Me and My Shadow - Making the Sun-Earth Connection
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Qncq More.Y T/Eers
NORTH CASCADES CONSERVATION COUNCIL Volume V June lgbl' Number b Trl8 secure the support of the people and the government in the protection and preservation of scenic, scientific, wildlife, wilderness, and outdoor recreational resources values in the North Cascades. ..." QnCQ MoRe.y DQBR T/eeRs/ How many millions of Americans read, and saw, the case for wilderness presented recently in Life? We don't know. But we do know this unprecedentedly wide distri bution of "our side" is one more reason for saying the time for action is now. CONRAD WLRTH, Director of the National Park Service: "... people are aaking up to the problem . and are beginning to take the initiative. ..." "STEWART UDALL, Secretary of the Interior: "... never before has a President of the United States given such a broad and comprehensive mandate to conservation. ..." DR. IRA N. GABRIELSON, President of the Wildlife Management Institute: "The Wilderness Bill, before Congress each of the past five years has the President's support. It has the people's support. it merits immediate approval by Congress." CDJLPFORD V. HEIMBUCHER, President of Trustees for Conservation: "The Wilder ness Bill. has in the 87th Congress the best chance for enactment it has ever had." SENATOR CLINTON ANDERSON, Chairman of the Senate Interior and Insular Affairs Committee: ". I believe the sfth Congress will send a Wilderness Act to the Presi dent and he will sign it into law." HENRY V: "Once more unto the breach, dear friends, once more. In peace there's nothing so becomes a man As modest stillness and humanity; But when the blast of war blows in our ears, Then imitate the action of the tiger. -
The Origin and Evolution of Calipers
History of Precision Measuring Instruments The Origin and Evolution of Calipers MAP1481_E12029_2_MeasuringHistory_Calipers.indd 1 18/5/21 1:34 PM Contents 1. About the Nogisu ...............................................................................................................................1 2. About the Caliper ...............................................................................................................................2 3. Origin of the Name Nogisu and Vernier Graduations ..........................................................................4 4. Oldest Sliding Caliper: Nogisu .............................................................................................................8 5. Scabbard Type Sliding Caliper till the Middle of 19th Century .............................................................9 6. World's Oldest Vernier Caliper (Nogisu) in Existence .........................................................................11 7. Theory That the Vernier Caliper (Nogisu) Was Born in the U.S. ..........................................................12 8. Calipers before Around 1945 (the End of WWII) in the West ...........................................................13 8. 1. Slide-Catching Scale without Vernier Graduations: Simplified Calipers ......................................14 8. 2. Sliding Calipers with Diagonal Scale ..........................................................................................18 8. 3. Sliding Caliper with a Vernier Scale: Vernier Caliper ..................................................................19 -
AIM: Latitude and Longitude
AIM: Latitude and Longitude Latitude lines run east/west but they measure north or south of the equator (0°) splitting the earth into the Northern Hemisphere and Southern Hemisphere. Latitude North Pole 90 80 Lines of 70 60 latitude are 50 numbered 40 30 from 0° at 20 Lines of [ 10 the equator latitude are 10 to 90° N.L. 20 numbered 30 at the North from 0° at 40 Pole. 50 the equator ] 60 to 90° S.L. 70 80 at the 90 South Pole. South Pole Latitude The North Pole is at 90° N 40° N is the 40° The equator is at 0° line of latitude north of the latitude. It is neither equator. north nor south. It is at the center 40° S is the 40° between line of latitude north and The South Pole is at 90° S south of the south. equator. Longitude Lines of longitude begin at the Prime Meridian. 60° W is the 60° E is the 60° line of 60° line of longitude west longitude of the Prime east of the W E Prime Meridian. Meridian. The Prime Meridian is located at 0°. It is neither east or west 180° N Longitude West Longitude West East Longitude North Pole W E PRIME MERIDIAN S Lines of longitude are numbered east from the Prime Meridian to the 180° line and west from the Prime Meridian to the 180° line. Prime Meridian The Prime Meridian (0°) and the 180° line split the earth into the Western Hemisphere and Eastern Hemisphere. Prime Meridian Western Eastern Hemisphere Hemisphere Places located east of the Prime Meridian have an east longitude (E) address. -
Date Day Peculiarity Position of the Sun Northern Hemisphere Southern
Date Day Peculiarity Position of the Northern Southern sun hemisphere hemisphere March 21 Equinox Length of day Above the From March and night will Equator 21 to be equal ( 0° ) June 21 Spring Autumn June 21 Summer Northern Above the From June 21 Solstice Hemisphere Tropic of to September experiences its Cancer 23 longest day (231⁄2°N) and shortest night Summer Winter September 23 Equinox Length of day Above the From and night will Equator September 23 be equal ( 0° ) to December 22 Autumn Spring December 22 Winter Solstice Northern Above Tropic From Hemisphere of Capricorn December 22 experiences (231⁄2°S) to March 21 its shortest day and longest night. Winter Summer Utharayanam Dakshinayanam The Sun sets its northward apparent The Sun sets its movement southward apparent movement from Tropic of Capricorn (231⁄2°S) and from Tropic of Cancer (231⁄2°N) and it it culminates on Tropic of Cancer (231⁄2°N) culminates on Tropic of Capricorn (231⁄2°S) Following the winter solstice to June 21. Following the summer solstice to December 22 Causes Earth's revolution It is in an elliptical orbit that the Earth revolves around the Sun Tilt of the axis The axis of the Earth is tilted at an angle of ( the inclination of axis ) 661⁄2° from the orbital plane. If measured from the vertical plane this would be 231⁄2° Parallelism of the Earth's axis. The Earth maintains this tilt throughout its revolution. The apparent movement of the Sun. Since the parallelism is maintained same throughout the revolution, the position of the Sun in relation to the Earth varies apparently between Tropic of Cancer (231⁄2° North) and Tropic of Capricorn (231⁄2° South). -
The International Date Line!
The International Date Line! The International Date Line (IDL) is a generally north-south imaginary line on the surface of the Earth, passing through the middle of the Pacific Ocean, that designates the place where each calendar day begins. It is roughly along 180° longitude, opposite the Prime Meridian, but it is drawn with diversions to pass around some territories and island groups. Crossing the IDL travelling east results in a day or 24 hours being subtracted, so that the traveller repeats the date to the west of the line. Crossing west results in a day being added, that is, the date is the eastern side date plus one calendar day. The line is necessary in order to have a fixed, albeit arbitrary, boundary on the globe where the calendar date advances. Geography For part of its length, the International Date Line follows the meridian of 180° longitude, roughly down the middle of the Pacific Ocean. To avoid crossing nations internally, however, the line deviates to pass around the far east of Russia and various island groups in the Pacific. In the north, the date line swings to the east of Wrangel island and the Chukchi Peninsula and through the Bering Strait passing between the Diomede Islands at a distance of 1.5 km (1 mi) from each island. It then goes southwest, passing west of St. Lawrence Island and St. Matthew Island, until it passes midway between the United States' Aleutian Islands and Russia's Commander Islands before returning southeast to 180°. This keeps Russia which is north and west of the Bering Sea and the United States' Alaska which is east and south of the Bering Sea, on opposite sides of the line in agreement with the date in the rest of those countries. -
Lithium Abundance and Rotation of Seismic Solar Analogues P
Lithium abundance and rotation of seismic solar analogues P. G. Beck, J.-D. Do Nascimento, T. Duarte, D. Salabert, A. Tkachenko, S. Mathis, S. Mathur, R. A. García, M. Castro, P. L. Pallé, et al. To cite this version: P. G. Beck, J.-D. Do Nascimento, T. Duarte, D. Salabert, A. Tkachenko, et al.. Lithium abun- dance and rotation of seismic solar analogues: Solar and stellar connection from Kepler and Hermes observations. Astronomy and Astrophysics - A&A, EDP Sciences, 2017, 602, pp.A63. 10.1051/0004- 6361/201629820. cea-02988985 HAL Id: cea-02988985 https://hal-cea.archives-ouvertes.fr/cea-02988985 Submitted on 5 Nov 2020 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. A&A 602, A63 (2017) Astronomy DOI: 10.1051/0004-6361/201629820 & c ESO 2017 Astrophysics Lithium abundance and rotation of seismic solar analogues Solar and stellar connection from Kepler and Hermes observations? P.G. Beck1, J.-D. do Nascimento Jr.2; 3, T. Duarte2, D. Salabert1, A. Tkachenko4, S. Mathis1, S. Mathur5, R. A. García1, M. Castro2, P.L. Pallé6; 7, R. Egeland8; 9, D. Montes10, O. Creevey11, M. -
Surveying and Drawing Instruments
SURVEYING AND DRAWING INSTRUMENTS MAY \?\ 10 1917 , -;>. 1, :rks, \ C. F. CASELLA & Co., Ltd II to 15, Rochester Row, London, S.W. Telegrams: "ESCUTCHEON. LONDON." Telephone : Westminster 5599. 1911. List No. 330. RECENT AWARDS Franco-British Exhibition, London, 1908 GRAND PRIZE AND DIPLOMA OF HONOUR. Japan-British Exhibition, London, 1910 DIPLOMA. Engineering Exhibition, Allahabad, 1910 GOLD MEDAL. SURVEYING AND DRAWING INSTRUMENTS - . V &*>%$> ^ .f C. F. CASELLA & Co., Ltd MAKERS OF SURVEYING, METEOROLOGICAL & OTHER SCIENTIFIC INSTRUMENTS TO The Admiralty, Ordnance, Office of Works and other Home Departments, and to the Indian, Canadian and all Foreign Governments. II to 15, Rochester Row, Victoria Street, London, S.W. 1911 Established 1810. LIST No. 330. This List cancels previous issues and is subject to alteration with out notice. The prices are for delivery in London, packing extra. New customers are requested to send remittance with order or to furnish the usual references. C. F. CAS ELL A & CO., LTD. Y-THEODOLITES (1) 3-inch Y-Theodolite, divided on silver, with verniers to i minute with rack achromatic reading ; adjustment, telescope, erect and inverting eye-pieces, tangent screw and clamp adjustments, compass, cross levels, three screws and locking plate or parallel plates, etc., etc., in mahogany case, with tripod stand, complete 19 10 Weight of instrument, case and stand, about 14 Ibs. (6-4 kilos). (2) 4-inch Do., with all improvements, as above, to i minute... 22 (3) 5-inch Do., ... 24 (4) 6-inch Do., 20 seconds 27 (6 inch, to 10 seconds, 403. extra.) Larger sizes and special patterns made to order. -
Toand Television Irrom June 25
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Maps and Diagrams. Their Compilation and Construction
~r HJ.Mo Mouse andHR Wilkinson MAPS AND DIAGRAMS 8 his third edition does not form a ramatic departure from the treatment of artographic methods which has made it a standard text for 1 years, but it has developed those aspects of the subject (computer-graphics, quantification gen- erally) which are likely to progress in the uture. While earlier editions were primarily concerned with university cartography ‘ourses and with the production of the- matic maps to illustrate theses, articles and books, this new edition takes into account the increasing number of professional cartographer-geographers employed in Government departments, planning de- partments and in the offices of architects pnd civil engineers. The authors seek to ive students some idea of the novel and xciting developments in tools, materials, echniques and methods. The growth, mounting to an explosion, in data of all inds emphasises the increasing need for discerning use of statistical techniques, nevitably, the dependence on the com- uter for ordering and sifting data must row, as must the degree of sophistication n the techniques employed. New maps nd diagrams have been supplied where ecessary. HIRD EDITION PRICE NET £3-50 :70s IN U K 0 N LY MAPS AND DIAGRAMS THEIR COMPILATION AND CONSTRUCTION MAPS AND DIAGRAMS THEIR COMPILATION AND CONSTRUCTION F. J. MONKHOUSE Formerly Professor of Geography in the University of Southampton and H. R. WILKINSON Professor of Geography in the University of Hull METHUEN & CO LTD II NEW FETTER LANE LONDON EC4 ; © ig6g and igyi F.J. Monkhouse and H. R. Wilkinson First published goth October igj2 Reprinted 4 times Second edition, revised and enlarged, ig6g Reprinted 3 times Third edition, revised and enlarged, igyi SBN 416 07440 5 Second edition first published as a University Paperback, ig6g Reprinted 5 times Third edition, igyi SBN 416 07450 2 Printed in Great Britain by Richard Clay ( The Chaucer Press), Ltd Bungay, Suffolk This title is available in both hard and paperback editions. -
Download This Article in PDF Format
A&A 602, A63 (2017) Astronomy DOI: 10.1051/0004-6361/201629820 & c ESO 2017 Astrophysics Lithium abundance and rotation of seismic solar analogues Solar and stellar connection from Kepler and Hermes observations? P.G. Beck1, J.-D. do Nascimento Jr.2; 3, T. Duarte2, D. Salabert1, A. Tkachenko4, S. Mathis1, S. Mathur5, R. A. García1, M. Castro2, P.L. Pallé6; 7, R. Egeland8; 9, D. Montes10, O. Creevey11, M. F. Andersen12, D. Kamath4, and H. van Winckel4 1 Laboratoire AIM, CEA/DRF – CNRS – Univ. Paris Diderot – IRFU/SAp, Centre de Saclay, 91191 Gif-sur-Yvette Cedex, France e-mail: [email protected] 2 Departamento de Física, Universidade Federal do Rio Grande do Norte, 59072-970 Natal, RN, Brazil 3 Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA 4 Instituut voor Sterrenkunde, KU Leuven, 3001 Leuven, Belgium 5 Space Science Institute, 4750 Walnut street Suite 205, Boulder, CO 80301, USA 6 Instituto de Astrofísica de Canarias, 38200 La Laguna, Tenerife, Spain 7 Departamento de Astrofísica, Universidad de La Laguna, 38206 La Laguna, Tenerife, Spain 8 High Altitude Observatory, National Center for Atmospheric Research, PO Box 3000, Boulder, CO 80307-3000, USA 9 Department of Physics, Montana State University, Bozeman, MT 59717-3840, USA 10 Dpto. Astrofísica, Facultad de CC. Físicas, Universidad Complutense de Madrid, 28040 Madrid, Spain 11 Laboratoire Lagrange, Université de Nice Sophia-Antipolis, UMR 7293, CNRS, Observatoire de la Côte d’Azur, Nice, France 12 Stellar Astrophysics Centre, Aarhus University, Ny Munkegade 120, 8000 Aarhus C, Denmark Received 30 September 2016 / Accepted 2 February 2017 ABSTRACT Context. -
Equation of Time — Problem in Astronomy M
This paper was awarded in the II International Competition (1993/94) "First Step to Nobel Prize in Physics" and published in the competition proceedings (Acta Phys. Pol. A 88 Supplement, S-49 (1995)). The paper is reproduced here due to kind agreement of the Editorial Board of "Acta Physica Polonica A". EQUATION OF TIME | PROBLEM IN ASTRONOMY M. Muller¨ Gymnasium M¨unchenstein, Grellingerstrasse 5, 4142 M¨unchenstein, Switzerland Abstract The apparent solar motion is not uniform and the length of a solar day is not constant throughout a year. The difference between apparent solar time and mean (regular) solar time is called the equation of time. Two well-known features of our solar system lie at the basis of the periodic irregularities in the solar motion. The angular velocity of the earth relative to the sun varies periodically in the course of a year. The plane of the orbit of the earth is inclined with respect to the equatorial plane. Therefore, the angular velocity of the relative motion has to be projected from the ecliptic onto the equatorial plane before incorporating it into the measurement of time. The math- ematical expression of the projection factor for ecliptic angular velocities yields an oscillating function with two periods per year. The difference between the extreme values of the equation of time is about half an hour. The response of the equation of time to a variation of its key parameters is analyzed. In order to visualize factors contributing to the equation of time a model has been constructed which accounts for the elliptical orbit of the earth, the periodically changing angular velocity, and the inclined axis of the earth. -
Moon-Earth-Sun: the Oldest Three-Body Problem
Moon-Earth-Sun: The oldest three-body problem Martin C. Gutzwiller IBM Research Center, Yorktown Heights, New York 10598 The daily motion of the Moon through the sky has many unusual features that a careful observer can discover without the help of instruments. The three different frequencies for the three degrees of freedom have been known very accurately for 3000 years, and the geometric explanation of the Greek astronomers was basically correct. Whereas Kepler’s laws are sufficient for describing the motion of the planets around the Sun, even the most obvious facts about the lunar motion cannot be understood without the gravitational attraction of both the Earth and the Sun. Newton discussed this problem at great length, and with mixed success; it was the only testing ground for his Universal Gravitation. This background for today’s many-body theory is discussed in some detail because all the guiding principles for our understanding can be traced to the earliest developments of astronomy. They are the oldest results of scientific inquiry, and they were the first ones to be confirmed by the great physicist-mathematicians of the 18th century. By a variety of methods, Laplace was able to claim complete agreement of celestial mechanics with the astronomical observations. Lagrange initiated a new trend wherein the mathematical problems of mechanics could all be solved by the same uniform process; canonical transformations eventually won the field. They were used for the first time on a large scale by Delaunay to find the ultimate solution of the lunar problem by perturbing the solution of the two-body Earth-Moon problem.