Islamic University of Gaza Civil Engineering Department Surveying II ECIV 2332

Similar documents
Chapter-2 Direct Measurement Indirect Measurement Method of linear measurement Taping corrections Optical measurement Tachometry EDM Measurement

INTRODUCTION TO ENGINEERING SURVEYING (CE 1305)

Measurement of Distance and Elevation Equipment and Procedures

Surveying Prof. Bharat Lohani Department of Civil Engineering Indian Institute of Technology, Kanpur. Module - 3 Lecture - 4 Linear Measurements

Chapter 5 Telescopes

Fig. 8.1 illustrates the three measurements. air medium A. ray 1. air medium A. ray 2. air medium A. ray 3. Fig For Examiner s Use

UNCERTAINTY IN TACHEOMETRIC MEASUREMENT OF CONVERGENCES IN TUNNELS

Wavelength (λ)- Frequency (ν)- Which of the following has a higher frequency?

Space Physics Questions CfE

Leveling. 3.1 Definitions

Figure 1 shows white light passing through a triangular glass prism. The white light splits up into different colours. Two of the colours are shown.

0.4 s 0.8 s 1.5 s. 2.5 s. 2. A beam of light from a ray box spreads out as shown in the diagram and strikes a plane mirror.

The generation of terahertz frequency radiation by optical rectification

GEOMATICS ENGINEERING

Interferometer for Squareness measurement

Determination of Cauchy s Contants

Measurement of Horizontal Distances. the distance between two points means the horizontal distance

Lecture Outlines. Chapter 5. Astronomy Today 8th Edition Chaisson/McMillan Pearson Education, Inc.

UNIT-5 EM WAVES UNIT-6 RAY OPTICS

UNIT 1- CONTROL SURVEYING PART A

Experiment O-2. The Michelson Interferometer

Unit 5 Lesson 1 Images from Space. Copyright Houghton Mifflin Harcourt Publishing Company

Physics and the Quantum Mechanical Model

5.3. Physics and the Quantum Mechanical Model

CE6404 SURVEYING II. 3. Arbitrary Bench Mark: When the RL of some fixed Points are assumed, they are termed a arbitrary Bench mark

Chapter 3 Telescopes 2/19/2014. Lecture Outline. 3.1 Optical Telescopes. 3.1 Optical Telescopes. Units of Chapter Optical Telescopes

Basic Field Instruments Field Orientation, Basic Navigation ESRM 304

Because light behaves like a wave, we can describe it in one of two ways by its wavelength or by its frequency.

Astronomy A BEGINNER S GUIDE TO THE UNIVERSE EIGHTH EDITION

Chapter 6 Light and Telescopes

Astronomical Tools. Optics Telescope Design Optical Telescopes Radio Telescopes Infrared Telescopes X Ray Telescopes Gamma Ray Telescopes

Grade 8 Science: Unit 3-Optics Chapter 4: Properties of Light

Do Now: Bohr Diagram, Lewis Structures, Valence Electrons 1. What is the maximum number of electrons you can fit in each shell?

FOCUS 30/FOCUS 35 Field Calibration with Survey Pro Field Software


Class XII Chapter 8 Electromagnetic Waves Physics

PhysicsAndMathsTutor.com 1

Optics and Telescopes

Name Class Date. For each pair of terms, explain how the meanings of the terms differ.

DETERMINATION OF AIR REFRACTION INFLUENCE ON TRIGONOMETRIC HEIGHT DIFFERENCES

ABOUT SPOTTINGSCOPES Background on Telescopes

Foundations of Astronomy 13e Seeds. Chapter 6. Light and Telescopes

Exam 3--Sp 08. Name: Class: Date: Multiple Choice Identify the choice that best completes the statement or answers the question.

CHENDU COLLEGE OF ENGINEERING & TECHNOLOGY DEPARTMENT OF CIVIL ENGINEERING SUB CODE & SUB NAME : CE6404 SURVEYING II

Optics and Telescope. Chapter Six

Grade 8 Science Unit 2: Optics Chapters 4, 5 and 6

Tutorials. 1. Autocollimator. Angle Dekkor. General

LECTURE 11 ELECTROMAGNETIC WAVES & POLARIZATION. Instructor: Kazumi Tolich

CHEM6416 Theory of Molecular Spectroscopy 2013Jan Spectroscopy frequency dependence of the interaction of light with matter

Astronomy. Optics and Telescopes

NAT 5 - Waves and Radiation Powerpoint Answers

Lecture 14: Non-Optical Telescopes. Resolving Power. When light enters a telescope, it is bent slightly:

ELECTROMAGNETIC WAVES

Experiment 24: Spectroscopy

Write the electron configuration for Chromium (Cr):

Model 556X User s Manual. Optical Isolator

The Grating Spectrometer and Atomic Spectra

How Light Beams Behave. Light and Telescopes Guiding Questions. Telescopes A refracting telescope uses a lens to concentrate incoming light at a focus

The Secret Behind the Nobeyama 45-m Radio Telescope s Excellent

-I g in y e SURVEYING-I rv u S

E. K. A. ADVANCED PHYSICS LABORATORY PHYSICS 3081, 4051 FRAUNHOFER DIFFRACTION

DIFFRACTION GRATING. OBJECTIVE: To use the diffraction grating in the formation of spectra and in the measurement of wavelengths.

Some Topics in Optics

DOWNLOAD PDF PLANE AND GEODETIC SURVEYING FOR ENGINEERS

Total station LEICA TPS

SNC2D PHYSICS 4/27/2013. LIGHT & GEOMETRIC OPTICS L What Is Light? (P ) What Is Light? What Is Light?

Chapter 5 Electrons In Atoms

Phys 100 Astronomy (Dr. Ilias Fernini) Review Questions for Chapter 5

-SQA-SCOTTISH QUALIFICATIONS AUTHORITY NATIONAL CERTIFICATE MODULE: UNIT SPECIFICATION GENERAL INFORMATION. -Module Number Session

Electromagnetic Waves

Optical Telescopes. Telescopes. Refracting/Reflecting Telescopes. Physics 113 Goderya

Universe. Chapter 6. Optics and Telescopes 8/12/2015. By reading this chapter, you will learn. Tenth Edition

The well-composed image was recorded over a period of nearly 2 hours as a series of 30 second long, consecutive exposures on the night of October 5.

Crave the Wave! Your score will be based on your work (which you will show below) and not just the final answer.

Solution 3: A glass prism deviates the violet light most and the red light least.

Area 1: Space Exploration and Cosmology. 2. The weather information satellite NOAA-15 has a period of 99 minutes and an orbital height of 833 km.

Physics 30: Chapter 5 Exam Wave Nature of Light

DAY LABORATORY EXERCISE #5: PARALLAX & TRIANGULATION

Atomic emission spectra experiment

1) Introduction 2) Photo electric effect 3) Dual nature of matter 4) Bohr s atom model 5) LASERS

Obtain an optical "bench" setup (there should be three sliding mounts on the calibrated horizontal bar. The setup is shown in the diagram below.

Alignment-Aspects for the HERA-Experiments ZEUS and H1

1) What do all waves transport from one place to another?

Astro 1010 Planetary Astronomy Sample Questions for Exam 3

Package No.-36(Surveyor) Annexure -III

Lecture 7. Outline. ASTR 111 Section 002. Discuss Quiz 5 Light. Light travels through empty space at a speed of 300,000 km/s

Trigonometric Ratios of Acute Angles. Evaluate reciprocal trigonometric ratios. LEARN ABOUT the Math. In ^MNP, determine the length of MN.

PHYS 160 Astronomy Test #2 Fall 2017 Version A

Dispersion and resolving power of the prism and grating spectroscope (Item No.: P )

LECTURE 11 ELECTROMAGNETIC WAVES & POLARIZATION. Instructor: Kazumi Tolich

SPECTRUM. Dispersion. This phenomenon can be observed in a lab environment using a

: SINE, COSINE, & TANGENT RATIOS

Light and Telescope 10/22/2018. PHYS 1403 Introduction to Astronomy. Reminder/Announcement. Chapter Outline. Chapter Outline (continued)

Universe. Chapter 6. Optics and Telescopes 11/16/2014. By reading this chapter, you will learn. Tenth Edition

Investigation 3: Predicting Eruptions

Site Surveying Procedures for Construction and the Built Environment

Math 2 Trigonometry. People often use the acronym SOHCAHTOA to help remember which is which. In the triangle below: = 15

The Treptow Giant Telescope in Berlin is the longest moveable refracting telescope on Earth. Some of its properties are summarised below:

BLUE-PRINT II XII Physics

Physics I Keystone Institute Technology & Management Unit-II

Transcription:

Islamic University of Gaza Civil Engineering Department Surveying II ECIV 2332 By Belal Almassri

Chapter 6 Electronic Distance Measurement EDM - Introduction. - Electro-Optical Instrument. - Microwave Instrument. - Types of Mounts. - Operating Procedure. - Trigonometric Levelling. - Corrections and Examples.

Introduction Definition: A surveying instrument that utilizes an infrared or laser beam to measure the distance from the source point to a defined target point. Main Types: 1. Electro-Optical Instruments: Use the light and infrared waves. 2. Microwave Instruments: Use the radio waves.

Electro-optical Instruments Use the velocity of light waves to determine the distance between two points. Those instruments use both the visible lights (wavelength between 0.4-0.7) and the infrared lights (wavelength between 0.7-1.2). Infrared light much preferable because of the long wavelength. Source of light: Mercury lambs, Tungsten.

Electro-optical Principle S = Slope Distance. V = Velocity of Light. T = Travel Time.

Microwave Instruments Wave length λ = distance travelled during the period of one cycle. V = Velocity of emission F = Frequency in HZ

Disadvantages of Microwave Type Two operators are needed to measure a line. Sometimes there is difficulty to set up two units on both sides. The accuracy is affected by the atmosphere. Less accuracy than the electro-optical type.

Types of Mounts In General the EDM can be mounted alone or with another surveying tool, the most popular types as follows: Separate unit for (20-60 km). On top of standards of theodolite. On top of telescope of theodolite. Integral part of Total Station.

Retro Reflectors The reflectors used with the electrooptical type are called the retro-reflector using precise prisms which can be single or multiple. The max distance of measurement of EDM device depends on: The design, The quality and number of prisms, The atmospheric conditions.

Operating Procedure Set up the instrument over the survey station and record its height HI and set up the reflector on the other side. Point the instrument toward the reflector using the telescope. Adjust the pointing of tangents using the screws of the instrument. Read and record the Temperature, ATM pressure then press the correction button. Press measure and record the reading.

Corrections for zero centering The constant error appears in all distances measured by the combination of instrument and reflector. If AB is the measured distance between two points and so AC, CB The corrected AB = AB + c (correction) c = AB AC CB

Correction for frequency g = f / f f : measured frequency. f : theoretical frequency. AB (corrected) = g. AB (actual) + c Example 6.1 + 6.2

Trigonometric Levelling Short Line Def: It is the process of determining the height difference between two points using the measured distances and vertical angles.

Δh = h B h A = s.cosz + i t Terms: S=Slope Distance, z=vertical Angle. i=the height of the instrument. t=the height of the sight target. Example 6.6

In case of EDM mounted on top of the standards of the theodolite, the measured slope distance may not coincide with the line of sight in the angular measurement. So the following procedure is followed at that case: 1. Find the angle difference Δz. Δz = 180(HI-i+t-HT)sinz Π. S 2. Find the corrected angle Z =Z+ Δz 3. Find the height difference ΔH = H B -H A = S.cos Z + HI - HT

Where HI and HT = Height measurement of the instrument and the reflector of the EDM device. Example 6.7 Example 6.8

Extra Practice! EDM has slope distance AB of 561.276 m. EDM instrument is 1.820 m above station A, and the prism is 1.986 m above station B. The EDM is mounted on a theodolite whose optical center is 1.720 m above the station. The theodolite measured a vertical angle of +6º 21 38 to target on prism pole; the target is 1.810 m above station B. Compute both the horizontal distance AB and elevation of station B given an elevation at A of 186.275 m.

Solution!