1 SVY 207: Lecture 12 Modes of GPS Positioning Aim of this lecture: –To review and compare methods of static positioning, and introduce methods for kinematic.

Slides:



Advertisements
Similar presentations
GPS Theory and applications
Advertisements

2013 Western Australia Surveying Conference
June 12-14, 2013, Ottawa, Canada From dual- to triple-frequency PPP: method, problems and application in California Jianghui Geng, Yehuda Bock Scripps.
A quick GPS Primer (assumed knowledge on the course!) Observables Error sources Analysis approaches Ambiguities If only it were this easy…
Limits of static processing in a dynamic environment Matt King, Newcastle University, UK.
Space Weather influence on satellite based navigation and precise positioning R. Warnant, S. Lejeune, M. Bavier Royal Observatory of Belgium Avenue Circulaire,
Navigational System For An Autonomouse Farming Vehicle Group 942.
GTECH 201 Session 08 GPS.
Differential and precision GPS surveying for sub-meter and centimeter accuracy Feb 2007 Dr. Gary Oppliger.
Ground-Based Altimetry Using a Single- Receiver Single-Frequency GNSS Phase Ambiguity Resolution Technique G. Stienne* S. Reboul J.-B. Choquel M. Benjelloun.
GPS Receivers: Basics and Selection T.S. Stombaugh, J.D. Luck and S.A. Shearer Biosystems and Agricultural Engineering University of Kentucky.
EE 570: Location and Navigation: Theory & Practice The Global Positioning System (GPS) Thursday 11 April 2013 NMT EE 570: Location and Navigation: Theory.
13/06/13 H. Rho Slide 1 Geodetic Research Laboratory Department of Geodesy and Geomatics Engineering University of New Brunswick Evaluation of Precise.
How Global Positioning Devices (GPS) work
Planning for airborne LIDAR survey Dr.Lamyaa Gamal El-deen.
SVY 207: Lecture 4 GPS Description and Signal Structure
Mission Planning and SP1. Outline of Session n Standards n Errors n Planning n Network Design n Adjustment.
Part VI Precise Point Positioning Supported by Local Ionospheric Modeling GS894G.
What is GPS??? GPS is short for Global Positioning System
Modern Navigation Thomas Herring MW 11:00-12:30 Room A
NGS GPS ORBIT DETERMINATION Positioning America for the Future NATIONAL OCEANIC AND ATMOSPHERIC ADMINISTRATION National Ocean Service National Geodetic.
VRS Network The Magic Behind the Scene
GPS: Global Positioning System  The Geographer’s best friend!  You can say with confidence… “I’m not lost!, I’m never lost!”* *Of course, where everybody.
C-Nav GPS System GPS Services Group
How Does GPS Work ?. Objectives To Describe: The 3 components of the Global Positioning System How position is obtaining from a radio timing signal Obtaining.
Part Va Centimeter-Level Instantaneous Long-Range RTK: Methodology, Algorithms and Application GS894G.
Part V Centimeter-Level Instantaneous Long-Range RTK: Methodology, Algorithms and Application GS894G.
Lecturer: Jinglin Wang Student name: Hao Li Student ID:
Global Positioning System
1 SVY 207: Lecture 11 GPS Error Sources: Review Where can errors occur? –Satellite: ephemeris, clock, S/A (history) A/S –Propagation: ionosphere, troposphere,
SVY 207: Lecture 13 Ambiguity Resolution
West Hills College Farm of the Future. West Hills College Farm of the Future GLONASS Russia’s global satellite navigation system 24 satellites in three.
Geodetic Research Laboratory Department of Geodesy and Geomatics Engineering University of New Brunswick 01/06/27 S.Bisnath A NEW TECHNIQUE FOR GPS-BASED.
1 SVY 207: Lecture 14 Instruments and Applications Aim of this lecture: –To learn GPS specifications appropriate to different applications Short lecture.
Surveying with the Global Positioning System Phase Observable.
P. Wielgosz and A. Krankowski IGS AC Workshop Miami Beach, June 2-6, 2008 University of Warmia and Mazury in Olsztyn, Poland
A Geodesist’s View of the Ionosphere Gerald L. Mader National Geodetic Survey Silver Spring, MD.
CRGIS Global Positioning Systems The Basics CRGIS National Park Service.
Airborne GPS Positioning with cm-Level Precisions at Hundreds of km Ranges Gerald L. Mader National Geodetic Survey Silver Spring, MD National Geodetic.
GSI Japan - 21st of June 1999 GPS-Positioning using Virtual Reference Stations - Theory, Analysis and Applications Herbert Landau Spectra Precision Terrasat.
GALOCAD GAlileo LOcal Component for nowcasting and forecasting Atmospheric Disturbances R. Warnant*, G. Wautelet*, S. Lejeune*, H. Brenot*, J. Spits*,
GRIM & DynaPos Overview, Examples and Results Dr. Benjamin Remondi Kendall The XYZs' of GPS,
SVY 207: Lecture 7 Differential GPS By now you should understand: –How GPS point positioning works from first principles Aim of this lecture: –To understand.
1 SVY 207: Lecture 12 GPS Error Sources: Part 2 –Satellite: ephemeris, clock, S/A, and A/S –Propagation: ionosphere, troposphere, multipath –Receiver:antenna,
Lecture 5 – Differential Correction
Global Positioning System Overview
The Global Positioning System. Early Satellite Systems Satellite Surveying started more than 30 years ago. Now, High accuracy could be achieved in real.
Presented by: Technical contributions from: THE INTERNATIONAL ASSOCIATION OF GEODESY AND PRECISE POINT POSITIONING.
EE 495 Modern Navigation Systems
Global Positioning System Student : Min-Yin Huang Hong-Wei Du Teacher : Ru-Li Lin Department of Mechanical Engineering Southern Taiwan.
Pseudoranges to Four Satellites
SVY 207: Lecture 15 Instruments and Applications
Civil and Environmental Engineering and Geodetic Science This file can be found on the course web page:
Principles of the Global Positioning System Lecture 09 Prof. Thomas Herring Room A;
Using Real-time Networks in the Northeast
SVY207: Lecture 10 Computation of Relative Position from Carrier Phase u Observation Equation u Linear dependence of observations u Baseline solution –Weighted.
USM RTK Workshop Fugro Chance Inc. Starfix HP: High Performance GPS For Offshore Marine Survey, Navigation and Positioning Richard Barker, Dr. Dariusz.
GALOCAD GAlileo LOcal Component for nowcasting and forecasting Atmospheric Disturbances R. Warnant, G. Wautelet, S. Lejeune, H. Brenot, J. Spits, S. Stankov.
Relative positioning with Galileo E5 AltBOC code measurements DEPREZ Cécile Dissertation submitted to the University of Liège in partial requirements for.
Revised 10/30/20061 Overview of GPS FORT 130 Forest Mapping Systems.
SVY207 Lecture 8: The Carrier Phase Observable
AXK/JPL SBAS Training at Stanford University, October 27-30, 2003 Satellite Based Augmentation Systems Brazilian Ionosphere Group Training at Stanford.
Limits of static processing in a dynamic environment Matt King, Newcastle University, UK.
09/24/2008Unavco Track Intro1 TRACK: GAMIT Kinematic GPS processing module R King overview from longer T Herring.
Limits of static processing in a dynamic environment Matt King, Newcastle University, UK.
GPS: Global Positioning System
Appliance of IceCORS network 2017 by Dalia Prizginiene
SVY207: Lecture 16 GPS Field Procedures and Computations
KINEMATIC GPS AND AMBIGUITY RESOLUTION PROBLEM
Presentation transcript:

1 SVY 207: Lecture 12 Modes of GPS Positioning Aim of this lecture: –To review and compare methods of static positioning, and introduce methods for kinematic positioning. Overview –Point positioning –Differential positioning –Relative positioning –Static versus kinematic positioning –Precise kinematic positioning

2 Point Positioning Procedure –Single receiver, pseudoranges from  4 satellites –Use satellite ephemerides to compute for each satellite: »3 satellite coordinates and 1 clock bias –Estimate using least squares »3 station coordinates and 1 receiver clock bias Real-time point positioning –Broadcast Ephemerides from Navigation Message »Coordinate system: WGS-84 –Typical precision to around metres, NO S/A –Can average many single point positions to get better position metres »For best precision, software should attempt to model ionospheric and tropospheric delay »Navigation message also contains ionospheric parameters for single-frequency users (few m errors)

3 Precise Point Positioning Precise point positioning (post-processed) –Precise orbits (IGS, NGS, JPL) and satellite clocks together with GIPSY-OASIS II software. »Eliminates S/A: sub-metre positioning possible »Ionosphere: use dual-frequency data combination »Troposphere: modelled »Multipath: reasonable environment + chokering antenna »Estimated parameters: 3 receiver coordinates, 1 receiver clock, 1 troposphere (at zenith), and 1 carrier phase bias for each satellite –Using dual frequency carrier phase and pseudorange for few hours allows for sub-decimetre precision. –Greater than around 8 hours data yields 1cm precision –Full observable model - our model v. basic.

4 Differential positioning (DGPS) –Procedure Base station(s) tracking  4 satellites, computes and transmits “pseudorange corrections” Mobile receiver(s), corrects pseudoranges for  4 satellites Use broadcast ephemerides for orbits and sat. clocks Estimate using least squares, station position and clock –Real-time differential positioning Typical precision 1 to 7 metres S/A, satellite errors, and propagation errors mitigated by this procedure Errors grow with distance from base station (e.g., ionosphere, troposphere) Errors due to “age of correction” (several seconds) Errors from pseudorange multipath, measurement error Receiver can transform WGS-84 into national systems

5 Precise Relative positioning –Procedure 2 stations (baseline), or multiple stations (network) Carrier phases from  4 satellites, then double-difference Use broadcast or precise satellite orbits and clocks Assume values for one station and its clock time –e.g., use point position, or control point (WGS-84) Estimate, using weighted least squares, station coordinates, and carrier phase ambiguities Fix ambiguities to integer values and iterate. –Post-processed relative positioning Achievable precision: < 1 cm –over few  10 km using broadcast orbits –over all distances using IGS orbits Accuracy depends on hardware and software –dual frequency data, modelling capability, etc... Base Rover

6 “Static” versus “Kinematic” Positioning Static Positioning –Stationary receivers –Use all data to estimate each station position as a constant –Can use any method described previously »Obviously precisions will depend on method Kinematic Positioning –Mobile receivers –GPS positioning computation is identical to static problem –Solve for position at every epoch (e.g., 1 per second) »Can just use current data (at that epoch) »Can also use Kalman filter (= weighted average of position using current data + predicted position) »GPS can be integrated with other data types (gyrocompass, odometer, accelerometer, map info..)

7 Precise Kinematic Positioning Basic Idea –Use “relative positioning” to a base station  L      N –Double differenced carrier phase data,  L –Important: ambiguities  N must be known –“Initialisation” is the problem of finding  N in advance –If can initialise then difference between to epochs, collected by same receiver to same satellite = change in topocentric range i.e.,  L ’  (  L    N)   –Can be done in real time if there is a radio link Real Time Kinematic GPS (RTK)

8 Real Time Kinematic GPS (RTK) “RTK GPS” similar to “Differential GPS” »Both use radio transmissions from a base station (previous slide) “Differential GPS”  pseudorange corrections “RTK GPS”  dual frequency phase data, L »RTK requires FM radio link Higher data rate required than for differential GPS (10 hz-1 sec) Limit on radio transmitter power due to legal restrictions UK 0.5Watt Short range (15 km) Generally line of sight works best »RTK must find correct values for  N More difficult if receiver is moving “On the fly” ambiguity resolution Range limited by effect of ionosphere on finding  N Department has Leica’s RTK system 530 –530 receivers plus radio link and hand held controller

9 Initialisation Methods Method 1: Static –First do static positioning until  N are all resolved  L      N> 15 min (?) Method 2: Known points –First place 2 receivers at known coordinates –Solve for  N:  L      N instantaneous but not efficient/convenient Method 3: Antenna swap –Quickly swap 2 antennas between 2 fixed points, A and B –Solve for  N Before swap:  L AB   AB    N After swap:  L BA   BA    N  AB    N (1) + (2):  L AB (1)  L BA (2)   2   N

10 Initialisation Methods Method 4: On-The-Fly (OTF) –Several techniques »Extra-wide-laning »Ambiguity-mapping function »Least-squares ambiguity searching »Kalman Filter techniques Identify correct integer ambiguities (Perform integer search) Initialise RTK solution (fixed solution) Estimate initial position Verify correct intialisatoin

11 Types of “Kinematic” Positioning True Kinematic –Use all data that is recorded on the move –Use sophisticated ambiguity resolution technique (OTF) –Real time OR post processed –Preferred method today Historic methods(largely)! –Semi-Kinematic (“Stop and Go”) »While tracking, stop at various fixed points »Need to keep lock on signal at all times »OR correct for cycle slips (additional sensors may help) –Pseudo-Kinematic »Revisit fixed points within 1 hour »No need to use data while on the move