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Localization with GPS Localization with GPS From GPS Theory and Practice Fifth Edition Presented by Martin Constantine Introduction w GPS = Global Positioning System w Three segments: 1. Space (24 satellites) 2. Control (DOD) 3. User


  1. Localization with GPS Localization with GPS From GPS Theory and Practice Fifth Edition Presented by Martin Constantine

  2. Introduction w GPS = Global Positioning System w Three segments: 1. Space (24 satellites) 2. Control (DOD) 3. User (civilian and military receivers)

  3. GPS Overview w Satellites transmit L1 and L2 signals w L1--two pseudorandom noise signals – Protected (P-)code – Course acquisition (C/A) code (most civilian receivers) w L2--P-code only w Anti-spoofing adds noise to the P-code, resulting in Y-code

  4. Observables w Code pseudoranges

  5. Observables w Phase pseudoranges – N = number of cycles between satellite and receiver

  6. Observables w Doppler Data – Dots indicate derivatives wrt time.

  7. Observables w Biases and Noise

  8. Combining Observables w Generally w Linear combinations with integers w Linear combinations with real numbers w Smoothing

  9. Mathematical Models for Positioning w Point positioning w Differential positioning – With code ranges – With phase ranges w Relative positioning – Single differences – Double differences – Triple differences

  10. Point Positioning With Code Ranges With Carrier Phases With Doppler Data

  11. Differential Positioning Two receivers used: •Fixed, A: Determines PRC and RRC •Rover, B: Performs point pos’ning with PRC and RRC from A With Code Ranges

  12. Differential Positioning With Phase Ranges

  13. Relative Positioning Aim is to determine the baseline vector A->B. A is known, B is the reference point Assumptions: A, B are simultaneously observed Single Differences: •two points and one satellite •Phase equation of each point is differenced to yield

  14. Relative Positioning w Double differences – Two points and two satellites – Difference of two single-differences gives

  15. Relative Positioning w Triple-Differences – Difference of double-differences across two epochs

  16. Adjustment of Mathematical Models w Models above need adjusting so that they are in a linear form. w Idea is to linearize the distance metrics which carry the form:

  17. Adjustment of Mathematical Models w Each coordinate is decomposed as follows: Allowing the Taylor series expansion of f

  18. Adjustment of Mathematical Models w Computing the partial derivatives and substituting preliminary equations yields the linear equation:

  19. Linear Models w Point Positioning with Code Ranges – Recall: – Substitution of the linearized term (prev. slide) and rearranging all unknowns to the left, gives:

  20. Linear Models w Point Positioning with Code Ranges w Four unknowns implies the need for four satellites. Let:

  21. Linear Models w Point Positioning with Code Ranges w Assuming satellites numbered from 1 to 4 Superscripts denote satellite numbers, not indices.

  22. Linear Models Point Positioning with Code Ranges •We can now express the model in matrix form as l = Ax where

  23. Linear Models Point Positioning with Carrier Phases •Similarly computed. •Ambiguities in the model raise the number of unknowns from 4 to 8 •Need three epochs to solve the system. It produces 12 equations with 10 unknowns.

  24. Linear Models Point Positioning with Carrier Phases Linear Model

  25. Linear Models Point Positioning with Carrier Phases l = Ax

  26. Linear Models Relative Positioning •Carrier phases considered •Double-differences treated •Recall: DD equation * _ •The second term on the lhs is expanded and linearized as in previous models to yield:

  27. Linear Models Relative Positioning •The second term on the lhs is expanded and linearized as in previous models to yield ( [9.133]…see paper pg 262) • l’ s:

  28. Linear Models Relative Positioning • The right hand side is abbreviated as follows (a’s):

  29. Linear Models Relative Positioning •Since the coordinates of A must be known, the number of unknowns is reduced by three. Now, 4 satellites ( j,k,l,m) and two epochs are needed to solve the system.

  30. Extra References w Introduction and overview: http://www.gpsy.org/gpsinfo/gps-faq.txt

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