NOTES and DISCUSSIONS Using a Gyroscope to Find True North—A
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Utilising Accelerometer and Gyroscope in Smartphone to Detect Incidents on a Test Track for Cars
Utilising accelerometer and gyroscope in smartphone to detect incidents on a test track for cars Carl-Johan Holst Data- och systemvetenskap, kandidat 2017 Luleå tekniska universitet Institutionen för system- och rymdteknik LULEÅ UNIVERSITY OF TECHNOLOGY BACHELOR THESIS Utilising accelerometer and gyroscope in smartphone to detect incidents on a test track for cars Author: Examiner: Carl-Johan HOLST Patrik HOLMLUND [email protected] [email protected] Supervisor: Jörgen STENBERG-ÖFJÄLL [email protected] Computer and space technology Campus Skellefteå June 4, 2017 ii Abstract Utilising accelerometer and gyroscope in smartphone to detect incidents on a test track for cars Every smartphone today includes an accelerometer. An accelerometer works by de- tecting acceleration affecting the device, meaning it can be used to identify incidents such as collisions at a relatively high speed where large spikes of acceleration often occur. A gyroscope on the other hand is not as common as the accelerometer but it does exists in most newer phones. Gyroscopes can detect rotations around an arbitrary axis and as such can be used to detect critical rotations. This thesis work will present an algorithm for utilising the accelerometer and gy- roscope in a smartphone to detect incidents occurring on a test track for cars. Sammanfattning Utilising accelerometer and gyroscope in smartphone to detect incidents on a test track for cars Alla smarta telefoner innehåller idag en accelerometer. En accelerometer analyserar acceleration som påverkar enheten, vilket innebär att den kan användas för att de- tektera incidenter så som kollisioner vid relativt höga hastigheter där stora spikar av acceleration vanligtvis påträffas. -
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. -
A Tuning Fork Gyroscope with a Polygon-Shaped Vibration Beam
micromachines Article A Tuning Fork Gyroscope with a Polygon-Shaped Vibration Beam Qiang Xu, Zhanqiang Hou *, Yunbin Kuang, Tongqiao Miao, Fenlan Ou, Ming Zhuo, Dingbang Xiao and Xuezhong Wu * College of Intelligence Science and Engineering, National University of Defense Technology, Changsha 410073, China; [email protected] (Q.X.); [email protected] (Y.K.); [email protected] (T.M.); [email protected] (F.O.); [email protected] (M.Z.); [email protected] (D.X.) * Correspondence: [email protected] (Z.H.); [email protected] (X.W.) Received: 22 October 2019; Accepted: 18 November 2019; Published: 25 November 2019 Abstract: In this paper, a tuning fork gyroscope with a polygon-shaped vibration beam is proposed. The vibration structure of the gyroscope consists of a polygon-shaped vibration beam, two supporting beams, and four vibration masts. The spindle azimuth of the vibration beam is critical for performance improvement. As the spindle azimuth increases, the proposed vibration structure generates more driving amplitude and reduces the initial capacitance gap, so as to improve the signal-to-noise ratio (SNR) of the gyroscope. However, after taking the driving amplitude and the driving voltage into consideration comprehensively, the optimized spindle azimuth of the vibration beam is designed in an appropriate range. Then, both wet etching and dry etching processes are applied to its manufacture. After that, the fabricated gyroscope is packaged in a vacuum ceramic tube after bonding. Combining automatic gain control and weak capacitance detection technology, the closed-loop control circuit of the drive mode is implemented, and high precision output circuit is achieved for the gyroscope. -
Introduction to Astronomy from Darkness to Blazing Glory
Introduction to Astronomy From Darkness to Blazing Glory Published by JAS Educational Publications Copyright Pending 2010 JAS Educational Publications All rights reserved. Including the right of reproduction in whole or in part in any form. Second Edition Author: Jeffrey Wright Scott Photographs and Diagrams: Credit NASA, Jet Propulsion Laboratory, USGS, NOAA, Aames Research Center JAS Educational Publications 2601 Oakdale Road, H2 P.O. Box 197 Modesto California 95355 1-888-586-6252 Website: http://.Introastro.com Printing by Minuteman Press, Berkley, California ISBN 978-0-9827200-0-4 1 Introduction to Astronomy From Darkness to Blazing Glory The moon Titan is in the forefront with the moon Tethys behind it. These are two of many of Saturn’s moons Credit: Cassini Imaging Team, ISS, JPL, ESA, NASA 2 Introduction to Astronomy Contents in Brief Chapter 1: Astronomy Basics: Pages 1 – 6 Workbook Pages 1 - 2 Chapter 2: Time: Pages 7 - 10 Workbook Pages 3 - 4 Chapter 3: Solar System Overview: Pages 11 - 14 Workbook Pages 5 - 8 Chapter 4: Our Sun: Pages 15 - 20 Workbook Pages 9 - 16 Chapter 5: The Terrestrial Planets: Page 21 - 39 Workbook Pages 17 - 36 Mercury: Pages 22 - 23 Venus: Pages 24 - 25 Earth: Pages 25 - 34 Mars: Pages 34 - 39 Chapter 6: Outer, Dwarf and Exoplanets Pages: 41-54 Workbook Pages 37 - 48 Jupiter: Pages 41 - 42 Saturn: Pages 42 - 44 Uranus: Pages 44 - 45 Neptune: Pages 45 - 46 Dwarf Planets, Plutoids and Exoplanets: Pages 47 -54 3 Chapter 7: The Moons: Pages: 55 - 66 Workbook Pages 49 - 56 Chapter 8: Rocks and Ice: -
Map and Compass
UE CG 039-089 2018_UE CG 039-089 2018 2018-08-29 9:57 AM Page 56 MAP The north magnetic pole is not the same as the geographic North Pole, also known as AND COMPASS true north, which is the northern end of the axis around which the earth spins. In fact, the north magnetic pole currently lies Background Information approximately 800 mi (1300 km) south of the geographic North Pole, in northern A compass is an instrument that people use Canada. And because the north magnetic to find a direction in relation to the earth as pole migrates at 6.6 mi (10 km) per year, its a whole. The magnetic needle in the location is constantly changing. compass, which is the freely moving needle in the compass that has a red end, points The meridians of longitude on maps and north. More specifically, this needle points globes are based upon the geographic to the north magnetic pole, the northern North Pole rather than the north magnetic end of the earth’s magnetic field, which pole. This means that magnetic north, the can be imagined as lines of magnetism that direction that a compass indicates as north, leave the south magnetic pole, flow north is not the same direction as maps indicate around the earth, and then enter the north for north. Magnetic declination, the magnetic pole. difference in the angle between magnetic north and true north must, therefore, be Any magnetized object, an object with two taken into account when navigating with a oppositely charged ends, such as a magnet map and a compass. -
Some Guidelines for Effective Field-Use of the GPS Unit
PRBO Conservation Science 4990 Shoreline Highway Stinson Beach, CA 94970 415-868-1221 www.prbo.org Guidelines for Field Use of Garmin GPS Units GPS Checklist: Copy an updated version of the master "allpc" shapefile and other digital basemaps, including topo quads and aerial photos, from the GIS server (V: drive) before the field season starts. Know what coordinate system (e.g., UTM, zone 10) and datum (e.g., NAD83) your project uses. The PRBO default is UTM, WGS84 (same as NAD83). In the UTM coordinate system, your zone depends on where you are (see map). Download your GPS coordinates daily, using GPS Utility (www.gpsu.co.uk/) or Waypoint+ (www.tapr.org/~kh2z/Waypoint/) shareware. It is not uncommon for Garmin units to die in the field. You will need a PC Interface cable to download your data and a registration key for GPS Utility. If you are unable to download, record your coordinates by hand in the field. Always carry extra batteries, especially if you’re not planning to revisit the site, and turn off your GPS unit when not in use to avoid draining the internal lithium battery. Contact Garmin (www.garmin.com) for replacement or repair under warranty if your unit dies. UTM Zones Submit copies of your GPS coordinate files to the GIS lab at the end of the field season for archiving and general mapping purposes. In the Field GPS Unit Setup Before taking waypoints in the field, the GPS navigation display should be set up to match the coordinate system, horizontal datum, and units used at a particular field project’s location. -
Evaluation of Gyroscope-Embedded Mobile Phones
Evaluation of Gyroscope-embedded Mobile Phones Christopher Barthold, Kalyan Pathapati Subbu and Ram Dantu∗ Department of Computer Science and Engineering University of North Texas, Denton, Texas 76201 Email: [email protected], [email protected], [email protected] ∗ Also currently visiting professor in Massachusetts Institute of Technology. Abstract—Many mobile phone applications such as pedometers accurately determine the phone’s orientation. Similar mobile and navigation systems rely on orientation sensors that most applications cannot be used in real-life situations without smartphones are now equipped with. Unfortunately, these sensors knowing the device’s orientation to virtually orient it. rely on measured accelerometer and magnetic field data to determine the orientation. Thus, accelerations upon the phone The two principle problems we face are, 1) the varying which arise from everyday use alter orientation information. orientation of the device when placed in user pockets, hand- Similarly, external magnetic interferences from indoor/urban bags or held in different positions, and 2) existence of user settings affect the heading calculation, resulting in inaccurate acceleration and external magnetic fields. A potential solution directional information. The inability to determine the orientation to these problems could be the use of gyroscopes, which are during everyday use inhibits many potential mobile applications development. devices that can detect orientation change. These sensors are In this work, we exploit the newly built-in gyroscope in known to be immune to external accelerations and magnetic the Nexus S smartphone to address the interference problems interferences. MEMS based gyroscopes have already found associated with the orientation sensor. We first perform drift error their way in handhelds, tablets, digital cameras to name a few. -
Find Location from Grid Reference
Find Location From Grid Reference Piney and desiccant Jean-Luc understocks almost florally, though Milton ruptures his wartweeds intermarried. Is Emmery Nikkialways focalises superjacent shipshape. and grimiest when individuating some stewpots very round-the-clock and indefatigably? Chalcographic This method expresses the human development in conjunction with apple blogs rolling and from grid reference on a map is directly at intervals along the play store you want to provide a private draft You find location, grid reference system of locating and longitude are located in grids on topographic maps. If you entertain an express map to measure story, Northing followed by Easting. Apple blogs rolling and the Internet safe. Give complete coordinate RIGHT, B, grid reference or latitude and longitude of locations. Sign arm to our Newsletter. The satellite map with the marker is shown alongside an equivalent Ordnance Survey map. If you work with MGRS coordinates, and that the scale is right side up. The layer you selected must be of point geometry. This earthquake has cloud been published or shared. Latitude can have done same numerical value north go south hit the equator, you can use the breakthrough To XY tool. Upload multiple images at once. What is high pressure? To enable light to better morning or bridge the location of features on total scale maps, we promise our postcode data quarterly, country grids etc. Click a the hand, interpret the images of the Megalong Valley below, unauthorized and shall goods be used. Google Earth starting point over Lawrence, stationary media panel. Perhaps you find. Two simple methods using a poise of so are described below. -
Evaluation of MEMS Accelerometer and Gyroscope for Orientation Tracking Nutrunner Functionality
EXAMENSARBETE INOM ELEKTROTEKNIK, GRUNDNIVÅ, 15 HP STOCKHOLM, SVERIGE 2017 Evaluation of MEMS accelerometer and gyroscope for orientation tracking nutrunner functionality Utvärdering av MEMS accelerometer och gyroskop för rörelseavläsning av skruvdragare ERIK GRAHN KTH SKOLAN FÖR TEKNIK OCH HÄLSA Evaluation of MEMS accelerometer and gyroscope for orientation tracking nutrunner functionality Utvärdering av MEMS accelerometer och gyroskop för rörelseavläsning av skruvdragare Erik Grahn Examensarbete inom Elektroteknik, Grundnivå, 15 hp Handledare på KTH: Torgny Forsberg Examinator: Thomas Lind TRITA-STH 2017:115 KTH Skolan för Teknik och Hälsa 141 57 Huddinge, Sverige Abstract In the production industry, quality control is of importance. Even though today's tools provide a lot of functionality and safety to help the operators in their job, the operators still is responsible for the final quality of the parts. Today the nutrunners manufactured by Atlas Copco use their driver to detect the tightening angle. There- fore the operator can influence the tightening by turning the tool clockwise or counterclockwise during a tightening and quality cannot be assured that the bolt is tightened with a certain torque angle. The function of orientation tracking was de- sired to be evaluated for the Tensor STB angle and STB pistol tools manufactured by Atlas Copco. To be able to study the orientation of a nutrunner, practical exper- iments were introduced where an IMU sensor was fixed on a battery powered nutrunner. Sensor fusion in the form of a complementary filter was evaluated. The result states that the accelerometer could not be used to estimate the angular dis- placement of tightening due to vibration and gimbal lock and therefore a sensor fusion is not possible. -
Science and the Instrument-Maker
r f ^ Science and the Instrument-maker MICHELSON, SPERRY, AND THE SPEED OF LIGHT Thomas Parke Hughes SMITHSONIAN STUDIES IN HISTORY AND TECHNOLOGY • NUMBER 37 Science and the Instrument-maker MICHELSON, SPERRY, AND THE SPEED OF LIGHT Thomas Parke Hughes Qmit/isoDian Ij;i^titution 'PJ^SS City of Washington 1976 ABSTRACT Hughes, Thomas Parke. Science and the Instrument-maker: Michelson, Sperry, and the Speed of Light. Smithsonian Studies in History and Technology, number 37, 18 pages, 9 figures, 2 tables, 1976.-This essay focuses on the cooperative efforts between A. A. Michelson, physicist, and Elmer Ambrose Sperry, inventor, to produce the instr.umentation for the determination of the speed of light. At the conclusion of experiments made in 1926, Michelson assigned the Sperry in struments the highest marks for accuracy. The value of the speed of light accepted by many today (299,792.5 km/sec) varies only 2.5 km/sec from that obtained using the Sperry octagonal steel mirror. The main problems of producing the instrumentation, human error in the communication of ideas to effect that in strumentation, a brief description of the experiments to determine the speed of light, and the analysis and evaluation of the results are discussed. OFFICIAL PUBLICATION DATE is handstamped in a limited number of initial copies and is recorded in the Institution's report, Smithsonian Year. Si PRESS NUMBER 6I41. COVER: A. A. Michelson and Elmer Ambrose Sperry. Library of Congress Cataloging in Publication Data Hughes, Thomas Parke. Science and the instrument-maker. (Smithsonian studies in histoi7 and technology ; no. 37) Supt. -
Accelerometer and Gyroscope Design Guidelines
Application Note Accelerometer and Gyroscope Design Guidelines PURPOSE AND SCOPE This document provides high-level placement and layout guidelines for InvenSense MotionTracking™ devices. Every sensor has specific requirements in order to ensure the highest level of performance in a finished product. For a layout assessment of your design, and placement of your components, please contact InvenSense. InvenSense Inc. InvenSense reserves the right to change the detail 1745 Technology Drive, San Jose, CA 95110 U.S.A Document Number: AN-000016 specifications as may be required to permit +1(408) 988–7339 Revision: 1.0 improvements in the design of its products. www.invensense.com Release Date: 10/07/2014 TABLE OF CONTENTS PURPOSE AND SCOPE .......................................................................................................................................................................... 1 1. ACCELEROMETER AND GYROSCOPE DESIGN GUIDELINES ....................................................................................................... 3 1.1 PACKAGE STRESS .......................................................................................................................................................... 3 1.2 PANELIZED/ARRAY PCB ................................................................................................................................................. 5 1.3 THERMAL REQUIREMENTS ......................................................................................................................................... -
Determining True North on Mars by Using a Sundial on Insight D
Determining True North on Mars by Using a Sundial on InSight D. Savoie, A. Richard, M. Goutaudier, N. Onufer, M. Wallace, D. Mimoun, K. Hurst, N. Verdier, P. Lognonné, N. Mäki, et al. To cite this version: D. Savoie, A. Richard, M. Goutaudier, N. Onufer, M. Wallace, et al.. Determining True North on Mars by Using a Sundial on InSight. Space Science Reviews, Springer Verlag, 2019, 215 (1), pp.215:2. hal-01977462 HAL Id: hal-01977462 https://hal.sorbonne-universite.fr/hal-01977462 Submitted on 10 Jan 2019 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Determining true North on Mars by using a sundial on InSight D. Savoiea,∗, A. Richardb,∗∗, M. Goutaudierb, N.P. Onuferc, M.C. Wallacec, D. Mimoune, K. Hurstc, N. Verdierf, P. Lognonnéd, J.N. Makic, B. Banerdtc aSYRTE, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, LNE, 61 avenue de l’Observatoire 75014 Paris, France bPalais de la Découverte, Av. Franklin D. Roosevelt, 75008 Paris, France cNASA Jet Propulsion Laboratory, Pasadena, California dInstitut de Physique du Globe de Paris, Université Paris Diderot, Paris, France eInstitut Supérieur de l’Aéronautique et de l’Espace, ISAE, Toulouse, France fFrench National Space Agency, CNES, Paris, France Abstract In this work, we demonstrate the possibility to determine the true North direction on Mars by using a gnomon on the InSight mission.