Library Catalogue 2000, by Author
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Ira Sprague Bowen Papers, 1940-1973
http://oac.cdlib.org/findaid/ark:/13030/tf2p300278 No online items Inventory of the Ira Sprague Bowen Papers, 1940-1973 Processed by Ronald S. Brashear; machine-readable finding aid created by Gabriela A. Montoya Manuscripts Department The Huntington Library 1151 Oxford Road San Marino, California 91108 Phone: (626) 405-2203 Fax: (626) 449-5720 Email: [email protected] URL: http://www.huntington.org/huntingtonlibrary.aspx?id=554 © 1998 The Huntington Library. All rights reserved. Observatories of the Carnegie Institution of Washington Collection Inventory of the Ira Sprague 1 Bowen Papers, 1940-1973 Observatories of the Carnegie Institution of Washington Collection Inventory of the Ira Sprague Bowen Paper, 1940-1973 The Huntington Library San Marino, California Contact Information Manuscripts Department The Huntington Library 1151 Oxford Road San Marino, California 91108 Phone: (626) 405-2203 Fax: (626) 449-5720 Email: [email protected] URL: http://www.huntington.org/huntingtonlibrary.aspx?id=554 Processed by: Ronald S. Brashear Encoded by: Gabriela A. Montoya © 1998 The Huntington Library. All rights reserved. Descriptive Summary Title: Ira Sprague Bowen Papers, Date (inclusive): 1940-1973 Creator: Bowen, Ira Sprague Extent: Approximately 29,000 pieces in 88 boxes Repository: The Huntington Library San Marino, California 91108 Language: English. Provenance Placed on permanent deposit in the Huntington Library by the Observatories of the Carnegie Institution of Washington Collection. This was done in 1989 as part of a letter of agreement (dated November 5, 1987) between the Huntington and the Carnegie Observatories. The papers have yet to be officially accessioned. Cataloging of the papers was completed in 1989 prior to their transfer to the Huntington. -
Basic Principles of Celestial Navigation James A
Basic principles of celestial navigation James A. Van Allena) Department of Physics and Astronomy, The University of Iowa, Iowa City, Iowa 52242 ͑Received 16 January 2004; accepted 10 June 2004͒ Celestial navigation is a technique for determining one’s geographic position by the observation of identified stars, identified planets, the Sun, and the Moon. This subject has a multitude of refinements which, although valuable to a professional navigator, tend to obscure the basic principles. I describe these principles, give an analytical solution of the classical two-star-sight problem without any dependence on prior knowledge of position, and include several examples. Some approximations and simplifications are made in the interest of clarity. © 2004 American Association of Physics Teachers. ͓DOI: 10.1119/1.1778391͔ I. INTRODUCTION longitude ⌳ is between 0° and 360°, although often it is convenient to take the longitude westward of the prime me- Celestial navigation is a technique for determining one’s ridian to be between 0° and Ϫ180°. The longitude of P also geographic position by the observation of identified stars, can be specified by the plane angle in the equatorial plane identified planets, the Sun, and the Moon. Its basic principles whose vertex is at O with one radial line through the point at are a combination of rudimentary astronomical knowledge 1–3 which the meridian through P intersects the equatorial plane and spherical trigonometry. and the other radial line through the point G at which the Anyone who has been on a ship that is remote from any prime meridian intersects the equatorial plane ͑see Fig. -
Autobiography of Sir George Biddell Airy by George Biddell Airy 1
Autobiography of Sir George Biddell Airy by George Biddell Airy 1 CHAPTER I. CHAPTER II. CHAPTER III. CHAPTER IV. CHAPTER V. CHAPTER VI. CHAPTER VII. CHAPTER VIII. CHAPTER IX. CHAPTER X. CHAPTER I. CHAPTER II. CHAPTER III. CHAPTER IV. CHAPTER V. CHAPTER VI. CHAPTER VII. CHAPTER VIII. CHAPTER IX. CHAPTER X. Autobiography of Sir George Biddell Airy by George Biddell Airy The Project Gutenberg EBook of Autobiography of Sir George Biddell Airy by George Biddell Airy This eBook is for the use of anyone anywhere at no cost and with almost no restrictions whatsoever. You may copy it, give it away or re-use it under the terms of the Project Gutenberg Autobiography of Sir George Biddell Airy by George Biddell Airy 2 License included with this eBook or online at www.gutenberg.net Title: Autobiography of Sir George Biddell Airy Author: George Biddell Airy Release Date: January 9, 2004 [EBook #10655] Language: English Character set encoding: ISO-8859-1 *** START OF THIS PROJECT GUTENBERG EBOOK SIR GEORGE AIRY *** Produced by Joseph Myers and PG Distributed Proofreaders AUTOBIOGRAPHY OF SIR GEORGE BIDDELL AIRY, K.C.B., M.A., LL.D., D.C.L., F.R.S., F.R.A.S., HONORARY FELLOW OF TRINITY COLLEGE, CAMBRIDGE, ASTRONOMER ROYAL FROM 1836 TO 1881. EDITED BY WILFRID AIRY, B.A., M.Inst.C.E. 1896 PREFACE. The life of Airy was essentially that of a hard-working, business man, and differed from that of other hard-working people only in the quality and variety of his work. It was not an exciting life, but it was full of interest, and his work brought him into close relations with many scientific men, and with many men high in the State. -
New Force at Large Distances
New force at large distances Daniel Grumiller Institute for Theoretical Physics Vienna University of Technology TEDx Vienna, November 2010 I What are the fundamental forces in Nature? I What is the nature of space, time and matter? Some questions physics cannot address: We live in the golden age of fundamental physics Goal: want to understand how the Universe works Some questions physics can address: I What is the Universe made of? (picture by NASA) D. Grumiller | New force 2/11 I What is the nature of space, time and matter? Some questions physics cannot address: We live in the golden age of fundamental physics Goal: want to understand how the Universe works Some questions physics can address: I What is the Universe made of? I What are the fundamental forces in Nature? (picture by lifesbalancebeam) D. Grumiller | New force 2/11 Some questions physics cannot address: We live in the golden age of fundamental physics Goal: want to understand how the Universe works Some questions physics can address: I What is the Universe made of? I What are the fundamental forces in Nature? I What is the nature of space, time and matter? (picture by spacescan.org) D. Grumiller | New force 2/11 We live in the golden age of fundamental physics Goal: want to understand how the Universe works Some questions physics can address: I What is the Universe made of? I What are the fundamental forces in Nature? I What is the nature of space, time and matter? Some questions physics cannot address: D. Grumiller | New force 2/11 What is the Universe made of? D. -
List of Honorary Fellows
LIST OF HONORARY FELLOWS. 847 LIST OF HONORARY FELLOWS .110 AT MARCH 1897. His Royal Highness The PRINCE OF WALES. FOREIGNERS (LIMITED TO THIRTY-SIX BY LAW X.). Elected. 495 1897 Alexander Agassiz, Cambridge (Mass.). 1897 E.-H. Amagat, Paris. 1889 Marcellin Pierre Eugene Berthelot, Paris. 1895 Ludwig Boltzmann, Vienna. 1864 Rohert Wilhelm Bunsen, Heidelberg. 1897 Stanislao Cannizzaro, Rome, 1883 Luigi Cremona, Rome. 1877 Carl Gegenbaur, Heidelberg, 1888 Ernst Haeckel, Jena. 1883 Julius Hann, Vienna. 1884 Charles Hermite, Paris. 1879 Jules Janssen, Paris, 1864 Alhert von Kblliker, Wilrzhurg. 1864 Rudolph Leuckart, Leipzig, 1897 Gabriel Lippmann, Paris. 1895 fileuthere-6lie-Nicolas Mascart, Paris. 1888 Demetrius Ivanovich Mendel6ef, St Petersburg. 1895 Carl Menger, Vienna. 1886 Alphonse Milne-Edwards Paris. 1864 Theodore Mommsen, Berlin. 1897 Fridtjof Nansen, Christiania. 1881 Simon Newcomb, Washington. 1895 Max von Pettenkofer, Munich. 1895 Jules Henri Poincare, Paris. 1889 Georg Hermann Quincke, Heidelberg. 1886 Alphonse Renard, Ghent. 1897 Ferdinand von Ricbthofen, Berlin. 1897 Henry A. Rowland, Baltimore. 1897 Giovanni V. Schiaparelli, Milan, 1881 Johannes Iapetus Smith Steenstrup, Copenhagen. 1878 Otto Wilhelm Strove, St Petersburg. 1886 Tobias Robert Thaten, Upsala. 1874 Otto Torell, Lund. 1868 Rudolph Yirchow, Berlin. 1892 Gustav Wiedemann, Leipzig. 1897 Ferdinand Zirkel, Leipzig. Total, 36. 848 LIST OF HONORARY FELLOWS. BRITISH SUBJECTS (LIMITED TO TWENTY BY LAW x.). Elected. 1889 Sir Robert Stawell Ball, Kt., LL.D., F.R.S., M.R.I. A., Lowndean, Professor of Astronomy in the University of Cambridge, Cambridge 1897 The Very Rev. John Caird, D.D., LL.D., Principal of the Uni- versity of Glasgow, Glasgow. 1892 Colonel Alexander Ross Clarke, C.B., R.E., F.R.S., Redhill, Surrey 1897 George Howard Darwin, M.A., LL.D., F.R.S., Plumian Professor of Astronomy in the University of Cambridge, Cambridge. -
Kew Observatory and the Evolution of Victorian Science, 1840–1910
introduction Kew Observatory, Victorian Science, and the “Observatory Sciences” One more recent instance of the operations of this Society in this respect I may mention, in addition to those I have slightly enumerated. I mean the important accession to the means of this Society of a fixed position, a place for deposit, regula- tion, and comparison of instruments, and for many more purposes than I could name, perhaps even more than are yet contemplated, in the Observatory at Kew. Address by Lord Francis Egerton to British Association for the Advancement of Science, June 1842 When in 1842 Lord Egerton, president of the British Association for the Advancement of Science (BAAS), announced the association’s acquisition of Kew Observatory (figure I.1), he heralded the inaugura- tion of what would become one of the major institutions of nineteenth- century British—indeed international—science. Originally built as a pri- vate observatory for King George III and long in a moribund state, after 1842 the Kew building would, as Egerton predicted, become a multi- functional observatory, put to more purposes than were even imagined in 1842. It became distinguished in several sciences: geomagnetism, me- teorology, solar astronomy, and standardization—the latter term being used in this book to refer to testing scientific instruments and develop- ing prototypes of instruments to be used elsewhere, as well as establish- ing and refining constants and standards of measurement. Many of the major figures in the physical sciences of the nineteenth century were in some way involved with Kew Observatory. For the first twenty months of the twentieth century, Kew was the site of the National Physical Labora- 3 © 2018 University of Pittsburgh Press. -
3-16 Events in Europe and the Rest of the World in the 1860S
3-16 Rest of the World in the 1860s 1 of 3 A Living Resource Guide to Lincoln's Life and Legacy Events in Europe and the Rest of the World in the 1860s In the United States In Europe and the Rest of the World . Lincoln is elected President 1860 . Garibaldi conquers Sicily and Naples . South Carolina secedes from the Union . George Eliot (Mary Ann Evans) . The US Secret Service is created publishes A Mill on the Floss . The Pony Express begins its overland . Frenchman Jean J. Lenoir builds the message delivery service first gas-burning engine . Olympia Brown becomes the first . Florence Nightingale founds the female theology student in the US world’s first nursing school . In Boston Elizabeth Peabody . The first British Open Golf establishes the first English-language Championship is held kindergarten . Louis Agassiz rejects Darwin’s theory of evolution, citing missing links . Alvan Clarks discovers that Sirius is a double star . Croquet becomes a popular pastime . Abraham Lincoln is inaugurated 1861 . Unification of Italy President . Czar Alexander II abolishes serfdom . The Confederate States of America is in Russia created . Prince Albert, consort of Queen . Fort Sumter is fired on, beginning the Victoria, dies – leading the queen into Civil War 3 years of mourning . Lincoln orders a blockade of Southern . The principalities of Moldavia and ports Wallachia unite to form Romania . The South defeats the North in the . According to some, Edouard Manet’s First Battle of Bull Run Spanish Singer marks the beginning . Kansas is admitted to the Union of Impressionism . Matthew Brady begins his . -
Recent News 28,270 MILES - WAY to GO!
Number 62 Spring 2017 TREASURE HUNT – 16 Where is this bridge (hint: it is not in the UK) and who designed it? Can you see the parabola and its tangent? Recent News 28,270 MILES - WAY TO GO! In October last year a record was set for the longest single road route ever worked out. The Travelling Salesperson Problem (TSP) was first posed in the 1930’s by Merrill Flood who was looking to solve a school bus routing problem in the US and it asks the following question: "Given a list of cities and the distances between each pair of cities, what is the shortest possible route that visits each city exactly once and returns to the origin city?" This is an example of an optimisation problem and is of immense importance to businesses who need to make deliveries to many places as the shortest route between the warehouse and drop off points generally means considerable saving in time and money. The TSP also has applications in computing DNA sequences, aiming telescopes and designing computer chip circuits. William Cook and a team of researchers at the University of Waterloo in Ontario, Canada calculated a round route that starts in Portland, Dorset and finishes in Weymouth, four miles away has at least 100 times more stops than the previous longest TSP. It links 24,727 hostelries in the UK. EDITORIAL SQUARE NUMBERS Welcome back to a new term and a new year! We In SYMmetryplus 61, Autumn 2016, modular arithmetic congratulate Mathematical Pie for their 200th edition was used to find a prime factor of 283 1. -
The Mystery and Majesty
The mystery and majesty Nearly 40 years after THE SPACE AGE BLASTED off when the Soviet Union launched the Voyager 2 visited Uranus world’s first artificial satellite in 1957. Since then, humanity has explored our cosmic and Neptune, scientists are backyard with vigor — and yet two planets have fallen to the planetary probe wayside. eager for new expeditions. In the 63 years since Sputnik, humanity has only visited Neptune and Uranus once BY JOEL DAVIS — when Voyager 2 flew past Uranus in January 1986 and Neptune in August 1989 40 ASTRONOMY • DECEMBER 2020 of the ICE GIANTS — and even that wasn’t entirely pre- interstellar mission, more than a dozen pro- In 1781, Uranus became the first planet planned. The unmitigated success of posals have been offered for return missions ever discovered using a telescope. Nearly 200 years later, Voyager 2 Voyager 1 and 2 on their original mission to one or both ice giants. So far, none have became the first spacecraft to visit to explore Jupiter and Saturn earned the made it past the proposal stage due to lack Uranus and Neptune, in 1986 and 1989 respectively. NASA/JPL twin spacecrafts further missions in our of substantial scientific interest. Effectively, solar system and beyond, with Neptune and the planetary research community has been Uranus acting as the last stops on a Grand giving the ice giants the cold shoulder. Tour of the outer solar system. But recently, exoplanet data began In the 31 years since Voyager 2 left the revealing the abundance of icy exoplanets Neptune system in 1989 and began its in our galaxy “and new questions about WWW.ASTRONOMY.COM 41 With a rotation axis tilted more than 90 degrees compared to its orbital plane, Neptune likewise has a highly tilted rotation axis and tilted magnetic axis. -
Einstein, History, and Other Passions : the Rebellion Against Science at the End of the Twentieth Century
Einstein, history, and other passions : the rebellion against science at the end of the twentieth century The Harvard community has made this article openly available. Please share how this access benefits you. Your story matters Citation Holton, Gerald James. 2000. Einstein, history, and other passions : the rebellion against science at the end of the twentieth century. Cambridge, MA: Harvard University Press. Published Version http://www.hup.harvard.edu/catalog.php?isbn=9780674004337 Citable link http://nrs.harvard.edu/urn-3:HUL.InstRepos:23975375 Terms of Use This article was downloaded from Harvard University’s DASH repository, and is made available under the terms and conditions applicable to Other Posted Material, as set forth at http:// nrs.harvard.edu/urn-3:HUL.InstRepos:dash.current.terms-of- use#LAA EINSTEIN, HISTORY, ANDOTHER PASSIONS ;/S*6 ? ? / ? L EINSTEIN, HISTORY, ANDOTHER PASSIONS E?3^ 0/" Cf72fM?y GERALD HOLTON A HARVARD UNIVERSITY PRESS C%772^r?<%gf, AizziMc^zzyeZZy LozzJozz, E?zg/%??J Q AOOO Many of the designations used by manufacturers and sellers to distinguish their products are claimed as trademarks. Where those designations appear in this book and Addison-Wesley was aware of a trademark claim, the designations have been printed in capital letters. PHYSICS RESEARCH LIBRARY NOV 0 4 1008 Copyright @ 1996 by Gerald Holton All rights reserved HARVARD UNIVERSITY Printed in the United States of America An earlier version of this book was published by the American Institute of Physics Press in 1995. First Harvard University Press paperback edition, 2000 o/ CoMgre.w C%t%/og;Hg-zM-PMMt'%tz'c7t Dzztzz Holton, Gerald James. -
The Charles Knight-Joseph Hooker Correspondence
A man tenax propositi: transcriptions of letters from Charles Knight to William Jackson Hooker and Joseph Dalton Hooker between 1852 and 1883 David J. Galloway Hon. Research Associate Landcare Research, and Te Papa Tongarewa [email protected] Geoscience Society of New Zealand miscellaneous publication 133J December 2013 Published by the Geoscience Society of New Zealand Inc, 2013 Information on the Society and its publications is given at www.gsnz.org.nz © Copyright David J. Galloway, 2013 Geoscience Society of New Zealand miscellaneous publication 133J ISBN 978-1-877480-36-2 ISSN 2230-4495 (Online) ISSN 2230-4487 (Print) This document is available as a PDF file that can be downloaded from the Geoscience Society website at: http://www.gsnz.org.nz/information/misc-series-i-49.html Bibliographic Reference Galloway D.J. 2013: A man tenax propositi: transcriptions of letters from Charles Knight to William Jackson Hooker and Joseph Dalton Hooker between 1852 and 1883 Geoscience Society of New Zealand miscellaneous publication 133J. 88 pages. A man tenax propositi: transcriptions of letters from Charles Knight to William Jackson Hooker and Joseph Dalton Hooker between 1852 and 1883 Contents Introduction 3 Charles Knight correspondence at Kew 5 Acknowledgements 6 Summaries of the letters 7 Transcriptions of the letters from Charles Knight 15 Footnotes 70 References 77 Figure 1: Dr Charles Knight FLS, FRCS 2 Figure 2: Group photograph including Charles Knight 2 Figure 3: Page of letter from Knight to Hooker 14 Table 1: Comparative chronology of Charles Knight, W.J. Hooker and J.D. Hooker 86 1 Figure 1: Dr Charles Knight FLS, FRCS Alexander Turnbull Library,Wellington, New Zealand ¼-015414 Figure 2: Group taken in Walter Mantell‟s garden about 1865 showing Charles Knight (left), John Buchanan and James Hector (right) and Walter Mantell and his young son, Walter Godfrey Mantell (seated on grass). -
The Celestial Sphere
The Celestial Sphere Useful References: • Smart, “Text-Book on Spherical Astronomy” (or similar) • “Astronomical Almanac” and “Astronomical Almanac’s Explanatory Supplement” (always definitive) • Lang, “Astrophysical Formulae” (for quick reference) • Allen “Astrophysical Quantities” (for quick reference) • Karttunen, “Fundamental Astronomy” (e-book version accessible from Penn State at http://www.springerlink.com/content/j5658r/ Numbers to Keep in Mind • 4 π (180 / π)2 = 41,253 deg2 on the sky • ~ 23.5° = obliquity of the ecliptic • 17h 45m, -29° = coordinates of Galactic Center • 12h 51m, +27° = coordinates of North Galactic Pole • 18h, +66°33’ = coordinates of North Ecliptic Pole Spherical Astronomy Geocentrically speaking, the Earth sits inside a celestial sphere containing fixed stars. We are therefore driven towards equations based on spherical coordinates. Rules for Spherical Astronomy • The shortest distance between two points on a sphere is a great circle. • The length of a (great circle) arc is proportional to the angle created by the two radial vectors defining the points. • The great-circle arc length between two points on a sphere is given by cos a = (cos b cos c) + (sin b sin c cos A) where the small letters are angles, and the capital letters are the arcs. (This is the fundamental equation of spherical trigonometry.) • Two other spherical triangle relations which can be derived from the fundamental equation are sin A sinB = and sin a cos B = cos b sin c – sin b cos c cos A sina sinb € Proof of Fundamental Equation • O is