Mathematical Instruments Commonly Used Among the Ottomans
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Improving Point Cloud Quality for Mobile Laser Scanning
School of Engineering and Science Dissertation for a Ph.D. in Computer Science Improving Point Cloud Quality for Mobile Laser Scanning Jan Elseberg November 2013 Supervisor: Prof. Dr. Andreas Nüchter Second Reviewer: Prof. Dr. Andreas Birk Third Reviewer: Prof. Dr. Joachim Hertzberg Fourth Reviewer: Prof. Dr. Rolf Lakämper Date of Defense: 13th of September 2013 Abstract This thesis deals with mobile laser scanning and the complex challenges that it poses to data processing, calibration and registration. New approaches to storing, searching and displaying point cloud data as well as algorithms for calibrating mobile laser scanners and registering laser scans are presented and discussed. Novel methods are tested on state of the art mobile laser scanning systems and are examined in detail. Irma3D, an autonomous mobile laser scanning platform has been developed for the purpose of experimentation. This work is the result of several years of research in robotics and laser scanning. It is the accumulation of many journal articles and conference papers that have been reviewed by peers in the field of computer science, robotics, artificial intelligence and surveying. Danksagung The work that goes into finishing a work like this is long and arduous, yet it can at times be pleasing, exciting and even fun. I would like to thank my advisor Prof. Dr. Andreas Nüchter for providing such joy during my experiences as a Ph.D. student. His infectious eagerness for the subject and his ability to teach are without equal. Prof. Dr. Joachim Hertzberg deserves many thanks for introducing me to robotics and for being such an insightful teacher of interesting subjects. -
Abd Al-Rahman Al-Sufi and His Book of the Fixed Stars: a Journey of Re-Discovery
ResearchOnline@JCU This file is part of the following reference: Hafez, Ihsan (2010) Abd al-Rahman al-Sufi and his book of the fixed stars: a journey of re-discovery. PhD thesis, James Cook University. Access to this file is available from: http://eprints.jcu.edu.au/28854/ The author has certified to JCU that they have made a reasonable effort to gain permission and acknowledge the owner of any third party copyright material included in this document. If you believe that this is not the case, please contact [email protected] and quote http://eprints.jcu.edu.au/28854/ 5.1 Extant Manuscripts of al-Ṣūfī’s Book Al-Ṣūfī’s ‘Book of the Fixed Stars’ dating from around A.D. 964, is one of the most important medieval Arabic treatises on astronomy. This major work contains an extensive star catalogue, which lists star co-ordinates and magnitude estimates, as well as detailed star charts. Other topics include descriptions of nebulae and Arabic folk astronomy. As I mentioned before, al-Ṣūfī’s work was first translated into Persian by al-Ṭūsī. It was also translated into Spanish in the 13th century during the reign of King Alfonso X. The introductory chapter of al-Ṣūfī’s work was first translated into French by J.J.A. Caussin de Parceval in 1831. However in 1874 it was entirely translated into French again by Hans Karl Frederik Schjellerup, whose work became the main reference used by most modern astronomical historians. In 1956 al-Ṣūfī’s Book of the fixed stars was printed in its original Arabic language in Hyderabad (India) by Dārat al-Ma‘aref al-‘Uthmānīa. -
UC San Diego UC San Diego Electronic Theses and Dissertations
UC San Diego UC San Diego Electronic Theses and Dissertations Title The science of the stars in Danzig from Rheticus to Hevelius / Permalink https://escholarship.org/uc/item/7n41x7fd Author Jensen, Derek Publication Date 2006 Peer reviewed|Thesis/dissertation eScholarship.org Powered by the California Digital Library University of California UNIVERSITY OF CALIFORNIA, SAN DIEGO THE SCIENCE OF THE STARS IN DANZIG FROM RHETICUS TO HEVELIUS A dissertation submitted in partial satisfaction of the requirements for the degree Doctor of Philosophy in History (Science Studies) by Derek Jensen Committee in charge: Professor Robert S. Westman, Chair Professor Luce Giard Professor John Marino Professor Naomi Oreskes Professor Donald Rutherford 2006 The dissertation of Derek Jensen is approved, and it is acceptable in quality and form for publication on microfilm: _________________________________________ _________________________________________ _________________________________________ _________________________________________ _________________________________________ Chair University of California, San Diego 2006 iii FOR SARA iv TABLE OF CONTENTS Signature Page........................................................................................................... iii Dedication ................................................................................................................. iv Table of Contents ...................................................................................................... v List of Figures .......................................................................................................... -
Bīrūnī's Telescopic-Shape Instrument for Observing the Lunar
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Revistes Catalanes amb Accés Obert Bīrūnī’s Telescopic-Shape Instrument for Observing the Lunar Crescent S. Mohammad Mozaffari and Georg Zotti Abstract:This paper deals with an optical aid named barbakh that Abū al-Ray¬ān al- Bīrūnī (973–1048 AD) proposes for facilitating the observation of the lunar crescent in his al-Qānūn al-Mas‘ūdī VIII.14. The device consists of a long tube mounted on a shaft erected at the centre of the Indian circle, and can rotate around itself and also move in the vertical plane. The main function of this sighting tube is to provide an observer with a darkened environment in order to strengthen his eyesight and give him more focus for finding the narrow crescent near the western horizon about the beginning of a lunar month. We first briefly review the history of altitude-azimuthal observational instruments, and then present a translation of Bīrūnī’s account, visualize the instrument in question by a 3D virtual reconstruction, and comment upon its structure and applicability. Keywords: Astronomical Instrumentation, Medieval Islamic Astronomy, Bīrūnī, Al- Qānūn al-Mas‘ūdī, Barbakh, Indian Circle Introduction: Altitude-Azimuthal Instruments in Islamic Medieval Astronomy. Altitude-azimuthal instruments either are used to measure the horizontal coordinates of a celestial object or to make use of these coordinates to sight a heavenly body. They Suhayl 14 (2015), pp. 167-188 168 S. Mohammad Mozaffari and Georg Zotti belong to the “empirical” type of astronomical instruments.1 None of the classical instruments mentioned in Ptolemy’s Almagest have the simultaneous measurement of both altitude and azimuth of a heavenly object as their main function.2 One of the earliest examples of altitude-azimuthal instruments is described by Abū al-Ray¬ān al- Bīrūnī for the observation of the lunar crescent near the western horizon (the horizontal coordinates are deployed in it to sight the lunar crescent). -
Hadley's Octant (A. D. 1731)
HADLEY’S OCTANT (A. D. 1731). On the occasion of the second centenary of the invention of reflecting instruments and in accordance with the usual custom of reproducing in the Hydrographic Review documents of particular interest connected with the history of nautical and hydrographic science, the communication made by John Hadley to the Royal Society of London on 13th May, 1731, is repro duced hereafter in facsimile. This communication was published in N° 420 of the Philosophical Transactions. It appears that the oldest document in which allusion is made to the principle of reflection by plane mirrors, as applied to the measurement of angles, is the History of the Royal Society of London by B ir c h . In this book, under the date of 22nd August, 1666, it is stated “ Mr. H o o k mentionned a new astronomical instrument for making observations of distances by reflection”. In another place it may be read that on the 29th August of the same year, H o o k spoke of this instrument again, it being then under construction, to the members of the Society. They invited him to submit it as soon as possible and this was done on 12th September of that year. The instrument submitted by H o o k differed in important details from the modern sextant; it was provided with but one mirror and thus was a single reflecting instrument. This was the fundamental defect which made it impos sible for H o o k ’s invention to be a success. However, the idea of using reflection from a plane mirror for the measu rement of angles was not forgotten and, in spite of H o o k ’s want of success the principle was taken up by others who sought to correct the disadvantages of the instrument as first invented. -
SIS Bulletin Issue 68
Scientific Inst~ u: nent SOciety • ~ ~': ~z ~ ........ ....... ~ :~,,, _~ , ......~ ,~ ., .. ~. "i I, ~'~..~ i;.)~ i!~ ~' • Bulletin March No. 68 2001 Bulletin of the Scientific Instrument Society IssN 0956-8271 For Table of Contents, see back cover President Gerard Turner Vice-President Howard Dawes Honorary Committee Stuart Talbot, Chairman Gloria Clifton, SecretaW John Didcock, Treasurer WiUem Hackmann, Editor Sunon Chetfetz Alexander Crum-Ewmg Peter de Clercq Tom l~mb Svh'ia Sunmra L~ba Taub Membership and Administrative Matters The Executive Officer (Wg Cdr Geoffrey Bennett) 31 HJ~h Sweet Stanford m the Vale Farmgdon Tel: 01367 710223 Oxon SNr7 8LH Fax: 01367 718963 e-mail: [email protected] See outside back cover for infvrmation on membership Editorial Matters Dr. Willem D. Hackmann Museum of the History of Science Old Ashmolean Building Tel: 01865 277282 (office) Broad Street Fax: 01865 277288 Oxford OXI 3AZ Tel: 01608 811110 (home) e-mail: willemhackmann@m~.ox,ac.uk " Society's Website http://ww~,.sis.org.uk Advertising .See 'Summary of Advertising Services' panel elsewhere in this Bulletin. Further enquiries to the Executive Officer. Typesetting and Printing IJthoflow Ltd 26-36 Wharfdale Road Tel: 020 7833 2344 King's Cross Fax: 020 7833 8150 London N1 9RY Price: £6 per issue, including back numbers where available. (Enquiries to the Executive Officer) The Scientific Instrument Society is Registered Charily No. 326733 :~ The Scientific Instrument Society 2001 i; Editorial Spring is in the Air - Somewhere maxnum opus on Elizabethan Lnstruments. Getting the March Bulletin ready always Object' brings with it a special excitement as it This issue's 'Mystery has elicited a coincides with nature awakening from its great deal of interest,and has been correctly winter slumber; there is a sense of renewal, identified as what the German's call a for measunng the of new plausibilities. -
Lunar Distances Final
A (NOT SO) BRIEF HISTORY OF LUNAR DISTANCES: LUNAR LONGITUDE DETERMINATION AT SEA BEFORE THE CHRONOMETER Richard de Grijs Department of Physics and Astronomy, Macquarie University, Balaclava Road, Sydney, NSW 2109, Australia Email: [email protected] Abstract: Longitude determination at sea gained increasing commercial importance in the late Middle Ages, spawned by a commensurate increase in long-distance merchant shipping activity. Prior to the successful development of an accurate marine timepiece in the late-eighteenth century, marine navigators relied predominantly on the Moon for their time and longitude determinations. Lunar eclipses had been used for relative position determinations since Antiquity, but their rare occurrences precludes their routine use as reliable way markers. Measuring lunar distances, using the projected positions on the sky of the Moon and bright reference objects—the Sun or one or more bright stars—became the method of choice. It gained in profile and importance through the British Board of Longitude’s endorsement in 1765 of the establishment of a Nautical Almanac. Numerous ‘projectors’ jumped onto the bandwagon, leading to a proliferation of lunar ephemeris tables. Chronometers became both more affordable and more commonplace by the mid-nineteenth century, signaling the beginning of the end for the lunar distance method as a means to determine one’s longitude at sea. Keywords: lunar eclipses, lunar distance method, longitude determination, almanacs, ephemeris tables 1 THE MOON AS A RELIABLE GUIDE FOR NAVIGATION As European nations increasingly ventured beyond their home waters from the late Middle Ages onwards, developing the means to determine one’s position at sea, out of view of familiar shorelines, became an increasingly pressing problem. -
Science and Technology in Medieval Islam
Museum of the History of Science Science and Islam Introduction to Astronomy in Islam Science and Learning in Medieval Islam • Early Islamic teaching encouraged the pursuit of all knowledge that helped to improve people’s lives • Muslims translated important works from ancient Greece and Egypt - Arabic became the international language of scholarship • Huge libraries were established in big cities like Baghdad, Cairo and Damascus Astronomy Astronomy was important to Muslims for practical reasons: • Observations of the sun and moon were used to determine prayer times and an accurate calendar • Astronomical observations were important for purposes of navigation • Astronomical observations were import for the practice of astrology Raj Jai Singh II’s observatory (C18th) in Jaipur, India Large observatories were established and new instruments such as the astrolabe were developed Ottoman observatory 1781 Photograph: The Whipple Museum, Cambridge The quadrant The quadrant is an observational instrument used to measure the angle or altitude of a celestial object. Horary quadrants also had markings on one side that would enable the user to calculate the time of day. Armillary sphere The armillary sphere was a model used to demonstrate the motions of the celestial sphere (stars) and the annual path of the sun (the ecliptic). It could also be used to demonstrate the seasons, the path of the sun in the sky for any day of the year, and to make other astronomical calculations. Early Islamic models were based on a model of the Universe established by Ptolemy in which the Earth was placed at the centre. The astrolabe The astrolabe was a type of astronomical calculator and were developed to an extraordinary level of sophistication by early Muslim scholars. -
Muslims in Pioneering Modern Knowledge: Chronicles of the Freely Or Unconsciously Surrendered Legacies to the West
Nazhruna: Jurnal Pendidikan Islam Vol. 3 No 3, 2020. Hal. 406-424 E-ISSN: 2614-8013 DOI: https://doi.org/10.31538/nzh.v3i3.805 MUSLIMS IN PIONEERING MODERN KNOWLEDGE: CHRONICLES OF THE FREELY OR UNCONSCIOUSLY SURRENDERED LEGACIES TO THE WEST Abdulrahman Yusuf Maigida Faculty of Education, University of Port Harcourt, Nigeria [email protected] Received: 30-09-2020 Revised: 10-10-2020 Accepted: 03-11-2020 Abstract The paper dwelt on exemplification of the role of early Muslim world in pioneering modern knowledge with a magnification of the legacies that these torchbearers in Islam bequeathed to the world. The peculiarity of Nigeria as a nation with more than half of its entire population as Muslims was retrospectively reviewed from the pre- colonial to colonial-era; focusing on scholasticism. The study was examined purely from the historical perspective, to appraise how the impressive efforts of the early Muslim pioneers of modern knowledge in Medicine, Chemistry, Physics, Astronomy, Geometry, Mathematics, History, Geography and Biological Sciences were undertaken. The study did not finish without the expression of concern on how the golden legacies of the early Muslim pioneers have been played down by the Muslims of today, where knowledge or groundbreaking discoveries are now credited to the West, making it look like stolen legacies or freely surrendered legacies to those who are currently worried about the development. Based on these genuine concerns, several wells thought out recommendations were penned down, not limited to a suggestion on growing above externally triggered wars and hostilities among Muslim nations, and giving peace and unity chance, to settle down to reflect on how sustainable progress can be achieved in the world of knowledge economy. -
The Islamic Connection
THE ISLAMIC CONNECTION CONTRIBUTIONS MADE BY THE ARABS TO MATHEMATICS by John E. Sasser, Ph.D. COPYRIGHT Copyright © 2007 by John E. Sasser. All rights reserved. No part of this paper may be reproduced in any form, electronic or mechanical, including photocopy recording, or any information storage or retrieval system, without permission in writing from the author. 2 The Arab Contribution to Mathematics CONTENTS Foreword...............................................……............... 4 Dedication..................................................…….......... 5 Preface........................................................…….......... 7 Map............................................................…….......... 9 List of Illustrations…………………………………... 10 Introduction..................................................……........ 11 The Search for Knowledge.....................…................. 23 Antiquity and the European Renaissance: Translations. Geometry: Geometric Constructions……………….. Trigonometry Direction Time NumberTheory: ……………………………………. The Hindu-Arabic Numeration System. Astronomy and the Calendar: Algebra: Conclusion..........................................……................. References........................................……................... Glossary……………………………………………... Index......................................................…….............. 3 The Arab Contribution to Mathematics FOREWORD This paper describes selected principal contributions to mathematics and the Arabs. Selection of appropriate examples to illustrate -
A Survey for Low-Mass Stellar and Substellar Members of the Hyades Open Cluster
Astronomy & Astrophysics manuscript no. aa30134-16˙12Jan2018 © ESO 2018 January 16, 2018 A survey for low-mass stellar and substellar members of the Hyades open cluster. Stanislav Melnikov1;2 and Jochen Eislo¨ffel1 1 Thuringer¨ Landessternwarte Tautenburg, Sternwarte 5, 07778 Tautenburg, Germany 2 Ulugh Beg Astronomical Institute, Astronomical str. 33, 700052 Tashkent, Uzbekistan Received / Accepted ABSTRACT Context. Unlike young open clusters (with ages < 250 Myr), the Hyades cluster (age ∼ 600 Myr) has a clear deficit of very low-mass stars (VLM) and brown dwarfs (BD). Since this open cluster has a low stellar density and covers several tens of square degrees on the sky, extended surveys are required to improve the statistics of the VLM/BD objects in the cluster. Aims. We search for new VLM stars and BD candidates in the Hyades cluster to improve the present-day cluster mass function down to substellar masses. Methods. An imaging survey of the Hyades with a completeness limit of 21m: 5 in the R band and 20m: 5 in the I band was carried out with the 2k × 2k CCD Schmidt camera at the 2m Alfred Jensch Telescope in Tautenburg. We performed a photometric selection of the cluster member candidates by combining results of our survey with 2MASS JHKs photometry. Results. We present a photometric and proper motion survey covering 23.4 deg2 in the Hyades cluster core region. Using optical/IR colour-magnitude diagrams, we identify 66 photometric cluster member candidates in the magnitude range 14m: 7 < I < 20m: 5. The proper motion measurements are based on several all-sky surveys with an epoch difference of 60-70 years for the bright objects. -
United States National Museum
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