Assessment and Mitigation of Ionospheric Effects on GNSS...
Transcript of Assessment and Mitigation of Ionospheric Effects on GNSS...
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Assessment and Mitigation of Ionospheric Effects on GNSS
Accuracy and Integrity
Wu Chen, Duojie Weng, Shengyue Ji, Zhizhao Liu
Department of Land Surveying and Geoinformatics Hong Kong Polytechnic University
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Background • GPS revolutionize the concepts of
positioning/navigation/timing (PNT) • GPS has become an important infrastructure to support
economic development – Military – Transportation – Telecommunication – Space Industry – Finance – Location Based Services – Surveying – Weather forecasting – Scientific researches
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Background
• Major Concerns on GPS
– Military Design • not built or operated for safety of life requirements
– Military Control • No guarantee on performance and continuity of
services
– Single State Ownership • Clear economical benefits for US
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Background • International Developments
– Augmentation systems • To improve performance of GPS
– Accuracy, Integrity, Coverage • Satellite Based Augmentation Systems (SBAS)
– WAAS, EGNOS, MSAS, QZSS, GAGAN, …. • Ground Based Augmentation systems (GBAS)
– Other Independent GNSS systems • GLONASS (Russian) • Compass (Beidou, China) • Galileo (Europe) • IRNSS (India)
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Background
• GNSS Based Services – Global Services
• GPS, GLONASS, Beidou (III) – Regional Services
• Beidou (II), IRNSS • Satellite Based Augmentation Systems (SBAS)
– WAAS, EGNOS, MSAS, QZSS, GAGAN, …. – Local Services
• DGPS Services – i.e. DGPS station
• GNSS RTK Network – i.e. GNSS CORS network
• Ground Based Augmentation systems (GBAS)
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GNSS Infrastructures in Hong Kong
• DGPS Service – Marine Department (DGPS Beacon for marine
navigation in Hong Kong Water) • Hong Kong GNSS active Network
– RTK for engineering surveying – Established in 2001 – 12 stations, – GPS/GLONASS since last year
• Airport Authority – Feasibility study for implementation of GBAS for Hong Kong
Airport
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Hong Kong GNSS Active Network
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Global Ionosphere activities
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Example of ionosphere distribution in HK
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01 02 03 04 05 06 07 08 09 10 11 12 -0.1
0
0.1
0.2
0.3
0.4
0.5
0.6
0.7 Statistical Character of Temporal Differential VTEC (ROTI)
Month
RM
S (U
nit:
TEC
U)
Distribution of Ionospheric Scintillation in 2001
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How to Model Ionospheric Delay in Low Latitude?
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Analysis of Receiver Bias estimation
• How accurate is the ionosphere estimation? – The receiver bias estimation give a clue
• To test variations of bias estimation
– Global data – Different models – Different Regions
P=P1-P2=m(α)Iv(x,y,h)+DCB+n
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Used dataset – 60 stations
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DCB in America area
Range of daily variation and RMS increase while the latitude decreases.
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The global vs the station-specific
Maximum difference can reach 14.3 TECU. Bigger ones at the low latitude stations.
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Taylor series vs Spherical Harmonic model
Station Name
Taylor (TECU)
Regional SH (TECU)
Difference (TECU)
Geographic longitude
Geographic latitude
gold -12.6 -15.5 2.9 243.11 35.42 jplm 22.5 18.9 3.6 241.82 34.20 pin1 -12.1 -14.6 2.5 243.54 33.61 hers -30.8 -35.9 5.1 0.33 50.86 brus -6.3 -11.1 4.9 4.35 50.79 kosg 34.2 30.8 3.4 5.80 52.17
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Daily variations vs distance between stations
similar latitude
Station name
Latitude longitude Distance To tcms(km)
Correlation coefficient of DCB daily variation
tcms 24.8 120.9 0 --- tnml 24.8 120.9 5 0.977 wuhn 30.5 114.3 910 0.843 kunm 25.0 102.7 1830 0.514 lhaz 29.5 91.1 2973 0.238
Station Latitude longitude Distance To tcms(km)
Correlation coefficient DCB daily variation
tcms 24.8 120.9 0 --- shao 31.1 121.2 698 0.894 pimo 14.5 121.1 1123 0.541 daej 36.3 127.37 1420 0.484
similar longitude
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Summary
• Receiver Bias estimation accuracy is dependent on ionospheric model accuracy
• Spherical harmonics or Taylor series are commonly used – Large number of coefficients – Difficult for prediction
• Can we have a good model to model ionospheric TEC distribution?
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five mathematical functions
cosine normal distribution parabola
cubics witch of Agnesi
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• No.1 function:
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• No.2 function:
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• No.3 function:
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• No.4 function:
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• No.5 function:
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Function performance
• Result-RMS (DCBs are estimated with Bernese)
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Comparison of No. 1 and 3 • DCBs as unknown parameters
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Predictability of model
• Model derived from former day to fit next day
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Use 2 hours data to predict the next 2 hours
• The improved constraint condition
0
2
4
6
8
10
12
2to4 4to6 6to8 8to10 10to12 12to14 14to16 16to18 18to20 20to22 22to24
RMS without constraint
RMS with constraint
RMS with improved constraint
RMS(TecU)
Period(hours)
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Prediction Results • Klobuchar
• Residual error of Prediction model without constraint
• Residual error of Prediction model with constraint
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Prediction Results
Models unit: TECU
Klobuchar (STDEV) 9.14 Without constraint (RMS) 5.71 With constraint (RMS) 4.67
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MEASURES OF PRECISION AND
ACCURACY • Sigma (σ)
– Standard deviation in one, two and three dimensions
– Associated probability levels (in %)
1-d
1 σ 68.0
2 σ 95.0
3 σ 99.7
Probability Density
0.1 0.2 0.3 0.4
-3σ
-2σ
-1σ
0
1σ
2σ
3σ
y
x
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High Accuracy Positioning Service in Hong Kong
• DGNSS + • Data quality improvement
–Smoothing • Spatial Error correction
–Localized models • Reduce effects of scintillation
–Data statistical models
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Data Smoothing
• Data smoothing
Standard Kalman Filter
Smoothed P1, P2
GPS observablesParameter setting
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Code smoothing
• Results – original and smoothed
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Differential Positioning
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Modeling Ionospheric delay along Satellite tracks
Satellite one
Satellite two
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Ionosphere gradients
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Positioning Results
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Results: the std of noise under different ionosphere conditions
Group Number Intervals / meter (RMS of DVTEC)
(Overbounding)
(Overbounding
) Quiet 1,243,192 <0.02 0.372 0.602 0.201
Medium I 7,686, 0.02--0.04 0.412 0.966 0.322
Medium II 3,437 0.04--0.06 0.506 1.396 0.465
Severe 3,607 >0.06 0.743 1.531 0.510
IFσ ,noise IFσ noiseσ
STD of noise under different ionosphere conditions in March, 2001
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Groups of the observations
Class
RoTI /TECU
Quiet
0-0.09
Moderate I
0.09-0.18
Moderate II
0.18-0.27
Severe
> 0.27
41
/0 1
cnoise a a e θ θσ −= +
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Noise level under different ionosphere conditions in 2001
42
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Positioning Results
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Summary
• We have developed a local ionospheric model suitable for low latitude region, with the accuracy of 5 TECU
• To achieve high accuracy positioning in low latitudes: – Gradient of Ionosphere – Statistical models for ionosphere scintillation
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