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Benefits from receiver clock modeling: from PPP-based GPS seismology to Navigation in harsh environment Steffen Sch¨ on 1,2 , Thomas Krawinkel 1,2 , and Ulrich Weinbach 3 1: Institut f¨ ur Erdmessung Leibniz Universit¨ at Hannover 2: Centre for QUantum Engineering and Space Time Research (QUEST), Hannover 3: former IfE and QUEST staff member Introduction In the last years, progress has been made to enable high rate (> 1 Hz) applications for GNSS in Earth observation. In addition to new receiver designs (up to 100 Hz), especially high-rate satellite clock products from the IGS and its analysis centers are now available with a data rate of up to 5 s. Geophysical and atmopheric studies (e.g. vulcano monitoring, tsunami prediction, and especially studies of co- and post-seismic displacements) benefit from these developments opening up new temporal scales for analyses. Fig. 1: Relationship between the parameter tropospheric delay, station height, and receiver clock error. However, high correlations between the parameters of up to 0.99 occur depending on the elevation cut-off angle. This yields a significant degradation of positioning in the vertical direction and masks many valuable geophysical or atmospheric features. Our Solution: Clock modeling improving parameter estimates by incooperation of external clock information. Concept of clock modeling If I the GNSS receiver is driven by a stable oscillator, I its accumulated time error due to random frequency fluctuations of the oscillator σ y (in terms of the Allan deviation) is smaller than the GNSS receiver noise σ l (e.g. 1% of the wavelength) over a significant time interval τ p , i.e. RMS x (τ p )= τ p · σ y (τ p ) l , (1) then I the temporal variation of the receiver clock offset can be - in a physically meaningful way - constrained over intervals τ p where (1) is met. I Within this interval the receiver clock error can be described by a linear or quadratic polynomial, since the random oscillator fluctuations cannot be resolved by GNSS observations because they are below the receiver noise. Fig. 2: Time prediction error τ p · σ y (τ p ) due to random frequency fluctuations for a number of high-precision frequency sources black dashed-lines: noise of the ionosphere-free linear combination of the code b P 3 and carrier phase b L3 observations. Currently only hydrogen maser frequency standards fulfill the condition given by equation (1) and can be modeled over extended time intervals (up to several hours) in GNSS solutions based on carrier phase observations. About 65 stations in the IGS network are equipped with hydrogen maser clocks and typically more than 20 of these reliably deliver frequency stabilities that meet or outperform the specifications given above. Some chips scaled atomic clocks, like e.g., the CSAC can be used for clock modeling in code-based navigation. Application of clock modeling to the Chile 2010 Earthquake GPS Data and analysis concept I 1 Hz GPS data of the IGS station CONZ made available by BKG I 3 hours data before and after earthquake included for reliably estimating the float carrier phase ambiguities I GPS receiver (CONZ) connected to well-maintained hydrogen maser frequency standard I processed with PPP software developed at Institut f¨ ur Erdmessung I linearly interpolated 5 s GPS satellite clocks, provided by CODE, (Bock et al. 2009) I epoch-wise independent receiver clock offsets or piece-wise linear segments (5 min) intervals. Mainshock (a) (b) Fig. 3: Kinematic PPP position estimates and receiver clock error during the main shock of the 8.8 magnitude 2010 Chile earthquake (a) using epoch-wise clock estimation, (b) using clock modeling taking the h-maser performance at CONZ into account Benefits: less jumps, continuous and reliable time series Application of clock modeling to the Chile 2010 Earthquake Aftershock -0.04 -0.02 0 0.02 Δ N [m] 0.14 0.16 0.18 0.2 Δ E [m] -0.04 -0.02 0 0.02 Δ U [m] 7:59 8:00 8:01 8:02 8:03 8:04 8:05 8:06 8:07 0.04 0.06 0.08 0.1 Δ t r [m] UTC [h:min] (a) -0.04 -0.02 0 0.02 Δ N [m] 0.14 0.16 0.18 0.2 Δ E [m] -0.04 -0.02 0 0.02 Δ U [m] 7:59 8:00 8:01 8:02 8:03 8:04 8:05 8:06 8:07 0.04 0.06 0.08 0.1 Δ t r [m] UTC [h:min] (b) Fig. 4: Kinematic PPP position estimates and receiver clock error during a 6.9 magnitude aftershock (a) using epoch-wise clock estimation, (b) using clock modeling taking the h-maser performance at CONZ into account I Vertical station displacements hidden in the noise of the kinematic height estimates (Conventional PPP solutions Fig.5(a)) I High mathematical correlation (here about 89.6%) expressed by the similarity of the vertical position time series and the epoch-wise receiver clock offsets (cf. arrows, Fig.5(a)) I Tightly constraining the receiver clock according to the physical clock performance, the signature of the earthquake becomes clearly visible also in the height component (Fig.5(b)) I The standard deviation of height time series is improved by 37% from 12 mm to 7.5 mm. Application of clock modeling to code-based navigation (a) (b) (c) (d) Fig. 5: Kinematic code-based position estimates and receiver clock error during a kinematic test drive (a) Test trajectory (b) receiver set up with three identical receivers, (c) Results with internal clock, (d) Results from clock modeling I Clock modeling with two states (offset, drift) Kalman model. I Again, the noise of the height component is reduced (Static positioning up to 23%, kinematic positioning up to 50%). I Height component less vulnerable w.r.t. systematics, since correlations between the parameters are reduced. I Availability improved, since positioning with only three satellites in view is possible. I Vibrations may degrade the results. Conclusions I The usage of highly stable GNSS receiver oscillators allows to improve the accuracy of kinematic vertical position estimates by a factor of 2-3. I Co-seismic few mm vertical displacements of a stand-alone GPS receiver connected to a hydrogen maser frequency standard can be detected using the PPP approach with enhanced clock modeling. I More accurate height variations can be derived from Precise Point Positioning using IGS orbit and clock products. This is interesting for high-frequency deformation monitoring such as GPS seismology. I Chip-scaled atomic clocks together with clock modeling improve the availability, continuity and precision of code-based navigation solutions in harsh environments. References: Bock H, Dach R, Jaeggi A, Beutler G (2009): High-rate GPS clock corrections from CODE: Support of 1 Hz applications. J.Geod.83:1083–1094. Krawinkel T, Sch¨ on S, Bauch A (2014): Application of miniaturized atomic clocks in kinematic GNSS Single Point Positioning. In Proc. EFTF submitted. Krawinkel T, Sch¨ on S (2014): Applying miniaturized atomic clocks for improved kinematic GNSS Single Point Positioning. In Proc. ION GNSS submitted. Weinbach U, Sch¨ on S (2011): GNSS receiver clock modeling when using high-precision oscillatorsand its impact on PPP. Adv.SpaceRes.47(2):229-238. Weinbach U. (2013): Feasibility and impact of receiver clock modeling in precise GPS data analysis, PhD thesis, Wissenschaftliche Arbeiten der Fachrichtung Geod¨ asie und Geoinformatik der Leibniz Universit¨ at Hannover, No. 303. Acknowledgements: This work has been funded by the DeutscheForschungsGemeinschaft (DFG) in the framework of the centre for QUantum Engineering and Space Time research (QUEST), Hannover as well as the VENADU project funded ba a resolution of the German Bundestag under the label (50NA1213). The authors would like to thank BKG for making 1 Hz data of the station CONZ publicly available. The CODE satellite orbit and clock products were indispensable for this research. Institut f¨ ur Erdmessung Schneiderberg 50 D-30167 Hannover IGS Analysis Center Workshop 2014 | Pasadena | US 23. - 27. June, 2014 Steffen Sch¨ on Thomas Krawinkel Ulrich Weinbach www.ife.uni-hannover.de {schoen}@ife.uni-hannover.de

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Page 1: Benefits from receiver clock modeling: from PPP-based GPS ... 2014 - PS06 - Schon... · Benefits from receiver clock modeling: from PPP-based GPS seismology to Navigation in harsh

Benefits from receiver clock modeling: from PPP-based GPSseismology to Navigation in harsh environment

Steffen Schon1,2, Thomas Krawinkel1,2, and Ulrich Weinbach3

1: Institut fur Erdmessung Leibniz Universitat Hannover

2: Centre for QUantum Engineering and Space Time Research (QUEST), Hannover

3: former IfE and QUEST staff member

Introduction

In the last years, progress has beenmade to enable high rate (> 1 Hz)applications for GNSS in Earthobservation. In addition to newreceiver designs (up to 100 Hz),especially high-rate satellite clockproducts from the IGS and itsanalysis centers are now availablewith a data rate of up to 5 s.Geophysical and atmopheric studies(e.g. vulcano monitoring, tsunamiprediction, and especially studies ofco- and post-seismicdisplacements) benefit from thesedevelopments opening up newtemporal scales for analyses.

Fig. 1: Relationship between the parameter tropospheric delay, station height,and receiver clock error.

However, high correlations between the parameters of up to 0.99 occur depending on theelevation cut-off angle. This yields a significant degradation of positioning in the verticaldirection and masks many valuable geophysical or atmospheric features.

Our Solution: Clock modeling improving parameter estimates by incooperation ofexternal clock information.

Concept of clock modeling

IfI the GNSS receiver is driven by a stable

oscillator,I its accumulated time error due to random

frequency fluctuations of the oscillator σy (interms of the Allan deviation) is smaller thanthe GNSS receiver noise σl (e.g. 1% of thewavelength) over a significant time intervalτp , i.e.

RMSx(τp) = τp · σy(τp) < σl, (1)

thenI the temporal variation of the receiver clock

offset can be - in a physically meaningfulway - constrained over intervals τp where (1)is met.

I Within this interval the receiver clock errorcan be described by a linear or quadraticpolynomial, since the random oscillatorfluctuations cannot be resolved by GNSSobservations because they are below thereceiver noise.

Fig. 2: Time prediction error τp · σy(τp) due to random frequencyfluctuations for a number of high-precision frequency sourcesblack dashed-lines: noise of the ionosphere-free linear combinationof the code bP3 and carrier phase bL3 observations.Currently only hydrogen maser frequency standards fulfill thecondition given by equation (1) and can be modeled over extendedtime intervals (up to several hours) in GNSS solutions based oncarrier phase observations. About 65 stations in the IGS networkare equipped with hydrogen maser clocks and typically more than20 of these reliably deliver frequency stabilities that meet oroutperform the specifications given above.Some chips scaled atomic clocks, like e.g., the CSAC can be usedfor clock modeling in code-based navigation.

Application of clock modeling to the Chile 2010 Earthquake

GPS Data and analysis conceptI 1 Hz GPS data of the IGS station CONZ made available by BKGI 3 hours data before and after earthquake included for reliably estimating the float carrier

phase ambiguitiesI GPS receiver (CONZ) connected to well-maintained hydrogen maser frequency standardI processed with PPP software developed at Institut fur ErdmessungI linearly interpolated 5 s GPS satellite clocks, provided by CODE, (Bock et al. 2009)I epoch-wise independent receiver clock offsets or piece-wise linear segments (5 min)

intervals.

Mainshock

(a) (b)

Fig. 3: Kinematic PPP position estimates and receiver clock error during the main shock of the 8.8 magnitude 2010 Chile earthquake(a) using epoch-wise clock estimation, (b) using clock modeling taking the h-maser performance at CONZ into accountBenefits: less jumps, continuous and reliable time series

Application of clock modeling to the Chile 2010 Earthquake

Aftershock

−0.04

−0.02

0

0.02

Δ N

[m]

0.14

0.16

0.18

0.2

Δ E

[m]

−0.04

−0.02

0

0.02

Δ U

[m]

7:59 8:00 8:01 8:02 8:03 8:04 8:05 8:06 8:070.04

0.06

0.08

0.1

Δ t r [m

]

UTC [h:min]

(a)

−0.04

−0.02

0

0.02

Δ N

[m]

0.14

0.16

0.18

0.2

Δ E

[m]

−0.04

−0.02

0

0.02

Δ U

[m]

7:59 8:00 8:01 8:02 8:03 8:04 8:05 8:06 8:070.04

0.06

0.08

0.1

Δ t r [m

]

UTC [h:min]

(b)

Fig. 4: Kinematic PPP position estimates and receiver clock error during a 6.9 magnitude aftershock (a) using epoch-wise clockestimation, (b) using clock modeling taking the h-maser performance at CONZ into account

I Vertical station displacements hidden in the noise of the kinematic height estimates(Conventional PPP solutions Fig.5(a))

I High mathematical correlation (here about 89.6%) expressed by the similarity of the verticalposition time series and the epoch-wise receiver clock offsets (cf. arrows, Fig.5(a))

I Tightly constraining the receiver clock according to the physical clock performance, thesignature of the earthquake becomes clearly visible also in the height component (Fig.5(b))

I The standard deviation of height time series is improved by 37% from 12 mm to 7.5 mm.

Application of clock modeling to code-based navigation

(a) (b)

(c) (d)

Fig. 5: Kinematic code-based position estimates and receiver clock error during akinematic test drive (a) Test trajectory (b) receiver set up with three identical receivers,(c) Results with internal clock, (d) Results from clock modeling

I Clock modeling with twostates (offset, drift) Kalmanmodel.

I Again, the noise of the heightcomponent is reduced (Staticpositioning up to 23%,kinematic positioning up to50%).

I Height component lessvulnerable w.r.t. systematics,since correlations between theparameters are reduced.

I Availability improved, sincepositioning with only threesatellites in view is possible.

I Vibrations may degrade theresults.

Conclusions

I The usage of highly stable GNSS receiver oscillators allows to improve the accuracy ofkinematic vertical position estimates by a factor of 2-3.

I Co-seismic few mm vertical displacements of a stand-alone GPS receiver connected to ahydrogen maser frequency standard can be detected using the PPP approach with enhancedclock modeling.

I More accurate height variations can be derived from Precise Point Positioning using IGSorbit and clock products. This is interesting for high-frequency deformation monitoring suchas GPS seismology.

I Chip-scaled atomic clocks together with clock modeling improve the availability, continuityand precision of code-based navigation solutions in harsh environments.

References:Bock H, Dach R, Jaeggi A, Beutler G (2009): High-rate GPS clock corrections from CODE: Support of 1 Hz applications.J.Geod.83:1083–1094.Krawinkel T, Schon S, Bauch A (2014): Application of miniaturized atomic clocks in kinematic GNSS Single Point Positioning. InProc. EFTF submitted.Krawinkel T, Schon S (2014): Applying miniaturized atomic clocks for improved kinematic GNSS Single Point Positioning. In Proc.ION GNSS submitted.Weinbach U, Schon S (2011): GNSS receiver clock modeling when using high-precision oscillatorsand its impact on PPP.Adv.SpaceRes.47(2):229-238.Weinbach U. (2013): Feasibility and impact of receiver clock modeling in precise GPS data analysis, PhD thesis, WissenschaftlicheArbeiten der Fachrichtung Geodasie und Geoinformatik der Leibniz Universitat Hannover, No. 303.

Acknowledgements:This work has been funded by the DeutscheForschungsGemeinschaft (DFG) in the framework of the centre for QUantum Engineeringand Space Time research (QUEST), Hannover as well as the VENADU project funded ba a resolution of the German Bundestagunder the label (50NA1213). The authors would like to thank BKG for making 1 Hz data of the station CONZ publicly available.The CODE satellite orbit and clock products were indispensable for this research.

Created with LATEX beamerposterInstitut fur ErdmessungSchneiderberg 50D-30167 Hannover

IGS Analysis Center Workshop 2014 |Pasadena | US

23. - 27. June, 2014

Steffen SchonThomas Krawinkel

Ulrich Weinbachwww.ife.uni-hannover.de

{schoen}@ife.uni-hannover.de