Astrometry 1960-80: from Hamburg to Hipparcos by Erik Høg, 2014.08.06 Niels Bohr Institute, Copenhagen University
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A Multislit Photoelectric Star Micrometer for the Meridian Circle of the Nikolayev Astronomical Observatory
A Multislit Photoelectric Star Micrometer for the Meridian Circle of the Nikolayev Astronomical Observatory. V. V. Konin and A. D. Pogonij Nikolaev Astronomical Observatory, Nikolaev, USSR In the course of the cooperation between the Nikolaev and the Pulkovo Observatories, a photoelectric micrometer, similar to that proposed by E. Htfg, was designed and installed on the Repsold meridian circle. The optics of the finder includes an achromatic wedge for the deflection of light from the objective to the finderTs eyepiece. The grating is composed only of a system of inclined slits (Hrfg 1970, p. 92, No. 2). The slits are 5V3 wide and spaced at 38V3. One can use from 7 to 14 slit pairs in the micrometer for observations. A rectangular diaphragm isolates an element of 19" x 27" from the working grating. This has 4 initial positions. The required initial position depends on the instrument's position, the type of culmination and the observing interval (30s or 60s for an equatorial star). The diaphragm is moved by a stepping motor, whose speed of rotation is controlled by the observer and depends on declination. The motor can be switched on either by hand or automatically after the star appears in the field defined by the diaphragm. During transit, the clock readings of the start and the end of the observation are recorded with a precision of 0? 001. Photon counts are taken for every 0S1 time interval. There is a block for recording contact signals from a moving mark in the control unit (Konin et al., 1982). Karyakina et al. -
A Politico-Social History of Algolt (With a Chronology in the Form of a Log Book)
A Politico-Social History of Algolt (With a Chronology in the Form of a Log Book) R. w. BEMER Introduction This is an admittedly fragmentary chronicle of events in the develop ment of the algorithmic language ALGOL. Nevertheless, it seems perti nent, while we await the advent of a technical and conceptual history, to outline the matrix of forces which shaped that history in a political and social sense. Perhaps the author's role is only that of recorder of visible events, rather than the complex interplay of ideas which have made ALGOL the force it is in the computational world. It is true, as Professor Ershov stated in his review of a draft of the present work, that "the reading of this history, rich in curious details, nevertheless does not enable the beginner to understand why ALGOL, with a history that would seem more disappointing than triumphant, changed the face of current programming". I can only state that the time scale and my own lesser competence do not allow the tracing of conceptual development in requisite detail. Books are sure to follow in this area, particularly one by Knuth. A further defect in the present work is the relatively lesser availability of European input to the log, although I could claim better access than many in the U.S.A. This is regrettable in view of the relatively stronger support given to ALGOL in Europe. Perhaps this calmer acceptance had the effect of reducing the number of significant entries for a log such as this. Following a brief view of the pattern of events come the entries of the chronology, or log, numbered for reference in the text. -
A Propensity for Genius: That Something Special About Fritz Zwicky (1898 - 1974)
Swiss American Historical Society Review Volume 42 Number 1 Article 2 2-2006 A Propensity for Genius: That Something Special About Fritz Zwicky (1898 - 1974) John Charles Mannone Follow this and additional works at: https://scholarsarchive.byu.edu/sahs_review Part of the European History Commons, and the European Languages and Societies Commons Recommended Citation Mannone, John Charles (2006) "A Propensity for Genius: That Something Special About Fritz Zwicky (1898 - 1974)," Swiss American Historical Society Review: Vol. 42 : No. 1 , Article 2. Available at: https://scholarsarchive.byu.edu/sahs_review/vol42/iss1/2 This Article is brought to you for free and open access by BYU ScholarsArchive. It has been accepted for inclusion in Swiss American Historical Society Review by an authorized editor of BYU ScholarsArchive. For more information, please contact [email protected], [email protected]. Mannone: A Propensity for Genius A Propensity for Genius: That Something Special About Fritz Zwicky (1898 - 1974) by John Charles Mannone Preface It is difficult to write just a few words about a man who was so great. It is even more difficult to try to capture the nuances of his character, including his propensity for genius as well as his eccentric behavior edging the abrasive as much as the funny, the scope of his contributions, the size of his heart, and the impact on society that the distinguished physicist, Fritz Zwicky (1898- 1974), has made. So I am not going to try to serve that injustice, rather I will construct a collage, which are cameos of his life and accomplishments. In this way, you, the reader, will hopefully be left with a sense of his greatness and a desire to learn more about him. -
The Oscillating Slit Micrometer of the Meridian Circle Pmc 190 Tokyo
THE OSCILLATING SLIT MICROMETER OF THE MERIDIAN CIRCLE PMC 190 TOKYO C. Kuhne, Carl Zeiss, D-7082 Oberkochen, Federal Republic of Germany M. Miyamoto, M. Yoshizawa, Tokyo Astronomical Observatory, Mitaka, Tokyo 181, Japan ABSTRACT The meridian circle installed at the Tokyo Astronomical Observatory in 1982/83 is equipped with a photoelectric Double Slit Micrometer which is one of the basic prerequisites for fully automatic observation. A slit plate is located in the image field of the telescope. It oscil lates parallel to right ascension while being guided at the mean tra veling speed of the star. The paper describes the procedure by which the moment of the star pas sage through the instruments meridian and declination is determined. Furthermore, the autocollimation devices are described which are an essential prerequisite for the determination and periodical checking of the instrumental errors. Also, the measuring devices for the passage of the sun and the moon are dealt with briefly. 1 . INTRODUCTION The Double Slit Micrometer was introduced in 1972 by the first author during the engineering phase of the meridian circle project. The con cept is based on the multislit micrometer used by E. H<6g (1970) at the meridian circle in Perth. The +_ 45° inclination was retained, but the multitude of slits was replaced by only one movable pair. Therefore, the system became independent of the starfs velocity, a higher degree of statistic averaging could be applied, and a more simple and stable kind of collimation measurement became available. 2. DESIGN PRINCIPLE The telescope of the PMC 190 has a double-walled tube whose inner part houses the objective and the section of the micrometer which has to per- 379 H. -
Chapter 7 Mapping The
BASICS OF RADIO ASTRONOMY Chapter 7 Mapping the Sky Objectives: When you have completed this chapter, you will be able to describe the terrestrial coordinate system; define and describe the relationship among the terms com- monly used in the “horizon” coordinate system, the “equatorial” coordinate system, the “ecliptic” coordinate system, and the “galactic” coordinate system; and describe the difference between an azimuth-elevation antenna and hour angle-declination antenna. In order to explore the universe, coordinates must be developed to consistently identify the locations of the observer and of the objects being observed in the sky. Because space is observed from Earth, Earth’s coordinate system must be established before space can be mapped. Earth rotates on its axis daily and revolves around the sun annually. These two facts have greatly complicated the history of observing space. However, once known, accu- rate maps of Earth could be made using stars as reference points, since most of the stars’ angular movements in relationship to each other are not readily noticeable during a human lifetime. Although the stars do move with respect to each other, this movement is observable for only a few close stars, using instruments and techniques of great precision and sensitivity. Earth’s Coordinate System A great circle is an imaginary circle on the surface of a sphere whose center is at the center of the sphere. The equator is a great circle. Great circles that pass through both the north and south poles are called meridians, or lines of longitude. For any point on the surface of Earth a meridian can be defined. -
Internet Engineering Jan Nikodem, Ph.D. Software Engineering
Internet Engineering Jan Nikodem, Ph.D. Software Engineering Theengineering paradigm Software Engineering Lecture 3 The term "software crisis" was coined at the first NATO Software Engineering Conference in 1968 by: Friedrich. L. Bauer Nationality;German, mathematician, theoretical physicist, Technical University of Munich Friedrich L. Bauer 1924 3/24 The term "software crisis" was coined at the first NATO Software Engineering Conference in 1968 by: Peter Naur Nationality;Dutch, astronomer, Regnecentralen, Niels Bohr Institute, Technical University of Denmark, University of Copenhagen. Peter Naur 1928 4/24 Whatshouldbe ourresponse to software crisis which provided with too little quality, too late deliver and over budget? Nationality;Dutch, astronomer, Regnecentralen, Niels Bohr Institute, Technical University of Denmark, University of Copenhagen. Peter Naur 1928 5/24 Software should following an engineering paradigm NATO conference in Garmisch-Partenkirchen, 1968 Peter Naur 1928 6/24 The hope is that the progress in hardware will cure all software ills. The Oberon System User Guide and Programmer's Manual. ACM Press Nationality;Swiss, electrical engineer, computer scientist ETH Zürich, IBM Zürich Research Laboratory, Institute for Media Communications Martin Reiser 7/24 However, a critical observer may notethat software manages to outgrow hardware in size and sluggishness. The Oberon System User Guide and Programmer's Manual. ACM Press Nationality;Swiss, electrical engineer, computer scientist ETH Zürich, IBM Zürich Research Laboratory, Institute for Media Communications Martin Reiser 8/24 Wirth's computing adage Software is getting slower more rapidly than hardware becomes faster. Nationality;Swiss, electronic engineer, computer scientist ETH Zürich, University of California, Berkeley, Stanford University University of Zurich. Xerox PARC. -
Astrometry and Optics During the Past 2000 Years
1 Astrometry and optics during the past 2000 years Erik Høg Niels Bohr Institute, Copenhagen, Denmark 2011.05.03: Collection of reports from November 2008 ABSTRACT: The satellite missions Hipparcos and Gaia by the European Space Agency will together bring a decrease of astrometric errors by a factor 10000, four orders of magnitude, more than was achieved during the preceding 500 years. This modern development of astrometry was at first obtained by photoelectric astrometry. An experiment with this technique in 1925 led to the Hipparcos satellite mission in the years 1989-93 as described in the following reports Nos. 1 and 10. The report No. 11 is about the subsequent period of space astrometry with CCDs in a scanning satellite. This period began in 1992 with my proposal of a mission called Roemer, which led to the Gaia mission due for launch in 2013. My contributions to the history of astrometry and optics are based on 50 years of work in the field of astrometry but the reports cover spans of time within the past 2000 years, e.g., 400 years of astrometry, 650 years of optics, and the “miraculous” approval of the Hipparcos satellite mission during a few months of 1980. 2011.05.03: Collection of reports from November 2008. The following contains overview with summary and link to the reports Nos. 1-9 from 2008 and Nos. 10-13 from 2011. The reports are collected in two big file, see details on p.8. CONTENTS of Nos. 1-9 from 2008 No. Title Overview with links to all reports 2 1 Bengt Strömgren and modern astrometry: 5 Development of photoelectric astrometry including the Hipparcos mission 1A Bengt Strömgren and modern astrometry .. -
212 Publications of the Some Pioneer
212 PUBLICATIONS OF THE SOME PIONEER OBSERVERS1 By Frank Schlesinger In choosing a subject upon which to speak to you this eve- ning, I have had to bear in mind that, although this is a meeting of the Astronomical Society of the Pacific, not many of my audience are astronomers, and I am therefore debarred from speaking on too technical a matter. Under these circumstances I have thought that a historical subject, and one that has been somewhat neglected by the, formal historians of our science, may be of interest. I propose to outline, very briefly of course, the history of the advances that have been made in the accuracy of astronomical measurements. To do this within an hour, I must confine myself to the measurement of the relative places of objects not very close together, neglecting not only measure- ments other than of angles, but also such as can be carried out, for example, by the filar micrometer and the interferometer; these form a somewhat distinct chapter and would be well worth your consideration in an evening by themselves. It is clear to you, I hope, in how restricted a sense I am using the word observer ; Galileo, Herschel, and Barnard were great observers in another sense and they were great pioneers. But of their kind of observing I am not to speak to you tonight. My pioneers are five in number ; they are Hipparchus in the second century b.c., Tycho in the sixteenth century, Bradley in the eighteenth, Bessel in the first half of the nineteenth century and Rüther fur d in the second half. -
Reflections December 2020
Surviving the Bobcat Fire By Robert Anderson As recently as December 9, our solar astronomer, Steve Padilla, was taking his evening walk and noticed the smoke of a hotspot flaring up in the canyon just below the Observatory. It was a remnant of the Bobcat Fire, which started nearby on September 6. The local Angeles National Forest firefighters were notified of the flareup, either to monitor it or extinguish it if needed. They have returned many times during the last three months. And we are always glad to see them, especially those individuals who put water to flame here and battled to save the most productive and famous observatory in history. On the sunny Labor Day weekend, when the Bobcat Fire started near Cogswell Reservoir in a canyon east of the Mount Wilson, the Observatory’s maintenance staff went on cautious alert. As the fire spread out of control, it stayed to the east burning north and south of the reservoir for days, threatening communities in the foothills of the San Gabriels. Nevertheless, all non-essential staff and residents were evacuated off the mountain just in case. Under a surreal, smoke-filled September sky, crews David Cendejas, the superintendent of the Observatory, prepare to defend the Observatory. Photo: D. Cendejas and a skeleton crew of CHARA staff, stayed to monitor the situation and to secure the grounds. Routine year- round maintenance of Mount Wilson always includes In this issue . clearing a wide perimeter of combustibles from the buildings, but when a large fire is burning nearby, clearing Surviving the Fire ……………1 Betelgeuse & Baade …………….5 anything that has been missed becomes an urgent priority, News + Notes .….………………2 Thanks to our Supporters! ..….7 along with double-checking all the fire equipment. -
Boolean Matrix in the Matrix Equation (19)
General Disclaimer One or more of the Following Statements may affect this Document This document has been reproduced from the best copy furnished by the organizational source. It is being released in the interest of making available as much information as possible. This document may contain data, which exceeds the sheet parameters. It was furnished in this condition by the organizational source and is the best copy available. This document may contain tone-on-tone or color graphs, charts and/or pictures, which have been reproduced in black and white. This document is paginated as submitted by the original source. Portions of this document are not fully legible due to the historical nature of some of the material. However, it is the best reproduction available from the original submission. Produced by the NASA Center for Aerospace Information (CASI) C f I l 1 ^o } Technical Report 69-86 March 1969 Design Automation by the Computer Design Language by Yaohan Cho Professor fr N he computer time used was supported by the National Aeronautics and Space Administration under Grant NsO 398 to the Computer Science Center of the University of Maryland. /i Abstract A Computer Design Language (CDL) has been developed for facilitating design automation of digital computers. When the functional organizatl.on and sequential operation of a digital computer are conceived and specified by the CDL, this d CDL description is called a Macro design. The macro design is highly descriptive in computer elements. it describes precisely and concisely what the computer is expected to do functionally step by step. -
Die Hamburger Sternwarte Begründung Des Außergewöhnlichen Universellen Wertes
Die Hamburger Sternwarte Begründung des außergewöhnlichen universellen Wertes The Hamburg Observatory Justification of outstanding universal value Freie und Hansestadt Hamburg Kulturbehörde TENTATIVE LIST SUBMISSION FORMAT STATE PARTY: Germany DATE OF SUBMISSION: 2012 Submission prepared by: Name: Dr. Matthias Hünsch, Dr. Agnes Seemann, Prof. Dr. Gudrun Wolfschmidt Address: Große Bleichen 30, D-20354 Hamburg Institution: Freie und Hansestadt Hamburg/ Kulturbehörde/ Denkmalschutzamt E-mail: [email protected] Fax: +49 40 42731-0008 Telephone: +49 40 42824-750 NAME OF PROPERTY: Hamburger Sternwarte State, Province or Region: Hamburg/Germany Latitude and Longitude, or UTM coordinates: 582320, 5926440 (ETRS 1989, UTM Zone 32 N) DESCRIPTION: The Hamburg Observatory in Bergedorf was built between 1906 and 1912. It replaced the old observatory located at Millerntor on the western part of the ramparts around the core of Hamburg City. At the time, the new facility in Hamburg-Bergedorf was considered to be among the most modern and largest of Europe. About 20 kilometers away from the city centre, it was placed on a hill and extended over an area of some seven hectares that resembled a park. The facility consists of the main building, three residential buildings, several domes, the solar building and sheds for the various telescopes. There were several ancillary buildings, too. The design of the facility can be termed modern in that it was placed on a hill and far away from the city. Also, the fact that the instruments were housed in several buildings spread over the entire grounds was a new feature. The Hamburg Observatory is one of the first where the principle of setting up the instruments in a large ensemble of buildings was consistently put into practice. -
Niels Ivar Bech
Niels Ivar Bech Born 1920 Lemvig, Denmark; died 1975; originator of Danish computer development. Niels Ivar Bech was one of Europe's most creative leaders in the field of electronic digital computers.1 He originated Danish computer development under the auspices of the Danish Academy of Technical Sciences and was first managing director of its subsidiary, Regnecentralen, which was Denmark's (and one of Europe's) first independent designer and builder of electronic computers. Bech was born in 1920 in Lemvig, a small town in the northwestern corner of Jutland, Denmark; his schooling ended with his graduation from Gentofte High School (Statsskole) in 1940. Because he had no further formal education, he was not held in as high esteem as he deserved by some less gifted people who had degrees or were university professors. During the war years, Bech was a teacher. When Denmark was occupied by the Nazis, he became a runner for the distribution of illegal underground newspapers, and on occasion served on the crews of the small boats that perilously smuggled Danish Jews across the Kattegat to Sweden. After the war, from 1949 to 1957, he worked as a calculator in the Actuarial Department of the Copenhagen Telephone Company (Kobenhavns Telefon Aktieselskab, KTA). The Danish Academy of Technical Sciences established a committee on electronic computing in 1947, and in 1952 the academy obtained free access to the complete design of the computer BESK (Binar Electronisk Sekevens Kalkylator) being built in Stockholm by the Swedish Mathematical Center (Matematikmaskinnamndens Arbetsgrupp). In 1953 the Danish academy founded a nonprofit computer subsidiary, Regnecentralen.