Improving Point Cloud Quality for Mobile Laser Scanning

Total Page:16

File Type:pdf, Size:1020Kb

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. Ich danke zudem meinen Eltern, deren Unterstützung unschätzbaren Wert hat, meinen Geschwister, Niels, Tim und Tobias, meiner brillianten Kollegin und besten Freundin Dorit Borrmann, die mir immer mit Rat und Tat zur Seite stand, und allen meinen anderen Freunden, die es ebenfalls verdient haben, erwähnt zu werden. Aus tiefstem Herzen vielen Dank! v Contents 1 Introduction 1 1.1 Applications of Laser Scanning . 4 1.2 Laser Scanners and Other Range Sensors . 10 2 Rigid registration for terrestrial laser scanning 19 2.1 Registration based on Artificial Landmarks . 22 2.2 Automatic Registration . 23 2.2.1 Globally Consistent 3D Mapping with Scan Matching . 25 2.2.2 Study of Parameterizations for the Rigid Body Transformations of the Scan Registration Problem . 53 2.3 Point Cloud Processing . 99 2.3.1 An Octree for Efficient Processing of 3D Laser Scans . 99 2.3.2 Comparison of Nearest-Neighbor-Search Strategies and Implementations for Efficient Shape Registration . 135 3 Mobile Laser Scanning 155 3.1 Irma3D . 158 3.2 Algorithmic Solutions for computing accurate maximum likelihood 3D Point Clouds from Mobile Laser Scanning Platforms . 165 4 Conclusion 205 vii Chapter 1 Introduction We shall not cease from exploration And the end of all our exploring Will be to arrive where we started And know the place for the first time. T.S. Eliot, Little Gidding The science of surveying, the art of measuring space, the quantification of distances and angles are all ancient dating back to at least the old kingdom of Egypt. As early as 2540 BC the Egyptians were capable of constructing almost perfectly aligned and proportioned Pyramids using only simple tools and basic geometry [43]. Since then many advances have been made in these fields. From the classical Dioptra over the Azimuthal Quadrant to the modern Theodo- lite, surveyors developed ever more accurate and powerful tools (Fig. 1.1). Concurrent with the increasing complexity of the equipment and the increasing number of applications, advanced mathematical methods were also developed simultaneously. For example, the method of trian- gulation, which is still used to this day, was first described by Gemma Frisius in 1533 [32]. More often than not mathematical advances preceded or encouraged the development of technologies. The solution to the problem of longitude, that is, the task of determining the longitudinal co- ordinate of a point at sea, was well known in theory many decades before it could be solved in practice, by John Harrison when he invented the marine chronometer [68]. In 1997 one of the most versatile and powerful tools for surveying, the laser scanner, appeared on the market. A laser scanner, essentially a combination of a theodolite and a laser range finder, is capable of taking several thousands of range and angle measurements a second. The ability to rapidly acquire spatial data has led to a surge of new developments not only in the field of surveying but also in related fields such as robotics and computer science. As is frequently the case in computer science, this new technology has revealed a multitude of computational problems that are in need of algorithmic solutions. This thesis is the result of several years of research and of investigating solutions to the challenges that have newly emerged. During this time these new measurement devices were used for a variety of different applications. The most straight-forward use of a laser scanner is certainly as a surveying tool. First, one acquires several views on whatever the object, building or environment to be surveyed. Then one assembles a map, using either classical surveying 1 2 CHAPTER 1. INTRODUCTION Fig. 1.1: Top from left to right: A Dioptra, an Azimuthal Quadrant and a theodolite. All these devices are used for angle measurements of points relative to the observer. The Dioptra is an ancient tool that was invented at least 2000 years ago [1]. In the 13th century the Persian scholar Nasir al-Din al-Tusi invented the Azimuthal Quadrant for observing the movement of celestial bodies [41]. The theodolite was invented in the 16th century by Martin Waldseemüller who called it the polimetrum [2]. Since then many improvements to the original design have been made, resulting in modern theodolites such as the Topcon DT-205 (bottom left) [16]. The combination of a range finder with these devices is embodied by the tachymeter (bottom middle). The Cyrax 2400 (bottom right) is one of the first laser scanners to appear on the market in 1998 [27]. Laser scanners can be considered an advanced development of the tachymeter, in the sense that they acquire the same measurements, only at a much higher rate and do not require special targets. Images taken from the manufacturers. techniques or automatic algorithmic solutions. Automating this process further, by fixing the laser scanner on a mobile platform, creates yet again new opportunities and new challenges. Recently, this has culminated in a new process called mobile laser scanning, where the laser scanner is in use while the mobile platform is in motion. The opportunities inherent in this mode Improving Point Cloud Quality for Mobile Laser Scanning 3 of operation are obvious for robotics. The laser scanner is transformed from a surveying tool into a sensor valuable to the robot itself. The laser scanner enables a new mode of experiencing the environment that other sensors either cannot provide to such precision or only provide indirectly. Although a laser scanner gives a purely metrical impression of the world, machine learning techniques can be used to extract additional semantic information out of the data as well. The main focus has been to develop methods for creating accurate digital models of the world by using spatial information that is captured by laser scanners. These algorithms ought to require the least amount of human intervention as possible, ideally none at all, to the main benefit of automating and therefore speeding up these processes. The resulting model of the world is supposed to bea spatial likeness of the object or scene that has been captured. For this, one strives to create accurate, precise, yet compact representations of the data. Combining these should not only be possible, but easy, so as to create more accurate and more detailed representations of the world. This thesis is an accumulation of my work done on the topic of laser scanning in the format of a collection of journal articles. The papers herein have been peer-reviewed by an international community of scientists and experts in the field of computer science, robotics, artificial intelligence or surveying or a combination thereof. All of the following documents have therefore appeared in other publications before. Manuscripts that appear in this work: D. Borrmann, J. Elseberg, K. Lingemann, A. Nüchter, and J. Hertzberg. Globally Consistent 3D Mapping with Scan Matching. Journal of Robotics and Autonomous Systems (JRAS), 56(2):130– 142, February 2008. http://www.journals.elsevier.com/robotics-and-autonomous-systems J. Elseberg, D. Borrmann, and A. Nüchter. Algorithmic solutions for computing precise maxi- mum likelihood 3D point clouds from mobile laser scanning platforms. Remote Sensing (accepted) , 2013. http://www.mdpi.com/journal/remotesensing J. Elseberg, D. Borrmann, and A. Nüchter. One Billion Points in the Cloud - An Octree for Efficient Processing of 3D Laser Scans. ISPRS Journal of Photogrammetry and Remote Sensing, 76(0):76–88, 2013. http://www.journals.elsevier.com/isprs-journal-of-photogrammetry- and-remote-sensing J. Elseberg, S. Magnenat, R. Siegwart, and A. Nüchter. Comparison of Nearest-Neighbor- Search Strategies and Implementations for Efficient Shape Registration. Journal of Software Engineering for Robotics (JOSER), 3(1):2 – 12, 2012. http://www.joser.org A. Nüchter, J. Elseberg, P. Schneider, and D. Paulus. Study of Parameterizations for the Rigid Body Transformations of The Scan Registration Problem. Journal Computer Vision and Image Understanding (CVIU), 114(8):963–980, August 2010. http://www.journals.elsevier. com/computer-vision-and-image-understanding Improving Point Cloud Quality for Mobile Laser Scanning 4 CHAPTER 1. INTRODUCTION Fig. 1.2: Two green laser beams are pointed at the moon by the Laser Ranging Facility at the Geophys- ical and Astronomical Observatory at NASA’s Goddard Space Flight Center in Greenbelt, Md.
Recommended publications
  • 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 ..........................................................................................................
    [Show full text]
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • Mathematical Instruments Commonly Used Among the Ottomans
    Advances in Historical Studies, 2019, 8, 36-57 http://www.scirp.org/journal/ahs ISSN Online: 2327-0446 ISSN Print: 2327-0438 Mathematical Instruments Commonly Used among the Ottomans Irem Aslan Seyhan Department of Philosophy, Bartın University, Bartın, Turkey How to cite this paper: Seyhan, I. A. Abstract (2019). Mathematical Instruments Com- monly Used among the Ottomans. Ad- At the end of 17th century and during 18th century, after devastating Russian vances in Historical Studies, 8, 36-57. wars the Ottomans realized that they fell behind of the war technology of the https://doi.org/10.4236/ahs.2019.81003 Western militaries. In order to catch up with their Western rivals, they de- cided that they had to reform their education systems. For that they sent sev- Received: January 24, 2019 Accepted: March 5, 2019 eral students to abroad for education and started to translate Western books. Published: March 8, 2019 They established Western style military academies of engineering. They also invited foreign teachers in order to give education in these institutes and they Copyright © 2019 by author(s) and consulted them while there were preparing the curriculum. For all these, Scientific Research Publishing Inc. This work is licensed under the Creative during the modernization period, the reform (nizâm-ı cedid) planers mod- Commons Attribution International elled mainly France, especially for teaching the applied disciplines. Since their License (CC BY 4.0). main aim was to grasp the technology of the West, their interest focused on http://creativecommons.org/licenses/by/4.0/ the applied part of sciences and mathematics.
    [Show full text]
  • LIMITATIONS of METHODS: the ACCURACY of the VALUES MEASURED for the EARTH’S/SUN’S ORBITAL ELEMENTS in the MIDDLE EAST, A.D
    JHA, xliv (2013) LIMITATIONS OF METHODS: THE ACCURACY OF THE VALUES MEASURED FOR THE EARTH’S/SUN’S ORBITAL ELEMENTS IN THE MIDDLE EAST, A.D. 800–1500, PART 1 S. MOHAMMAD MOZAFFARI, Research Institute for Astronomy and Astrophysics of Maragha The present paper deals with the methods proposed and the values achieved for the eccentricity and the longitude of apogee of the (apparent) orbit of the Sun in the Ptolemaic context in the Middle East during the medieval period. The main goals of this research are as follows: first, to determine the accuracy of the historical values in relation to the theoretical accuracy and/or the intrinsic limitations of the methods used; second, to investigate whether medieval astronomers were aware of the limita- tions, and if so, which alternative methods (assumed to have a higher accuracy) were then proposed; and finally, to see what was the fruit of the substitution in the sense of improving the accuracy of the values achieved. In Section 1, the Ptolemaic eccentric orbit of the Sun and its parameters are introduced. Then, its relation to the Keplerian elliptical orbit of the Earth, which will be used as a criterion for comparing the historical values, is briefly explained. In Section 2, three standard methods of measurement of the solar orbital elements in the medieval period found in the primary sources are reviewed. In Section 3, more than twenty values for the solar eccentricity and longitude of apogee from the medieval period will be classified, provided with historical comments. Discus- sion and conclusions will appear in Section 4 (in Part 2), followed there by two discussions of the medieval astronomers’ considerations of the motion of the solar apogee and their diverse interpretations of the variation in the values achieved for the solar eccentricity.
    [Show full text]
  • Some Board of Longitude Instruments in the Nineteenth Century
    SOME BOARD OF LONGITUDE INSTRUMENTS IN THE NINETEENTH CENTURY A.N. STIMSON National Maritime Museum, Greenwich, London A series of calamitous British disasters at sea occurred at the turn of the 17th century, many of which can be attributed to poor navigation compounded by inability to find longitude. Perhaps the most momentous was that of Sir Cloudsley Shovel's returning Mediterranean Squadron which was comprehensively wrecked on the Scilly Islands in 1707 with the loss of four large warships and nearly 2000 men.1 An increasing public outcry at this regular loss of life and keenly felt loss of trade revenue resulted in an Act of Parliament which was intended to improve the inadequate state of navigation by stimulating an answer to the seemingly impossible problem of finding longitude at sea. On 20th July, 1714 Queen Anne gave her assent to "A Bill for Providing a Public Reward for such Person or Persons as shall Discover the Longitude at Sea". £ 20,000, an enormous sum of money at that time, was to be awarded to anyone who could provide a practical solution of general utility which would enable a navigator to find his ship's position to within twenty geographical miles. Lesser sums were to be awarded for methods which produced less accurate results.2 To oversee the management of these awards and to judge the prac- ticability of the solutions proposed, the Act provided for a Board of Commissioners. This was composed of the best scientific and seafaring minds of the day in addition to the inevitable political appointments.
    [Show full text]
  • An Overview of Ottoman Scientific Activities December 2006
    An Overview of Ottoman Scientific Activities IMPORTANT NOTICE: Author: Prof. Ekmeleddin Ihsanoglu Chief Editor: Prof. Mohamed El-Gomati All rights, including copyright, in the content of this document are owned or controlled for these purposes by FSTC Limited. In Associate Editor: Dr. Salim Ayduz accessing these web pages, you agree that you may only download the content for your own personal non-commercial Production: Savas Konur use. You are not permitted to copy, broadcast, download, store (in any medium), transmit, show or play in public, adapt or change in any way the content of this document for any other purpose whatsoever without the prior written permission of FSTC Release Date: December 2006 Limited. Publication ID: 629 Material may not be copied, reproduced, republished, downloaded, posted, broadcast or transmitted in any way except for your own personal non-commercial home use. Any other use Copyright: © FSTC Limited, 2006 requires the prior written permission of FSTC Limited. You agree not to adapt, alter or create a derivative work from any of the material contained in this document or use it for any other purpose other than for your personal non-commercial use. FSTC Limited has taken all reasonable care to ensure that pages published in this document and on the MuslimHeritage.com Web Site were accurate at the time of publication or last modification. Web sites are by nature experimental or constantly changing. Hence information published may be for test purposes only, may be out of date, or may be the personal opinion of the author. Readers should always verify information with the appropriate references before relying on it.
    [Show full text]
  • THE ENTRANCE of MODERN OPTICS to OTTOMAN SCIENCE by Sena Pekkendir B.S., Physics, Boğaziçi University, 2011 Submitted To
    THE ENTRANCE OF MODERN OPTICS TO OTTOMAN SCIENCE by Sena Pekkendir B.S., Physics, Boğaziçi University, 2011 Submitted to the Institute for Graduate Studies in Science and Engineeering in partial fulfillment of the requirements for the degree of Master of Science Graduate Program in Physics Boğaziçi University 2015 ii THE ENTRANCE OF MODERN OPTICS TO OTTOMAN SCIENCE APPROVED BY: Prof. Levent Kurnaz ………………………... (Thesis Supervisor) Prof. İhsan Fazlıoğlu ………………………… (Thesis Co-advisor) Assoc. Prof. Burçin Ünlü ………………………… Prof. Edhem Eldem ………………………… Prof. Naci İnci ………………………… DATE OF APPROVAL: 02.07.2015 iii Dedicated to my husband Behiç and my son Ömer Melih iv ACKNOWLEDGEMENTS First of all, I’d like to express my sincere gratitude to my thesis advisor Prof. Levent Kurnaz for teaching me how to do academic research at first by joining me to his Soft Condensed Matter Lab when I was a sophomore. Also I’m very lucky to have been attended to his lectures on History of Science for that I discovered the branch I want to spend my life with. I’m so thankful to him to encourage and support me to write a thesis on history of science. I’d like to express my gratitude to Prof. İhsan Fazlıoğlu for always forcing me to be better and for teaching me a great deal of wisdom of academy. I’m very grateful for the things I’ve learned from him and I’m lucky that I’ll continue learning from him in the upcoming years. I also would like to thank my mother Sera Sarı for being there whenever I need her and always supporting me.
    [Show full text]
  • Third-Order Frequency-Resolved Photon Correlations from a Single Quantum Dot's Resonance Fluorescence
    University of South Florida Scholar Commons Graduate Theses and Dissertations Graduate School March 2021 Third-Order Frequency-Resolved Photon Correlations from a Single Quantum Dot's Resonance Fluorescence Yamil A. Nieves González University of South Florida Follow this and additional works at: https://scholarcommons.usf.edu/etd Part of the Physics Commons Scholar Commons Citation Nieves González, Yamil A., "Third-Order Frequency-Resolved Photon Correlations from a Single Quantum Dot's Resonance Fluorescence" (2021). Graduate Theses and Dissertations. https://scholarcommons.usf.edu/etd/8834 This Dissertation is brought to you for free and open access by the Graduate School at Scholar Commons. It has been accepted for inclusion in Graduate Theses and Dissertations by an authorized administrator of Scholar Commons. For more information, please contact [email protected]. Third-Order Frequency-Resolved Photon Correlations from a Single Quantum Dot’s Resonance Fluorescence by Yamil A. Nieves González A dissertation submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy Department of Physics College of Art and Sciences University of South Florida Major Professor: Andreas Muller, Ph.D. Myung Kim, Ph.D. Dmitry Voronine, Ph.D. Theresa Evans-Nguyen, Ph.D. Date of Approval: February 11, 2021 Keywords: Semiconductor, Photon statistics, Quantum optics, Quantum emitter Copyright c 2021, Yamil A. Nieves González Dedication Para mi padre y madre, Anibal y Zoraida, quienes no saben ingles y, por tanto, no comprederan nada en esta disertación y aún así se enorgullecerán igual y para mi abuelo, Luis Camargo, quién, de niño, me empujó a una carrera en medicina, pero mi rebelde ser optó por estudiar Física.
    [Show full text]
  • The Scientific Instruments of the Lewis and Clark Expedition
    University of Nebraska - Lincoln DigitalCommons@University of Nebraska - Lincoln Great Plains Quarterly Great Plains Studies, Center for Winter 1984 The Scientific Instruments Of The Lewis And Clark Expedition Silvio A. Bedini Smithsonian Institution Follow this and additional works at: https://digitalcommons.unl.edu/greatplainsquarterly Part of the Other International and Area Studies Commons Bedini, Silvio A., "The Scientific Instruments Of The Lewis And Clark Expedition" (1984). Great Plains Quarterly. 1811. https://digitalcommons.unl.edu/greatplainsquarterly/1811 This Article is brought to you for free and open access by the Great Plains Studies, Center for at DigitalCommons@University of Nebraska - Lincoln. It has been accepted for inclusion in Great Plains Quarterly by an authorized administrator of DigitalCommons@University of Nebraska - Lincoln. THE SCIENTIFIC INSTRUMENTS OF THE LEWIS AND CLARK EXPEDITION SILVIO A. BEDINI The Lewis and Clark expedition, "the most on national geography than anyone else in the consequential and romantic peace-time achieve­ United States. He had spent many years collect­ ment in American history," had its genesis in ing and studying all that had been written and the mind of Thomas Jefferson fully two de­ published about the subject, and he had had cades before the exploring party departed from ample opportunity to meet Indians and others Pittsburgh on 31 August 1803.1 The need to who had traveled in the West and to record all determine the character and . expanse of the that he could learn from them. He was knowl­ western regions of the continent lingered in his edgeable about scientific practices and instru­ mind, and during the intervening years he en­ ments and was experienced in surveying, map­ couraged three unsuccessful attempts to explore ping, and making astronomical observations, them.
    [Show full text]
  • AST 112: Lab #3 the Celestial Sphere
    Name: ____________________ Partner(s): ________________ ________________ AST 112: Lab #3 The Celestial Sphere Objectives To use celestial coordinates to locate objects in the sky To locate objects in the sky with the Celestial Sphere and other sky charts To determine when objects in the sky will be visible in the night sky To determine the position of the Sun against the background of the stars To sketch a variety of constellations as they appear on the night sky using the Celestial Sphere To note the constellations of the zodiac and approximately the dates the Sun will cross in front of them Materials Celestial Sphere Star wheel Star chart Flip chart References Lab Manual for AST 102, Hopkins The Constellations: An Enthusiast’s Guide to the Night Sky, Motz & Nathanson Norton’s Star Atlas and Reference Handbook, 20th ed., ed. Ridpath The Box of Stars, Tenant Introduction In ancient times, people believed the Earth was immobile and surrounded by a sphere to which the stars were attached. This Celestial Sphere would revolve about the Earth once each day, carrying the stars along with it. While today we know the Earth is the object that moves, it is still convenient to describe the sky in this manner for the purpose of determining the positions of objects in the sky (a science called astrometry). We will use a model Celestial Sphere (and other sky charts) to describe the positions and appearances of various stars and constellations. We will also evaluate when certain objects will be visible in our night sky from our location.
    [Show full text]