Prague - The golden city, incredible architecture and sights, Charles bridge, Prague castle (the largest in the world), the ancient Jewish quarter, Easter European prices, Starbucks and other western food chains, wild nightlife & Czech Beer (pints for $1). Surely one of the most intriguing cies in the world as well as one of the most excing in Europe, Prague is a trip not to be missed! Munich - The land of lederhosen, pretzels and beer – and Oktoberfest! This famous Bavarian city as all of the culture, history, museums and of course beer to make it one of the world’s greatest cies! Munich’s reputaon for being Europe’s most fun city is well-deserved, as no maRer what season or me of year, there’s always a reason for a celebraon! Country: Prague - Czech Republic (Czechia); Munich - Germany Language Prague - Czech; Munich - German Currency Prague - Czech Koruna; Munich - Euro Typical Cuisine Prague - Pork, beef, dumplings, potatoes, beer hot spiced wine, Absinthe, Czech Beer. Munich - wurst (sausage), Pretzels, krautsalat (sauerkrautsalad), kartoffelsalat (potato salad) schweinshaxe (roasted pork knuckle), schnitzel, hendl (roasted chicken), strudels, schnapps, beer. Old Town Square, Lennon Wall, Wenceslas Square, Jewish Quarter, Astronomical Clock, Charles Bridge, Prague Castle. Must see: Prague - Old Town Square, Lennon Wall, Wenceslas Square, Jewish Quarter, Astronomical Clock, Charles Bridge, Prague Castle.. Munich - Horauhaus, Glockenspiel, English gardens, Beer Gardens DEPARTURE TIMES DEPARTURE CITIES Thursday Florence Florence - 8:00 pm Rome Rome - 5:00 -5:30 pm Fly In - meet in Prague Sunday Return Florence - very late Sunday night Rome - very late Sunday night/ early Monday morning WWW.EUROADVENTURES.COM What’s included Full Package: Transportation Only Package: Fly In Package: - round trip transportaon - round trip transportaon - 2 nights accommodaon in Prague - 1 night accomm. -
A Study of Ancient Khmer Ephemerides
A study of ancient Khmer ephemerides François Vernotte∗ and Satyanad Kichenassamy** November 5, 2018 Abstract – We study ancient Khmer ephemerides described in 1910 by the French engineer Faraut, in order to determine whether they rely on observations carried out in Cambodia. These ephemerides were found to be of Indian origin and have been adapted for another longitude, most likely in Burma. A method for estimating the date and place where the ephemerides were developed or adapted is described and applied. 1 Introduction Our colleague Prof. Olivier de Bernon, from the École Française d’Extrême Orient in Paris, pointed out to us the need to understand astronomical systems in Cambo- dia, as he surmised that astronomical and mathematical ideas from India may have developed there in unexpected ways.1 A proper discussion of this problem requires an interdisciplinary approach where history, philology and archeology must be sup- plemented, as we shall see, by an understanding of the evolution of Astronomy and Mathematics up to modern times. This line of thought meets other recent lines of research, on the conceptual evolution of Mathematics, and on the definition and measurement of time, the latter being the main motivation of Indian Astronomy. In 1910 [1], the French engineer Félix Gaspard Faraut (1846–1911) described with great care the method of computing ephemerides in Cambodia used by the horas, i.e., the Khmer astronomers/astrologers.2 The names for the astronomical luminaries as well as the astronomical quantities [1] clearly show the Indian origin ∗F. Vernotte is with UTINAM, Observatory THETA of Franche Comté-Bourgogne, University of Franche Comté/UBFC/CNRS, 41 bis avenue de l’observatoire - B.P. -
Guidetour Berne FFI Clubs Switzerland Views of Old-Town By
Guidetour Berne FFI Clubs Switzerland Berne the capital of Sitzerland, is a small to medium sized city with a population of about 136,000 in the city proper and roughly 350,000 in the agglomeration area. It sits on a peninsula formed by the meandering turns of the river Aare. The remarkable design coherence of the Berne's old town has earned it a place on the UNESCO World Heritage List. It features 4 miles of arcaded walkways along streets decked out with fountains and clock-towers. Berne is home to the prestigious University of Berne which currently enrolls approximately 13,000 students. In addition, the city has the University of Applied Science also known as Berner Fachhochschule. There are also many vocational schools and an office of the Goethe Institut. Wikipedia Cc by and https://www.openstreetmap.org/#map=14/46.9419/7.4585 Views of old-town by train from Solothurn – Start in trainstation Christoffelturm The Christoffelturm was a tower built between the years 1344 and 1346. It was located in the old part of the Swiss city of Bern, in the upper section of Spitalgasse, near Holy Spirit Church. After a political decision on December 15, 1864, the Christoffelturm was removed by Gottlieb Ott, a Swiss building contractor. Ott began the destruction of the tower in spring of the following year. Bundeshaus (Federal Palace of Switzerland),The Swiss House of Parliaments is a representative building dominating the Square. Constructed by the end of 19th century. The Federal Palace refers to the building in Bern housing the Swiss Federal Assembly (legislature) and the Federal Council (executive). -
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. -
Eastern Europe and Baltic Countries
English Version EASTERN EUROPE AND BALTIC COUNTRIES GRAND TOUR OF POLAND IMPERIAL CAPITALS GRAND TOUR OF THE BALTIC COUNTRIES GDANSK MALBORK TORUN BELARUS GRAND TOUR OF POLAND WARSAW POLAND GERMANY WROCLAW CZESTOCHOWA KRAKOW CZECH REPUBLIC WIELICZKA AUSCHWITZ UKRAINE SLOVAKIA Tour of 10 days / 9 nights AUSTRIA DAY 1 - WARSAW Arrival in Warsaw and visit of the Polish capital, entirely rebuilt after the Second World War. Dinner and accommodation.SUISSE DAY 2 - WARSAW Visit of the historic center of Warsaw: the Jewish Quarter, Lazienkowski Palace, the Royal route. In the afternoon, visit of the WarsawMILANO Uprising Museum, dedicated to the revolt of the city during World War II. Dinner and accommodation. FRANCE DAY 3 - WARSAW / MALBORKGENOA / GDANSK PORTO FINO Departure for the Baltic Sea. Stop for a visit of the Ethnographic Museum with its typical architecture. Continue withNICE a visit of the Fortress of Malbork listed at the UNESCO World Heritage Site. Then, CANNES departure for Gdansk. Dinner and accommodation.ITALIE DAY 4 - GDANSK / GDNIA / SOPOT / GDANSK City tour of Gdansk. Go through the Golden Gate, a beautiful street with Renaissance and Baroque facades, terraces and typical markets, the Court of Arthus, the Neptune Fountain and finally the Basilica Sainte Marie. Continue to the famous resort of Sopot with its elegant houses, also known as the Monte Carlo of the Baltic Sea. Dinner and accommodation. DAY 5 - GDANSK / TORUN / WROCLAW Departure for Torun, located on the banks of the Vistula and hometown of the astronomer Nicolas Copernicus. Guided tour of the historical center and visit the house of Copernicus. Departure to Wroclaw. -
Brunnezytig 2014 1.Pdf
Bern, 14. März 2014 1/2014 BrunneBrunne Erscheint vierteljährlich 30. Jahrgang Offizielles Organ des Leist der Untern Stadt Bern, Kesslergass-Gesellschaft,ZytigZytig Rathausgass-Brunngass-Leist, Kramgassleist, Matte-Leist, Vereinigte Altstadtleiste 2 30 JAHRE BRUNNE ZYTIG Brunne Zytig, 14. März 2014 EDITORIAL Das ist lange her – oder doch nicht? Dreissig Jahre Brunne Zytig – lass mal rechnen: 1984 – wie war das damals, hier in der Unteren Altstadt? Alles besser? oder andersrum? Ich komme in’s Grübeln: Da war noch das Swiss- Chalet im Hotel Glocke, wo Peter Hinnen alles in Sachen Swiss-Folklore zum Besten gab. Der Mini- «Jungbrunnen» – hat Cornelia Koch, Altstadtbe- in den Gassen erleben. Ganz am Schluss des Ge- Shop, bei dem man Fernseher und Radios zur Re- wohnerin auch sie, ihre Illustration zum 30. Ge- burtstagsjahres werden wir dann noch ein wenig aus paratur bringen konnte, oder die Schlosserei burtstag der Brunne Zytig auf der Titelseite getauft. dem Brunne Zytigs-Nähkästchen plaudern – und Benoit, wo in der offenen Esse geschmiedet Wir nehmen diesen Titel als Kompliment und An- über künftige Herausforderungen, den «Jungbrun- wurde; wenn am Zytglogge-Uhrwerk etwas nicht sporn zugleich. Kompliment, weil unser Quartier- nen» dabei fest im Blick. mehr funktionierte, wurde das fehlerhafte Teil in blatt mit 30 im besten Alter ist und sich über die die Werkstatt getragen und fachgerecht repariert; Jahrzehnte zwar nicht ständig neu erfunden hat, aber Zum Auftakt unserer Themen-Reihe geht es in die- und Herr Joss – der Glaser bei Walther und Müller doch immer reichhaltiger geworden ist. Und quick- ser Ausgabe um das Wohnen in der Altstadt. Es ist – sagte zu unserem Sohn: «Wenn du den Rem- lebendig ist. -
Grade 6 Quarter 1 Lessons Ycsd.Pdf
Name__________________________________________________________________ th 6 Grade - Grading Period 1 Overview Ohio's New Learning Standards Minerals have specific, quantifiable properties. (6.ESS.1) Igneous, Metamorphic, and Sedimentary rocks have unique characteristics that can be used for identification and/or classification. (6.ESS.2) Igneous, Metamorphic, and Sedimentary rocks form in different ways. (6.ESS.3) Clear Learning Targets "I can": 1. _____ follow a laboratory procedure and work collaboratively within a group using appropriate scientific tools. 2. _____ work individually, with a partner, and as a team to test a scientific concept, change a variable, and record the experimental outcome. 3. _____ use the engineering design cycle to develop a solution with a predictable outcome. 4. _____ cite specific text or online resource to support a proposed design solution. 5. ____ identify minerals by testing their properties 6. ____ use mineral properties, to use in testing and identifying minerals. 7. ____ use the rock cycle to describe the formation of igneous, sedimentary and metamorphic rocks. 8. ____ identify the unique characteristics to classify rocks. 9. ____ describe the formation of igneous, metamorphic, and sedimentary rocks 10. ____ use the unique characteristic of sedimentary rocks to identify and classify sedimentary rocks. 11. ____ identify the characteristics/classify metamorphic rocks. 12. ____ describe how metamorphic rocks form. Name_________________________________________________________________ th 6 Grade - Grading -
Leap Second - Wikipedia
Leap second - Wikipedia https://en.wikipedia.org/wiki/Leap_second A leap second is a one-second adjustment that is occasionally applied to civil time Coordinated Universal Time (UTC) to keep it close to the mean solar time at Greenwich, in spite of the Earth's rotation slowdown and irregularities. UTC was introduced on 1972 January 1st, initially with a 10 second lag behind International Atomic Time (TAI). Since that date, 27 leap seconds have been inserted, the most recent on December 31, 2016 at 23:59:60 UTC, so in 2018, UTC lags behind TAI by an offset of 37 seconds.[1] The UTC time standard, which is widely used for international timekeeping and as the reference for civil time in most countries, uses the international system (SI) definition of the second. The UTC second Screenshot of the UTC clock from time.gov has been calibrated with atomic clock on the duration of the Earth's mean day of the astronomical year (https://time.gov/) during the leap second on 1900. Because the rotation of the Earth has since further slowed down, the duration of today's mean December 31, 2016. In the USA, the leap second solar day is longer (by roughly 0.001 seconds) than 24 SI hours (86,400 SI seconds). UTC would step took place at 19:00 local time on the East Coast, ahead of solar time and need adjustment even if the Earth's rotation remained constant in the future. at 16:00 local time on the West Coast, and at Therefore, if the UTC day were defined as precisely 86,400 SI seconds, the UTC time-of-day would 14:00 local time in Hawaii. -
UA509: DCF77 Radio Clock DCF77 Radio Clock UA509 with 2 Serial Interfaces, Pulses Per Minute and Per Second, and a 2.5Mm LED Display
Meinberg Radio Clocks Auf der Landwehr 22 31812 Bad Pyrmont, Germany Phone: +49 (5281) 9309-0 Fax: +49 (5281) 9309-30 http://www.meinberg.de [email protected] UA509: DCF77 Radio Clock DCF77 Radio Clock UA509 with 2 serial interfaces, pulses per minute and per second, and a 2.5mm LED Display. Key Features - Direct conversion Quadrature Receiver - Pulses per second and per minute - 20mA input/output circuits - 2,5mm LED-display - 2 RS232 interfaces - Receiver status LEDs - Buffered hardware clock - Flash-EPROM with bootstrap loader rev 2006.0615.1425 Page 1/3 ua509 Description The hardware of UA509 is a 100mm x 160mm microprocessor board. The 20mm wide front panel contains an 8-digit LED display (2.5mm), three LED indicators and a time/date switch. The receiver is connected to the external ferrite antenna AI01 that is included in the sope of supply by the 5 meter 50 ohm coaxial cable (other lengths available). The radio controlled clock UA509 has been designed for applications where two independent serial interfaces are needed. The UA509 contains a flash EPROM with bootstrap loader that allows to upload a new firmware via the serial interface without removal of the clock. Characteristics Type of receiver Narrowband DCF77 quadrature receiver with automatic gain control, bandwidth: approx. 20Hz Display 8 digit 7-segment LED display (2.5mm) for time or date (switch-selectable) optional: 20HP (100mm) wide front panel with 10mm height 7-segment LED display Status info Modulation and field strength visualized by LEDs Free running state visualized by LED after switching to free running quartz clock mode Synchronization time 2-3 minutes after correct DCF77 signal reception Accuracy free run Accuracy of the quartz base after min. -
COORDINATE TIME in the VICINITY of the EARTH D. W. Allan' and N
COORDINATE TIME IN THE VICINITY OF THE EARTH D. W. Allan’ and N. Ashby’ 1. Time and Frequency Division, National Bureau of Standards Boulder, Colorado 80303 2. Department of Physics, Campus Box 390 University of Colorado, Boulder, Colorado 80309 ABSTRACT. Atomic clock accuracies continue to improve rapidly, requir- ing the inclusion of general relativity for unambiguous time and fre- quency clock comparisons. Atomic clocks are now placed on space vehi- cles and there are many new applications of time and frequency metrology. This paper addresses theoretical and practical limitations in the accuracy of atomic clock comparisons arising from relativity, and demonstrates that accuracies of time and frequency comparison can approach a few picoseconds and a few parts in respectively. 1. INTRODUCTION Recent experience has shown that the accuracy of atomic clocks has improved by about an order of magnitude every seven years. It has therefore been necessary to include relativistic effects in the reali- zation of state-of-the-art time and frequency comparisons for at least the last decade. There is a growing need for agreement about proce- dures for incorporating relativistic effects in all disciplines which use modern time and frequency metrology techniques. The areas of need include sophisticated communication and navigation systems and funda- mental areas of research such as geodesy and radio astrometry. Significant progress has recently been made in arriving at defini- tions €or coordinate time that are practical, and in experimental veri- fication of the self-consistency of these procedures. International Atomic Time (TAI) and Universal Coordinated Time (UTC) have been defin- ed as coordinate time scales to assist in the unambiguous comparison of time and frequency in the vicinity of the Earth.