History continued: vs.
|
|
- Emily Johnson
- 7 years ago
- Views:
Transcription
1 What is Geodesy? - The Merriam Webster Dictionary defines Geodesy as, "a branch of applied mathematics concerned with the determination of the size and shape of the earth and the exact positions of points on its surface and with the description of variations of its gravity field." - so more simply, Geodesy is the study of all aspects concerning the shape, size, and movements of the Earth.
2 History: - Geodesy dates back to the earliest of civilizations Back then, people were concerned more with the immediate lands around them, not the Earth as whole as we see it today Later, it expanded to the distances from the home to the markets and other places of exchange As transportation evolved, so did the need for more exact measurements of locations. Therefore Geodesy evolved.
3 History continued: - Earliest conceptions about the world held that is was flat First ideas of a spherical Earth didn't come about until 6th century BC - What methods of observation led to the Earth being a sphere? vs.
4 Dawn of the sphere: - The first reasonings for a spherical Earth relied on astronomical observations (weird that looking into space teaches us about Earth) 1. Earth's shadow on a lunar eclipse is curved 2. Polaris (North star) lowers in the sky as one travels south 3. Pythagoris reasoned that mathematically a sphere is a more perfect shape, therefore the gods would have fashioned Earth as such
5 As science often does... - The first attempts to "measure" the size of Earth began with pure conjecture 1. Plato guessed the circumference to be between 62,800 km and 74,000 km 2. Archimedes approximated a circumference of 55,500 km - Clearly they weren't entirely accurate...
6 Increasing accuracy: - First "accurate" measurement of the Earth's circumference was done by the Greek Eratosthenes "Measured" angle of the Sun at two points during the summer solstice o o One point the sun was directly overhead (showed to the bottom of a well) Other, the sun's angle of elevation measured to be 1 / 50th of a circle
7 Eratosthenes cont: - By "knowing" the distance between the two points to be now 1/50th of the total sphere, he calculated the circumference to be ~46,620 km (not bad) - Actual circumference is a little over 40,000 km
8 Others of note: - Posidonius: calculations of 240,000 stadia and later 180,000 stadia stadia is an ancient distance measurement - Aryabhata: Indian mathematician who accurately calculated the Earth's circumference as 24,835 miles, which was only 0.2% smaller than the actual value of 24,902 miles. This approximation remained the most accurate for over a thousand years.
9 Others of note: - Biruni ( ): Persian who used many trigonometry equations (mostly triangulation) to solve many complex geodesic equations. Attained a radius value of 6,339.9 km, just shy of today's values. Used the same techniques to calculate the heights of mountains and depths of valleys
10 "Modern" additions: - The first modern update comes from the development of the meridian arc measurement First uses by Jean Picard in 1700 and later by Jacques Cassini Showed that the Earth was not a perfect sphere but more of an oblate ellipsoid of revolution
11 Video:
12 So, what next... How do we get a more accurate picture of the Earth? What techniques or technologies would help?
13 Space! - That's right! To get a more accurate picture of the ground below us, we need to look to the sky above us.
14 Space Age: - The first satellite for geodesic research was launched in 1962 "The U.S. Army developed the SECOR (Sequential Collation of Range) system and the first SECOR transponder was orbited on ANNA-1B in The system operated on the principle that an electromagnetic wave propagated through space undergoes a phase shift proportional to the distance traveled. A ground station transmitted a phase modulated signal which was received by the satellite-borne transponder and returned to the ground. The phase shift experienced by the signal during the round trip from ground to satellite and back to ground was measured electronically at the ground station which provided as its output a digitized representation of range." - o So the information they utilized from the radio waves was based on the phase, or timing of the received signals
15 Modern Geodesy: - Modern Geodesic techniques all stem from those original space efforts: 1. Global Positioning System (GPS) and Global Navigation Satellite System (GNSS) - same thing but GPS is the american version 2. Very Long Baseline Interferometry (VLBI) 3. Satellite Ranging System (SLR) 4. Satellite Altimetry (measuring ocean height and topography)
16 1.) GPS and GNSS: - A total of 32 (optimally) satellites are maintained in orbit at any time o o 31 operational satellites in orbit as of today (July 2013) Allows for a minimum signal from 4 satellites
17 GPS Background Each GPS spacecraft Carries highly accurate clock Transmits its clock and position Signals are transmitted on 2 (or 3) frequencies
18 GPS Satellite Signal Structure Code modula*on: Iden*fies SV Spread power Range X GPS signal
19
20 GPS Positioning GPS Background
21 What is GPS used to do? First there is the obvious: Used to determine exact posi*oning of objects and loca*ons on the surface of Earth Besides the obvious: Determina*on of the TEC in the ionosphere TEC = Total Electron Content Based on differing delays of different frequencies as they pass through the atmosphere Important in studying the overall effects of the Sun s ac*vi*es on Earth
22 Ionospheric Parameters GPS can be used to measure Ground-Based Receivers Total Electron Content (TEC) Scintillation Parameters: S 4 and σ Φ Space-Based Receivers Electron Density Profiles (EDP) Scintillation Parameters: S 4 and σ Φ S4= sqrt ((<I 2 > - <I> 2 )/<I> 2 ), where I is the intensity of the signal and <> is the ensemble mean. σ Φ = sqrt((<φ 2 >-<Φ> 2 ), where Φ is the phase of the signal.
23 2.) VLBI: - VLBI, Very Long Baseline Interferometry, was developed for improved resolution in radio astronomy o o Resolution of radio (and optical) images increases as a function of the aperture size By using multiple radio antennae over long distances (baselines) effectively increases the size of radio aperture
24 VLBI basics: The same radio is gathered by different antennae and each signal is matched to a highly accurate atomic clock
25 VLBI basics: Tapes are no longer used, everything is digital now Each data set is then synchronized and correlated together to achieve a much stronger measurement of the radio data gathered Nowadays, as technology has improved, larger and larger amounts of data are able to be utilized as digital recording becomes more and more efficient
26 Geodetic VLBI: - It was quickly discovered that VLBI could be used to get clearer picture of Earth as well as space By using the very accurate timing data between the antennae sites, many of Earth's motions could be more accurately tracked. What motions in particular do you think VLBI could effectively track?
27
28 VLBI's geodetic contributions: - Variations in the Earth's orientation and length of day o o clearer picture of the Earth's axial precession, nutation, and polar wandering Earth's spin is actually slowing down and the day being lengthened by ~2 ms every century
29 VLBI's geodetic contributions: - Maintenance of the terrestrial reference frame - Measurement of gravitational forces of the Sun and Moon on the Earth - Regional deformation and uplift or subsistence - And one of its greatest contribution... The first direct evidence of plate tectonic movement!
30 Plate Tectonics: - Because of VLBI's high resolution, plate motion can be measured very precisely o millimeter accuracy! - By tracking time differences of many quasars using a global system of antennae, the change in baseline distance between the antennae can be tracked and measured directly
31 Video:
32
33 3.) SLR: - SLR stands for Satellite Laser Ranging and does exactly what it sounds like SLR stations emit ultrashort pulses of light at satellites that are equipped with special reflectors This data gives extremely precise ranging measurements that can be used in a variety of ways o If you want to know more:
34 4.) Satellite Altimetry: - Measuring the topography (heights) of the oceans using dual-band altimeters on satellites o Topex/Poseidon, Jason-1 and Jason-2 - Very useful in tracking climate change in both the short term as well as long term - Objectives: - Good flash presentations:
35 Is this important? Global sea level has risen about 3 millimeters (0.1 inch) a year since Topex/ Poseidon (on the left) began its precise measurement of sea surface height in 1993 and was followed by Jason-1 in In this graph, the vertical scale represents globally averaged sea level. Seasonal variations in sea level have been removed to show the underlying trend. Image credit: University of Colorado
36 Most important detail in geodesy: - Time! For any of these techniques to work, a standard time reference needs to be used across the board o o You also need extremely accurate clocks. Accurate clocks = good correlation of data between multiple observation points - Modern UTC: commons/a/ad/ Standard_time_zones_of_the_world.png
Günter Seeber. Satellite Geodesy 2nd completely revised and extended edition
Günter Seeber Satellite Geodesy 2nd completely revised and extended edition Walter de Gruyter Berlin New York 2003 Contents Preface Abbreviations vii xvii 1 Introduction 1 1.1 Subject of Satellite Geodesy...
More informationSolar System. 1. The diagram below represents a simple geocentric model. Which object is represented by the letter X?
Solar System 1. The diagram below represents a simple geocentric model. Which object is represented by the letter X? A) Earth B) Sun C) Moon D) Polaris 2. Which object orbits Earth in both the Earth-centered
More informationUse the following information to deduce that the gravitational field strength at the surface of the Earth is approximately 10 N kg 1.
IB PHYSICS: Gravitational Forces Review 1. This question is about gravitation and ocean tides. (b) State Newton s law of universal gravitation. Use the following information to deduce that the gravitational
More informationEarth In Space Chapter 3
Earth In Space Chapter 3 Shape of the Earth Ancient Greeks Earth casts a circular shadow on the moon during a lunar eclipse Shape of the Earth Ancient Greeks Ships were observed to disappear below the
More informationExamination Space Missions and Applications I (AE2103) Faculty of Aerospace Engineering Delft University of Technology SAMPLE EXAM
Examination Space Missions and Applications I AE2103 Faculty of Aerospace Engineering Delft University of Technology SAMPLE EXAM Please read these instructions first: This are a series of multiple-choice
More informationBasic Coordinates & Seasons Student Guide
Name: Basic Coordinates & Seasons Student Guide There are three main sections to this module: terrestrial coordinates, celestial equatorial coordinates, and understanding how the ecliptic is related to
More informationMotions of Earth, Moon, and Sun
Motions of Earth, Moon, and Sun Apparent Motions of Celestial Objects An apparent motion is a motion that an object appears to make. Apparent motions can be real or illusions. When you see a person spinning
More informationMath 215 Project (25 pts) : Using Linear Algebra to solve GPS problem
Due Thursday March 1, 2012 NAME(S): Math 215 Project (25 pts) : Using Linear Algebra to solve GPS problem 0.1 Introduction The age old question, Where in the world am I? can easily be solved nowadays by
More informationProf. Ludovico Biagi. Satellite Navigation and Monitoring
Prof. Ludovico Biagi Satellite Navigation and Monitoring Navigation: trajectories control positions estimations in real time, at high frequency popular applications: low accuracy (10 m) required specific
More information2. Orbits. FER-Zagreb, Satellite communication systems 2011/12
2. Orbits Topics Orbit types Kepler and Newton laws Coverage area Influence of Earth 1 Orbit types According to inclination angle Equatorial Polar Inclinational orbit According to shape Circular orbit
More informationHow To Monitor Sea Level With Satellite Radar
Satellite Altimetry Wolfgang Bosch Deutsches Geodätisches Forschungsinstitut (DGFI), München email: bosch@dgfi.badw.de Objectives You shall recognize satellite altimetry as an operational remote sensing
More informationToday FIRST HOMEWORK DUE NEXT TIME. Seasons/Precession Recap. Phases of the Moon. Eclipses. Lunar, Solar. Ancient Astronomy
Today FIRST HOMEWORK DUE NEXT TIME Seasons/Precession Recap Phases of the Moon Eclipses Lunar, Solar Ancient Astronomy How do we mark the progression of the seasons? We define four special points: summer
More informationToday. Solstices & Equinoxes Precession Phases of the Moon Eclipses. Ancient Astronomy. Lunar, Solar FIRST HOMEWORK DUE NEXT TIME
Today Solstices & Equinoxes Precession Phases of the Moon Eclipses Lunar, Solar Ancient Astronomy FIRST HOMEWORK DUE NEXT TIME The Reason for Seasons Hypothesis check: How would seasons in the northern
More information6. The greatest atmospheric pressure occurs in the 1) troposphere 3) mesosphere 2) stratosphere 4) thermosphere
1. The best evidence of the Earth's nearly spherical shape is obtained through telescopic observations of other planets photographs of the Earth from an orbiting satellite observations of the Sun's altitude
More informationTrimble CenterPoint RTX Post-Processing Services FAQs
Trimble CenterPoint RTX Post-Processing Services FAQs What is Trimble RTX technology? 30 September 2013 Trimble RTX TM (Real Time extended) is a high-accuracy, global GNSS correction technology that combines
More informationEarth Coordinates & Grid Coordinate Systems
Earth Coordinates & Grid Coordinate Systems How do we model the earth? Datums Datums mathematically describe the surface of the Earth. Accounts for mean sea level, topography, and gravity models. Projections
More informationPost Processing Service
Post Processing Service The delay of propagation of the signal due to the ionosphere is the main source of generation of positioning errors. This problem can be bypassed using a dual-frequency receivers
More informationTropical Horticulture: Lecture 2
Lecture 2 Theory of the Tropics Earth & Solar Geometry, Celestial Mechanics The geometrical relationship between the earth and sun is responsible for the earth s climates. The two principal movements of
More informationTIDES. 1. Tides are the regular rise and fall of sea level that occurs either once a day (every 24.8 hours) or twice a day (every 12.4 hours).
TIDES What causes tides? How are tides predicted? 1. Tides are the regular rise and fall of sea level that occurs either once a day (every 24.8 hours) or twice a day (every 12.4 hours). Tides are waves
More informationCELESTIAL CLOCK - THE SUN, THE MOON, AND THE STARS
INTRODUCTION CELESTIAL CLOCK - THE SUN, THE MOON, AND THE STARS This is a scientific presentation to provide you with knowledge you can use to understand the sky above in relation to the earth. Before
More informationA long time ago, people looked
Supercool Space Tools! By Linda Hermans-Killam A long time ago, people looked into the dark night sky and wondered about the stars, meteors, comets and planets they saw. The only tools they had to study
More informationWhat causes Tides? If tidal forces were based only on mass, the Sun should have a tidegenerating
What are Tides? Tides are very long-period waves that move through the oceans as a result of the gravitational attraction of the Moon and the Sun for the water in the oceans of the Earth. Tides start in
More informationThe Earth Really is Flat! The Globe and Coordinate Systems. Long History of Mapping. The Earth is Flat. Long History of Mapping
The Earth Really is Flat! The Globe and Coordinate Systems Intro to Mapping & GIS The Earth is Flat Day to day, we live life in a flat world sun rises in east, sets in west sky is above, ground is below
More informationMeasuring the Earth Using a GPS M. Scott Wilkerson & M. Beth Wilkerson, DePauw University, May 10, 2007
Measuring the Earth Using a GPS M. Scott Wilkerson & M. Beth Wilkerson, DePauw University, May 10, 2007 Modified from: Kerski, J.J., 2007, Measuring the Earth s Circumference with GPS, Copyright ESRI,
More informationThe Celestial Sphere. Questions for Today. The Celestial Sphere 1/18/10
Lecture 3: Constellations and the Distances to the Stars Astro 2010 Prof. Tom Megeath Questions for Today How do the stars move in the sky? What causes the phases of the moon? What causes the seasons?
More informationNewton s Law of Gravity
Gravitational Potential Energy On Earth, depends on: object s mass (m) strength of gravity (g) distance object could potentially fall Gravitational Potential Energy In space, an object or gas cloud has
More informationThe Dynamic Crust 2) EVIDENCE FOR CRUSTAL MOVEMENT
The Dynamic Crust 1) Virtually everything you need to know about the interior of the earth can be found on page 10 of your reference tables. Take the time to become familiar with page 10 and everything
More information1-2. What is the name given to the path of the Sun as seen from Earth? a.) Equinox b.) Celestial equator c.) Solstice d.
Chapter 1 1-1. How long does it take the Earth to orbit the Sun? a.) one sidereal day b.) one month c.) one year X d.) one hour 1-2. What is the name given to the path of the Sun as seen from Earth? a.)
More informationFIRST GRADE 1 WEEK LESSON PLANS AND ACTIVITIES
FIRST GRADE 1 WEEK LESSON PLANS AND ACTIVITIES UNIVERSE CYCLE OVERVIEW OF FIRST GRADE UNIVERSE WEEK 1. PRE: Describing the Universe. LAB: Comparing and contrasting bodies that reflect light. POST: Exploring
More informationName Period 4 th Six Weeks Notes 2015 Weather
Name Period 4 th Six Weeks Notes 2015 Weather Radiation Convection Currents Winds Jet Streams Energy from the Sun reaches Earth as electromagnetic waves This energy fuels all life on Earth including the
More informationChapter 3 The Science of Astronomy
Chapter 3 The Science of Astronomy Days of the week were named for Sun, Moon, and visible planets. What did ancient civilizations achieve in astronomy? Daily timekeeping Tracking the seasons and calendar
More informationNewton s Law of Universal Gravitation
Newton s Law of Universal Gravitation The greatest moments in science are when two phenomena that were considered completely separate suddenly are seen as just two different versions of the same thing.
More informationCELESTIAL MOTIONS. In Charlottesville we see Polaris 38 0 above the Northern horizon. Earth. Starry Vault
CELESTIAL MOTIONS Stars appear to move counterclockwise on the surface of a huge sphere the Starry Vault, in their daily motions about Earth Polaris remains stationary. In Charlottesville we see Polaris
More informationHow To Understand General Relativity
Chapter S3 Spacetime and Gravity What are the major ideas of special relativity? Spacetime Special relativity showed that space and time are not absolute Instead they are inextricably linked in a four-dimensional
More informationGNSS permanent stations as the part of integrated geodetic system in Estonia
GNSS permanent stations as the part of integrated geodetic system in Estonia Karin Kollo (MSc) Department of Geodesy Estonian Land Board United Nations/Croatia Workshop on the applications of Global Navigation
More informationScience Standard 4 Earth in Space Grade Level Expectations
Science Standard 4 Earth in Space Grade Level Expectations Science Standard 4 Earth in Space Our Solar System is a collection of gravitationally interacting bodies that include Earth and the Moon. Universal
More informationcircular motion & gravitation physics 111N
circular motion & gravitation physics 111N uniform circular motion an object moving around a circle at a constant rate must have an acceleration always perpendicular to the velocity (else the speed would
More informationRobot Perception Continued
Robot Perception Continued 1 Visual Perception Visual Odometry Reconstruction Recognition CS 685 11 Range Sensing strategies Active range sensors Ultrasound Laser range sensor Slides adopted from Siegwart
More informationGrade 6 Standard 3 Unit Test A Astronomy. 1. The four inner planets are rocky and small. Which description best fits the next four outer planets?
Grade 6 Standard 3 Unit Test A Astronomy Multiple Choice 1. The four inner planets are rocky and small. Which description best fits the next four outer planets? A. They are also rocky and small. B. They
More informationDouglas Adams The Hitchhikers Guide to the Galaxy
There is a theory which states that if ever anybody discovers exactly what the Universe is for and why it is here, it will instantly disappear and be replaced by something even more bizarre and inexplicable.
More informationastronomy 2008 1. A planet was viewed from Earth for several hours. The diagrams below represent the appearance of the planet at four different times.
1. A planet was viewed from Earth for several hours. The diagrams below represent the appearance of the planet at four different times. 5. If the distance between the Earth and the Sun were increased,
More informationSatellite Posi+oning. Lecture 5: Satellite Orbits. Jan Johansson jan.johansson@chalmers.se Chalmers University of Technology, 2013
Lecture 5: Satellite Orbits Jan Johansson jan.johansson@chalmers.se Chalmers University of Technology, 2013 Geometry Satellite Plasma Posi+oning physics Antenna theory Geophysics Time and Frequency GNSS
More informationAS COMPETITION PAPER 2008
AS COMPETITION PAPER 28 Name School Town & County Total Mark/5 Time Allowed: One hour Attempt as many questions as you can. Write your answers on this question paper. Marks allocated for each question
More informationNon-parametric estimation of seasonal variations in GNSS-derived time series
Military University of Technology, Poland (marta.gruszczynska@wat.edu.pl) Seasonal variations in the frame sites can bias the frame realization. I would like to invite you to click on each of the four
More informationNight Sky III Planetary Motion Lunar Phases
Night Sky III Planetary Motion Lunar Phases Astronomy 1 Elementary Astronomy LA Mission College Spring F2015 Quotes & Cartoon of the Day Everything has a natural explanation. The moon is not a god, but
More informationObjectives After completing this section, you should be able to:
Chapter 5 Section 1 Lesson Angle Measure Objectives After completing this section, you should be able to: Use the most common conventions to position and measure angles on the plane. Demonstrate an understanding
More informationReasons for Seasons. Question: TRUE OR FALSE. Question: TRUE OR FALSE? What causes the seasons? What causes the seasons?
Reasons for Seasons Question: TRUE OR FALSE? Earth is closer to the Sun in summer and farther from the Sun in winter. Question: TRUE OR FALSE? Earth is closer to the Sun in summer and farther from the
More informationEDMONDS COMMUNITY COLLEGE ASTRONOMY 100 Winter Quarter 2007 Sample Test # 1
Instructor: L. M. Khandro EDMONDS COMMUNITY COLLEGE ASTRONOMY 100 Winter Quarter 2007 Sample Test # 1 1. An arc second is a measure of a. time interval between oscillations of a standard clock b. time
More informationName Class Period. F = G m 1 m 2 d 2. G =6.67 x 10-11 Nm 2 /kg 2
Gravitational Forces 13.1 Newton s Law of Universal Gravity Newton discovered that gravity is universal. Everything pulls on everything else in the universe in a way that involves only mass and distance.
More informationcompass Encyclopedic Entry
This website would like to remind you: Your browser (Apple Safari 7) is out of date. Update your browser for more security, comfort and the best experience on this site. Encyclopedic Entry compass For
More informationEvolving a new Geodetic Positioning Framework: An Australian Perspective
Evolving a new Geodetic Positioning Framework: An Australian Perspective G. Johnston, J. Dawson Outline Introduction Precise Positioning National Geospatial Reference Systems Asia Pacific Reference Frame
More informationThe Moon. Nicola Loaring, SAAO
The Moon Nicola Loaring, SAAO Vital Statistics Mean distance from Earth Orbital Period Rotational Period Diameter 384,400 km 27.322 days 27.322 days 3476 km (0.272 x Earth) Mass 7.3477 10 22 kg (0.0123
More informationPeriods of Western Astronomy. Chapter 1. Prehistoric Astronomy. Prehistoric Astronomy. The Celestial Sphere. Stonehenge. History of Astronomy
Periods of Western Astronomy Chapter 1 History of Astronomy Western astronomy divides into 4 periods Prehistoric (before 500 B.C.) Cyclical motions of Sun, Moon and stars observed Keeping time and determining
More informationName: Earth 110 Exploration of the Solar System Assignment 1: Celestial Motions and Forces Due in class Tuesday, Jan. 20, 2015
Name: Earth 110 Exploration of the Solar System Assignment 1: Celestial Motions and Forces Due in class Tuesday, Jan. 20, 2015 Why are celestial motions and forces important? They explain the world around
More informationGEOPHYSICAL EFFECTS ON SITE DISPLACEMENTS FOR PERMANENT GPS TRACKING STATIONS IN TAIWAN
GEOPHYSICAL EFFECTS ON SITE DISPLACEMENTS FOR PERMANENT GPS TRACKING STATIONS IN TAIWAN C. C. Chang Department of Surveying and Mapping Engineering Chung Cheng Institute of Technology Tahsi, Taoyuan 335,
More informationSolving the Giza Puzzle
Solving the Giza Puzzle by Johan H. Oldenkamp, Ph.D. Pateo.nl In this paper, I present facts that will change our understanding of why the Giza pyramids were built, and also when this was done. Let us
More informationCelestial Sphere. Celestial Coordinates. Lecture 3: Motions of the Sun and Moon. ecliptic (path of Sun) ecliptic (path of Sun)
Lecture 3: Motions of the and Moon ecliptic (path of ) ecliptic (path of ) The 23.5 degree tilt of Earth s spin axis relative to its orbital axis around the causes the seasons Celestial Sphere Celestial
More informationTwo primary advantages of radars: all-weather and day /night imaging
Lecture 0 Principles of active remote sensing: Radars. Objectives: 1. Radar basics. Main types of radars.. Basic antenna parameters. Required reading: G: 8.1, p.401-40 dditional/advanced reading: Online
More informationDynamics of Iain M. Banks Orbitals. Richard Kennaway. 12 October 2005
Dynamics of Iain M. Banks Orbitals Richard Kennaway 12 October 2005 Note This is a draft in progress, and as such may contain errors. Please do not cite this without permission. 1 The problem An Orbital
More information5- Minute Refresher: Daily Observable Patterns in the Sky
5- Minute Refresher: Daily Observable Patterns in the Sky Key Ideas Daily Observable Patterns in the Sky include the occurrence of day and night, the appearance of the moon, the location of shadows and
More informationSatellite Altimetry Missions
Satellite Altimetry Missions SINGAPORE SPACE SYMPOSIUM 30 TH SEPTEMBER 2015 AUTHORS: LUCA SIMONINI/ ERICK LANSARD/ JOSE M GONZALEZ www.thalesgroup.com Table of Content General Principles and Applications
More informationThursday 23 May 2013 Morning
THIS IS A NEW SPECIFICATION H Thursday 23 May 2013 Morning GCSE TWENTY FIRST CENTURY SCIENCE PHYSICS A A181/02 Modules P1 P2 P3 (Higher Tier) *A137270613* Candidates answer on the Question Paper. A calculator
More informationGRAVITY CONCEPTS. Gravity is the universal force of attraction between all matter
IT S UNIVERSAL GRAVITY CONCEPTS Gravity is the universal force of attraction between all matter Weight is a measure of the gravitational force pulling objects toward Earth Objects seem weightless when
More informationThe following words and their definitions should be addressed before completion of the reading:
Seasons Vocabulary: The following words and their definitions should be addressed before completion of the reading: sphere any round object that has a surface that is the same distance from its center
More informationScale of the Solar System. Sizes and Distances: How Big is Big? Sizes and Distances: How Big is Big? (Cont.)
Scale of the Solar System Scale of the Universe How big is Earth compared to our solar system? How far away are the stars? How big is the Milky Way Galaxy? How big is the Universe? How do our lifetimes
More informationCelestial Observations
Celestial Observations Earth experiences two basic motions: Rotation West-to-East spinning of Earth on its axis (v rot = 1770 km/hr) (v rot Revolution orbit of Earth around the Sun (v orb = 108,000 km/hr)
More informationFrom Aristotle to Newton
From Aristotle to Newton The history of the Solar System (and the universe to some extent) from ancient Greek times through to the beginnings of modern physics. The Geocentric Model Ancient Greek astronomers
More informationNote S1: Eclipses & Predictions
The Moon's Orbit The first part of this note gives reference information and definitions about eclipses [14], much of which would have been familiar to ancient Greek astronomers, though not necessarily
More informationSURVEYING WITH GPS. GPS has become a standard surveying technique in most surveying practices
SURVEYING WITH GPS Key Words: Static, Fast-static, Kinematic, Pseudo- Kinematic, Real-time kinematic, Receiver Initialization, On The Fly (OTF), Baselines, Redundant baselines, Base Receiver, Rover GPS
More informationStellarium a valuable resource for teaching astronomy in the classroom and beyond
Stellarium 1 Stellarium a valuable resource for teaching astronomy in the classroom and beyond Stephen Hughes Department of Physical and Chemical Sciences, Queensland University of Technology, Gardens
More informationModule 13 : Measurements on Fiber Optic Systems
Module 13 : Measurements on Fiber Optic Systems Lecture : Measurements on Fiber Optic Systems Objectives In this lecture you will learn the following Measurements on Fiber Optic Systems Attenuation (Loss)
More informationEducator Guide to S LAR SYSTEM. 1875 El Prado, San Diego CA 92101 (619) 238-1233 www.rhfleet.org
Educator Guide to S LAR SYSTEM 1875 El Prado, San Diego CA 92101 (619) 238-1233 www.rhfleet.org Pre-Visit Activity: Orbital Paths Materials: Plastic Plate Marble Scissors To Do: 1. Put the plate on a flat
More information1. In the diagram below, the direct rays of the Sun are striking the Earth's surface at 23 º N. What is the date shown in the diagram?
1. In the diagram below, the direct rays of the Sun are striking the Earth's surface at 23 º N. What is the date shown in the diagram? 5. During how many days of a calendar year is the Sun directly overhead
More informationWeek 1-2: Overview of the Universe & the View from the Earth
Week 1-2: Overview of the Universe & the View from the Earth Hassen M. Yesuf (hyesuf@ucsc.edu) September 29, 2011 1 Lecture summary Protein molecules, the building blocks of a living organism, are made
More informationCDMA Technology : Pr. S. Flament www.greyc.fr/user/99. Pr. Dr. W. sk www.htwg-konstanz.de. On line Course on CDMA Technology
CDMA Technology : Pr. Dr. W. sk www.htwg-konstanz.de Pr. S. Flament www.greyc.fr/user/99 On line Course on CDMA Technology CDMA Technology : CDMA / DS : Principle of operation Generation of PN Spreading
More informationLocal Sidereal Time is the hour angle of the First Point of Aries, and is equal to the hour angle plus right ascension of any star.
1 CHAPTER 7 TIME In this chapter we briefly discuss the several time scales that are in use in astronomy, such as Universal Time, Mean Solar Time, Ephemeris Time, Terrestrial Dynamical Time, and the several
More informationMEASUREMENT. Historical records indicate that the first units of length were based on people s hands, feet and arms. The measurements were:
MEASUREMENT Introduction: People created systems of measurement to address practical problems such as finding the distance between two places, finding the length, width or height of a building, finding
More informationGravitational potential
Gravitational potential Let s assume: A particle of unit mass moving freely A body of mass M The particle is attracted by M and moves toward it by a small quantity dr. This displacement is the result of
More informationEarth-Sun Relationships. The Reasons for the Seasons
Earth-Sun Relationships The Reasons for the Seasons Solar Radiation The earth intercepts less than one two-billionth of the energy given off by the sun. However, the radiation is sufficient to provide
More informationSatellite Derived Dynamic Ocean Currents in the Arctic. Jens Olaf Pepke Pedersen Polar DTU / DTU Space www.polar.dtu.dk www.space.dtu.
Satellite Derived Dynamic Ocean Currents in the Arctic Jens Olaf Pepke Pedersen Polar DTU / DTU Space www.polar.dtu.dk www.space.dtu.dk Benefits of exploiting ocean currents Benjamin Franklins map of the
More informationThe Next Generation Science Standards (NGSS) Correlation to. EarthComm, Second Edition. Project-Based Space and Earth System Science
The Next Generation Science Standards (NGSS) Achieve, Inc. on behalf of the twenty-six states and partners that collaborated on the NGSS Copyright 2013 Achieve, Inc. All rights reserved. Correlation to,
More informationInteraction of Energy and Matter Gravity Measurement: Using Doppler Shifts to Measure Mass Concentration TEACHER GUIDE
Interaction of Energy and Matter Gravity Measurement: Using Doppler Shifts to Measure Mass Concentration TEACHER GUIDE EMR and the Dawn Mission Electromagnetic radiation (EMR) will play a major role in
More informationFor further information, and additional background on the American Meteorological Society s Education Program, please contact:
Project ATMOSPHERE This guide is one of a series produced by Project ATMOSPHERE, an initiative of the American Meteorological Society. Project ATMOSPHERE has created and trained a network of resource agents
More informationBasic Principles of Inertial Navigation. Seminar on inertial navigation systems Tampere University of Technology
Basic Principles of Inertial Navigation Seminar on inertial navigation systems Tampere University of Technology 1 The five basic forms of navigation Pilotage, which essentially relies on recognizing landmarks
More informationAstronomy 110 Homework #04 Assigned: 02/06/2007 Due: 02/13/2007. Name:
Astronomy 110 Homework #04 Assigned: 02/06/2007 Due: 02/13/2007 Name: Directions: Listed below are twenty (20) multiple-choice questions based on the material covered by the lectures this past week. Choose
More informationProduced by Billy Hix and Terry Sue Fanning. As part of the TeachSpace Program. For more ideas and an image of the current phase of the moon, visit:
The Moon Phase Book Produced by Billy Hix and Terry Sue Fanning As part of the TeachSpace Program For more ideas and an image of the current phase of the moon, visit: www.teachspace.us Printing Date: 10/29/2010
More informationEssential Question. Enduring Understanding
Earth In Space Unit Diagnostic Assessment: Students complete a questionnaire answering questions about their ideas concerning a day, year, the seasons and moon phases: My Ideas About A Day, Year, Seasons
More informationAntennas & Propagation. CS 6710 Spring 2010 Rajmohan Rajaraman
Antennas & Propagation CS 6710 Spring 2010 Rajmohan Rajaraman Introduction An antenna is an electrical conductor or system of conductors o Transmission - radiates electromagnetic energy into space o Reception
More informationSTUDY GUIDE: Earth Sun Moon
The Universe is thought to consist of trillions of galaxies. Our galaxy, the Milky Way, has billions of stars. One of those stars is our Sun. Our solar system consists of the Sun at the center, and all
More informationOrigins of the Cosmos Summer 2016. Pre-course assessment
Origins of the Cosmos Summer 2016 Pre-course assessment In order to grant two graduate credits for the workshop, we do require you to spend some hours before arriving at Penn State. We encourage all of
More informationArtificial Satellites Earth & Sky
Artificial Satellites Earth & Sky Name: Introduction In this lab, you will have the opportunity to find out when satellites may be visible from the RPI campus, and if any are visible during the activity,
More informationOptical Standards. John Nichol BSc MSc
Optical Standards John Nichol BSc MSc The following notes are presented to explain: Spherical Aberration The Airy Disk Peak to Valley, RMS and Strehl Ratio Standards of Optics produced by Nichol Optical
More informationCHAPTER 2 Energy and Earth
CHAPTER 2 Energy and Earth This chapter is concerned with the nature of energy and how it interacts with Earth. At this stage we are looking at energy in an abstract form though relate it to how it affect
More informationCurriculum Map Earth Science - High School
September Science is a format process to use Use instruments to measure Measurement labs - mass, volume, to observe, classify, and analyze the observable properties. density environment. Use lab equipment
More informationCase Study Australia. Dr John Dawson A/g Branch Head Geodesy and Seismic Monitoring Geoscience Australia. Chair UN-GGIM-AP WG1 Chair APREF.
Case Study Australia Dr John Dawson A/g Branch Head Geodesy and Seismic Monitoring Geoscience Australia Chair UN-GGIM-AP WG1 Chair APREF Page 1 Overview 1. Australian height system Australian Height Datum
More informationCalifornia Standards Grades 9 12 Boardworks 2009 Science Contents Standards Mapping
California Standards Grades 912 Boardworks 2009 Science Contents Standards Mapping Earth Sciences Earth s Place in the Universe 1. Astronomy and planetary exploration reveal the solar system s structure,
More informationThe Four Seasons. A Warm Up Exercise. A Warm Up Exercise. A Warm Up Exercise. The Moon s Phases
The Four Seasons A Warm Up Exercise What fraction of the Moon s surface is illuminated by the Sun (except during a lunar eclipse)? a) Between zero and one-half b) The whole surface c) Always half d) Depends
More informationMaybe you know about the Energy House.
Plans and experiments for the Energy House can be found at Design Coalition s website at www.designcoalition.org Maybe you know about the Energy House. Here are some more ideas for leaning about the sun
More informationChapter 3 Earth - Sun Relations
3.1 Introduction We saw in the last chapter that the short wave radiation from the sun passes through the atmosphere and heats the earth, which in turn radiates energy in the infrared portion of the electromagnetic
More informationGlobal Positioning System
B. Hofmann-Wellenhof, H. Lichtenegger, and J. Collins Global Positioning System Theory and Practice Third, revised edition Springer-Verlag Wien New York Contents Abbreviations Numerical constants xix xxiii
More information