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Estimation of uncalibrated hardware delays for single- difference ambiguity resolution Javier Tegedor , Ola Øvstedal Department of Mathematical Sciences and Technology Norwegian University of Life Sciences (UMB)

Javier Tegedor, Ola Øvstedal - Portal · – Receivers providing P1: Ashtech, Septentrio, Javad, Topcon… When only C1 observations are present (Trimble, Leica): 1. Estimate UHDs

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Page 1: Javier Tegedor, Ola Øvstedal - Portal · – Receivers providing P1: Ashtech, Septentrio, Javad, Topcon… When only C1 observations are present (Trimble, Leica): 1. Estimate UHDs

Estimation of uncalibrated hardware delays for single-

difference ambiguity resolution Javier Tegedor, Ola Øvstedal

Department of Mathematical Sciences and Technology

Norwegian University of Life Sciences (UMB)

Page 2: Javier Tegedor, Ola Øvstedal - Portal · – Receivers providing P1: Ashtech, Septentrio, Javad, Topcon… When only C1 observations are present (Trimble, Leica): 1. Estimate UHDs

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Contents

  Implementation of Wide-Lane and Narrow-Lane Uncalibrated Hardware Delays (UHD)

  Validation of WideLane UHDs with CNES products

  Impact of Differential Code Biases (P1-C1) in the UHD estimation

  Potential Extension for GLONASS

  Format proposal for exchange of biases

Page 3: Javier Tegedor, Ola Øvstedal - Portal · – Receivers providing P1: Ashtech, Septentrio, Javad, Topcon… When only C1 observations are present (Trimble, Leica): 1. Estimate UHDs

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Introduction

  Double difference (DD) ambiguity estimation has been traditionally used in network solutions

–  Identification of DD integer ambiguities

–  Hardware biases cancel out

  Recent developments (CNES, GFZ, NrCan) propose the estimation of the hardware biases

–  Ambiguity resolution for standalone receivers

•  Single differences (SD) between satellites

•  Zero-difference (ZD) when the station biases are also estimated

+ + - -

+ -

Page 4: Javier Tegedor, Ola Øvstedal - Portal · – Receivers providing P1: Ashtech, Septentrio, Javad, Topcon… When only C1 observations are present (Trimble, Leica): 1. Estimate UHDs

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IFik =

1f12 − f2

2 f12L1 − f2

2L2( )= ρ + c(Δti −Δt

k )−κNw −λn (N1 +ηi −ηk )

λn =c

f1 + f2≈10.7cm

  Wide-lane ambiguity extracted from Melbourne-Wübbena phase and code combination:

  Narrow-lane ambiguity are extracted from ionosphere-free phase

combination:

ESTIMATIO

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Mathematical model

MWik =

1f1 − f2

f1L1 − f2L2( )− 1f1 + f2

f1P1 + f2P2( ) =

= λw (Nw +ωi −ωk )→ Nw = N1 − N2

λw =c

f1 − f2≈ 86.2cm

Wide-lane Uncalibrated Hardware Delays (W-UHD)

Narrow-lane Uncalibrated Hardware Delays (N-UHD)

Page 5: Javier Tegedor, Ola Øvstedal - Portal · – Receivers providing P1: Ashtech, Septentrio, Javad, Topcon… When only C1 observations are present (Trimble, Leica): 1. Estimate UHDs

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Estimation of UHD in a network solution

  The estimation process uses undifferenced observations

  Double differencing is used in the ambiguity fixing for adding integer constraints to the normal equations

  As a by product, satellites and stations UHDs are generated

  Full consistency is ensured between UHDs and clocks

  1 constant W/N-UHD parameter per station/satellite over 24 hours

Page 6: Javier Tegedor, Ola Øvstedal - Portal · – Receivers providing P1: Ashtech, Septentrio, Javad, Topcon… When only C1 observations are present (Trimble, Leica): 1. Estimate UHDs

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Ambiguity Residuals from Network solution

  Zero-difference ambiguity fractional parts after estimation of satellite and

stations UHDs:

Page 7: Javier Tegedor, Ola Øvstedal - Portal · – Receivers providing P1: Ashtech, Septentrio, Javad, Topcon… When only C1 observations are present (Trimble, Leica): 1. Estimate UHDs

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PPP with ambiguity fixing

  The satellite UHD are used to recover integer ambiguities SD, added as a constraints to the normal equations

  The use of SD is beneficial as the station UHDs do not need to be estimated additionally

Page 8: Javier Tegedor, Ola Øvstedal - Portal · – Receivers providing P1: Ashtech, Septentrio, Javad, Topcon… When only C1 observations are present (Trimble, Leica): 1. Estimate UHDs

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Ambiguity Residuals from PPP solution

  Single-difference ambiguity residuals after correction with satellite UHDs:

80.2% 92.9 %

Page 9: Javier Tegedor, Ola Øvstedal - Portal · – Receivers providing P1: Ashtech, Septentrio, Javad, Topcon… When only C1 observations are present (Trimble, Leica): 1. Estimate UHDs

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Impact of P1-C1 bias on ambiguity resolution

  Typical IGS-like process uses P1/P2/L1/L2

–  Receivers providing P1: Ashtech, Septentrio, Javad, Topcon…

  When only C1 observations are present (Trimble, Leica):

1.  Estimate UHDs using C1/P2/L1/L2

•  A different set of UHDs (and clocks) is generated:

2.  Convert C1 to P1 applying DCBs to the observations

•  Any error in the DCB will translate into the estimated UHDs

•  Is the solution equivalent when using P1 or C1+DCB?

ωC1k =ωP1

k −f1

f1 + f2DCBP1−C1

k

ΔtC1k = ΔtP1

k +f12

c( f12 − f2

2 )DCBP1−C1

k

Page 10: Javier Tegedor, Ola Øvstedal - Portal · – Receivers providing P1: Ashtech, Septentrio, Javad, Topcon… When only C1 observations are present (Trimble, Leica): 1. Estimate UHDs

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Impact of P1-C1 bias on ambiguity resolution

  Estimation of W/N-UHD, orbit and clocks, in 3 network configurations:

1.  P1/P2

2.  C1/P2, correcting C1 with Differential Code bias P1-C1:

•  p1c1bias.hist and cc2noncc_v6.3

3.  C1/P2 with no DCB correction

•  Different set of biases and clocks

Page 11: Javier Tegedor, Ola Øvstedal - Portal · – Receivers providing P1: Ashtech, Septentrio, Javad, Topcon… When only C1 observations are present (Trimble, Leica): 1. Estimate UHDs

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Impact of P1-C1 bias on ambiguity resolution

-0.2

-0.15

-0.1

-0.05

0

0.05

0.1

0.15

0.2

1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31

Wid

eLan

e U

HD

diff

eren

ce (

ccyl

es)

GPS PRN Number

Differences with CNES values

UMB:P1/P2

UMB:C1+DCB/P2

-0.6

-0.4

-0.2

0

0.2

0.4

0.6

0.8

1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31

Wid

eLan

e U

HD

(cc

yles

)

GPS PRN Number

Estimation of WideLane biases for DOY 150/2011

CNES

UMB : P1/P2

UMB : C1+DCB/P2

UMB : C1/P2

Page 12: Javier Tegedor, Ola Øvstedal - Portal · – Receivers providing P1: Ashtech, Septentrio, Javad, Topcon… When only C1 observations are present (Trimble, Leica): 1. Estimate UHDs

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Impact of P1-C1 bias on ambiguity resolution

  Is it possible to resolve integer ambiguities with C1/P2 or C1+DCB/P2?

  The PPP ambiguity residuals at SD level are very similar, but the estimated UHDs are different

  PPP user needs to process the same signals for achieving successful ambiguity resolution

Page 13: Javier Tegedor, Ola Øvstedal - Portal · – Receivers providing P1: Ashtech, Septentrio, Javad, Topcon… When only C1 observations are present (Trimble, Leica): 1. Estimate UHDs

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Impact of P1-C1 bias on ambiguity resolution

  Estimation of W-UHD with P1/P2 or C1+DCB/P2

–  Process daily estimates for full year 2011

–  Analyse impact of the DCBs in the estimated WideLane biases

–  CNES values are taken as reference

–  A common offset is removed to allow for comparison

–  RMS for all satellites around 0.02 cycles

PRN30 anomaly

Page 14: Javier Tegedor, Ola Øvstedal - Portal · – Receivers providing P1: Ashtech, Septentrio, Javad, Topcon… When only C1 observations are present (Trimble, Leica): 1. Estimate UHDs

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PRN30 W-UHD estimation

PRN30/SVN30 decommissioned

Correct DCB value for

PRN30/SVN35

PRN30/SVN35 commissioned

2 3 1

Page 15: Javier Tegedor, Ola Øvstedal - Portal · – Receivers providing P1: Ashtech, Septentrio, Javad, Topcon… When only C1 observations are present (Trimble, Leica): 1. Estimate UHDs

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Ambiguity residuals for G30

  Inaccuracies in the DCBs are directly absorbed in the W-UHDs

  Fewer ratio of ambiguities fixed if DCB has an error

–  Even ambiguities fixed to the wrong integer!

1.7%

21.7% 75.5% 1 2 3

Page 16: Javier Tegedor, Ola Øvstedal - Portal · – Receivers providing P1: Ashtech, Septentrio, Javad, Topcon… When only C1 observations are present (Trimble, Leica): 1. Estimate UHDs

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Would it work for GLONASS?

  For GLONASS the inter-frequency biases do not cancel out completely in the differentiation process

  How stable are the biases within the same frequency?

–  Analyze wide-lane biases consistency between consecutive passes of the same satellite

–  48 h Rinex_v3 data from UNB3 (NETR5)

0

0.05

0.1

0.15

0.2

1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30

Wid

eLan

e cy

cles

GPS PRN Number

C1C/C2W

C1C/C2X

0

0.05

0.1

0.15

0.2

1 2 4 5 6 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24

Wid

eLan

e cy

cles

GLONASS orbit slot number

C1C/C2P

C1C/C2C

Page 17: Javier Tegedor, Ola Øvstedal - Portal · – Receivers providing P1: Ashtech, Septentrio, Javad, Topcon… When only C1 observations are present (Trimble, Leica): 1. Estimate UHDs

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Conclusions and format proposal

  Uncalibrated hardware delays can be generated in a network using different code signals

–  Accurate DCBs are needed to estimate reliable W-UHDs

  For the PPP user, it is fundamental to keep consistency with the satellite biases in order to achieve ambiguity fixing

  The proposed Bias Sinex format can be extended for accommodating these biases:

–  Add new bias identifiers: WHD & NHD

–  Example:

*-------------------------------------------------------------------------------!* Solution INdependent EXchange Format (SINEX) !*-------------------------------------------------------------------------------!+FILE/REFERENCE! REFERENCE FRAME IGS08!-FILE/REFERENCE!! DESCRIPTION Bias Sinex with Uncalibrated Hardware Delays ! CONTACT [email protected]!*-------------------------------------------------------------------------------!*-------------------------------------------------------------------------------!*-------------------------------------------------------------------------------!+BIAS/SOLUTION!*BIAS SVN_ PRN SITE DOMES____ OBS1 OBS2 BIAS_START__ BIAS_END____ UNIT __ESTIMATED_VALUE____ _STD_DEV___! WHD G048 G07 L1P L2P 11:200:00000 11:201:00000 m -.423123098473891E+00 .389234E-02! NHD G048 G07 L1P L2P 11:200:00000 11:201:00000 m .342346908876489E-02 .984758E-03!!