GNSS antenna offset field test in Metsähovi



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GNSS antenna offset field test in Metsähovi

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GNSS antenna offset field test in Metsähovi Ulla KALLIO, Hannu KOIVULA, Sonja NYBERG, Pasi Häkli, Paavo Rouhiainen, Veikko Saaranen, Finland Zane Cirule, Didzis Dobelis, Vladimirs Golovka, Latvia Questions How well the individual antenna calibration values are valid in the field? What is the consistency between two sets (Ashtech Choke Ring ASH700936C_M and Leica AR25.R4 with radome) of GPS antennas? 1

GPS compared with EDM Reference: The electronic distance measurements with Mekometer ME 5000 traceable to the definition of the metre through the Nummela Standard Baseline, which has been measured with the Väisälä light interference method. accuracy ±(0.2 mm +0.2 ppm) Baseline measurements in Olkiluoto deformation network in 2003 2012 investigation area, which was selected as a candidate for the final disposal sites of spent nuclear fuel Length [mm] Olkiluoto baseline 511259 GPS 511258 EDM 511257 511256 511255 1994 1999 2004 2009 Year Antenna calibration and test measurements in Kyviskes calibration baseline Individual absolute calibration for the antennas in 2009 (Geo ++) Measurements in Lithuania Kyviskes calibration baseline and testfield in 2008 (Hannu Koivula and Pasi Häkli) lengths 20...1320 m Processing strategies: individual and type calibrated antenna tables a local and global ionosphere model three different cut off elevation angles several linear combinations several ambiguity resolution strategies 2

Δφ = f ( α, z) Offset and phase center variation ARP One antenna, two calibrations mm 2.0 1.5 1.0 0.5 0.0 0.5 1.0 Differences of antenna calibration corrections in L1 We need a simple test to verify the calibration results! 3

Length [mm] 511259 511258 511257 Olkiluoto baseline Olkiluoto baseline, the latest results GPS EDM 511256 511255 1994 1999 2004 2009 Year Technique spesific offsets in local tie measurements Difference in local tie vector between terrestrial and GPS determination 4

Antennas used in our field test 8 Leica AR25.R4 antennas with radome 9 Ashtech Choke Ring antennas without radome Geo++ individual calibration tables for all antennas Cut off angle 15 degrees 8 4 0 4 LEIAR25.R4 LEIT ASH700936C_M 8 4 4 0 5

Simple test procedures Rotating the antennas without tilting (absolut N and E) Antenna swapping (relative) Comparing with ground truth (distances, height differences) Permutation method (relative) Antenna circulation (on three or more points) Full roving method (Bányai) 440 504 505 1 988 22 40 2 40 988 22 3 22 40 988 4 988 3 5 5 5 988 3 6 3 5 988 7 988 6 7 8 7 988 6 9 6 7 988 10 988 11 12 11 12 988 11 12 11 12 988 13 988 194 754 14 754 988 194 15 194 754 988 16 988 761 770 17 770 988 761 18 761 770 988 19 988 772 959 20 959 988 772 21 772 959 988 22 988 963 995 23 995 988 963 24 963 995 988 Observation schedule 48 h sessions cut of angle: 5 degrees 505 504 44 0 METS 6

Field work Zane Cirule, Didzis Dobelis and Vladimirs Golovka from Riga Technical University visited Finnish Geodetic Institute in summer 2011 in ERASMUS program. During three months in summer 2011 antennas were changed twice a week Bernese processing separately L1 and L2 solutions Geo++ individual absolute calibration tables using the offsets in tables (and with zero phase center offsets using only phase center variations) IGS rapid orbits and earth orientation parameters available soon after the measurements Ambiguites were solved using the sigma strategy The troposphere was modelled using Saastamoinen apriori model mapped with Dry Niell mapping function. Zenith path delay paremeteres were estimated using Wet Niell mapping function at 2 hour intervals. The observation cut off angle was set to 10 degrees. 7

Mathematical model in least squares adjustment Functional model X pb X pa + Oa 2 Oa1 = ΔX AB X pc X pa + Oa3 Oa1 = ΔX AC 1. session X pb X pa + Oa1 Oa3 = ΔX AB X pc X pa + Oa 2 Oa3 = ΔX AC 2. session X pb X pa + Oa3 Oa 2 = ΔX AB X pc X pa + Oa1 Oa 2 = ΔX AC 3. session Stochastic model Full covariance matrix from SINEX files Height difference compared with levelled height difference 8

Results L2 4,00 mm 3,00 2,00 1,00 0,00 1,00 The residual offsets, L2 solution North East Up 3 5 6 7 11 12 22 40 194 754 772 959 963 988 995 2,00 3,00 4,00 Results L1 4,00 3,00 2,00 1,00 The residual offsets, L1 solution North East Up mm 0,00 1,00 2,00 3,00 4,00 3 5 6 7 11 12 22 40 194 754 772 959 963 988 995 9

Conclusion Did we get answers to our questions? We may ecpect a small jump to time series of coordinates when we replace the antenna and antenna type The offset values of the individual absolute calibration were not consistent between the two antenna types tested in Metsähovi. There seems to be biases which propagate to the coordinate results. New questions What is the role of the near field effect? Can we isolate the near field effectfromourresults? What to do next? We will reprocess the data with several different strategies We will process the extra measurements we made in autumn 2011 We will continue our tests using different mountings in different location and environment. Thank you for your attention! 10