Abstract
Regional height systems are usually referred to the mean sea level at a reference tide gauge. As the mean sea level gravity potential changes from place to place, regional systems refer to different equipotential surfaces and the establishment of a unified datum requires the determination of one bias per region. This is what is referred to as the height datum problem. The possibility to solve this problem by exploiting the nowadays available satellite gravity mission data, the high resolution global gravity potential models, GNSS heights, as well as leveling and gravity data has been explored. A solution strategy and a first error budget have been presented in Gatti et al. (J Geod 87(1):15–22, 2012), showing that an accuracy of about 5 cm can be globally achieved in the bias computation. In the present work, this strategy, with refinements in the error modeling, is applied to the Italian case, where different height systems are used for the mainland and Sicily and Sardinia islands.
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1 Introduction
The availability of satellite gravity data together with accurate high resolution global gravity models have reopened the possibility to estimate regional height system biases with respect to a common global reference. Different solutions have been explored, for instance by Kotsakis et al. (2012) and Rummel (2012) to solve the problem either on a global or on a local scale. We started from a proposal in Gatti et al. (2012) and performed a first experiment in Italy, where three different height systems are present. The unknown bias of each region reflects in the normal heights of the region itself (Rummel and Teunissen 1988). Height anomalies obtained by differencing GNSS heights and normal heights contain the bias as well. The difference between these biased height anomalies and the corresponding values derived from an unbiased anomalous potential can be therefore modeled as the unknown bias plus errors. When these errors are kept low by an ad hoc combination of satellite-only and high resolution global gravity models, a sufficiently accurate (i.e. with a standard deviation below 5 cm) estimate of the unknowns can be obtained. Although not yet available, Italian normal heights of the main leveling network will be computed in the near future also thanks to a cooperation between the Istituto Geografico Militare (IGM), which is the official institution for creation and maintenance of the Italian geodetic reference network, and the Politecnico di Milano. In particular, normal heights of the GNSS national network will be derived with the corresponding height anomalies, thus allowing for the unification of the Italian height systems. In this work we report the results of a first experiment in this direction, mainly devoted to establish the feasibility of the procedure in terms of accuracy of the solution, when all the available information about the observation errors is exploited. Moreover, we obtained a preliminary estimate by substituting the needed, but not yet computed normal heights, with the currently official heights, derived from the adjustment of leveling data, without applying any correction accounting for gravity. Well aware that those heights can differ from the required normal ones up to some decimeters, we took into account this systematic error with an increased a priori standard deviation of the leveling observations. We will repeat the same evaluation once the proper observables will be computed and released, but we still consider useful the results of this first attempt.
2 The Height Datum Problem and the Adopted Solution
Global satellite gravity potential models can be profitably used in the solution of the height datum problem. The problem is that of determining the biases between the potential of the equipotential surfaces chosen as regional height references \(W = W_{0}^{j}\) and that of the geoid W = W 0:
where \(W_{0}^{j}\) is the actual potential of the mean sea surface at the reference tide gauge \(P_{0}^{j}\) for the region j, W 0 is equal to the normal gravity potential U 0 on the reference ellipsoid. This latter potential is in turn defined by the values of the angular velocity of the Earth ω, its mass M, the ellipsoid semi-major axis a and eccentricity e, which are all well known quantities. The regional bias δ W j in potential reflects in normal heights derived from spirit leveling and gravity observations (cf. Appendix). Height anomalies derived by comparing the nowadays available unbiased ellipsoidal heights h (here unbiased stands for not affected by the potential bias), with the biased normal heights \(\tilde{h}^{{\ast}j}\) of Eq. (12) will be biased as well:
By exploiting Bruns’s formula, for a generic point P of the region j, and recalling Eq. (12), one can write:
where \(\overline{\gamma }\) is the average value of the normal gravity between the ellipsoid and the telluroid, along the normal to the ellipsoid through P. Provided that an unbiased, sufficiently accurate value of the anomalous potential T is available, Eq. (3) can be used to estimate the regional biases h 0 ∗j. Note that a large uncertainty, say 10 m, in the knowledge of the normal height has a negligible effect on the evaluation of the average values of normal gravity \(\overline{\gamma }\). Gatti et al. (2012) proved that a proper combination of the satellite-only global model GOCO (Pail et al. 2010) and the high resolution global model EGM2008 (Pavlis et al. 2012) can give such an unbiased, sufficiently accurate anomalous potential, producing an overall accuracy of 5 cm on the estimated biases. More specifically, one can use satellite-only models up to a degree L, and high resolution models just for the highest degree from L + 1 to their maximum degree H. While satellite-only models are not biased, high resolution models, computed also from gravity anomalies derived from leveling and gravity measurements, are affected by the regional height biases. Nevertheless, the indirect (i.e. through the gravity anomaly Δ g) effects of those biases in the high degree coefficients can be disregarded (Gatti et al. 2012). The boundary degree L in the combination of the low resolution satellite-only model and the high resolution one has to be tuned case-by-case, mainly depending on the size of the involved regions.
3 The Least Squares Estimation: Observation Equations and Observation Error Models
The observation equation in Eq. (3), for a point P belonging to the region j, can be rewritten in the following way:
where T L is the prediction of the anomalous potential at the point P derived from the satellite gravity model up to degree L, T H is the prediction derived from EGM2008 from degree L + 1 up to degree H and ν is the observation noise. For N j points in J regions a linear system of N j × J equations and J unknowns can be solved by a least squares adjustment, once the observation error covariance matrix C ν is defined. This matrix has to account for the errors in the ellipsoidal heights derived from GNSS through the covariance matrix C h , the errors in the normal heights derived from leveling and gravity measurements through \(C_{\tilde{h}^{{\ast}}}\), the commission errors of the satellite-only gravity model up to the degree \(L\) through \(C_{T^{L}}\) and those in the high resolution model from degree L + 1 up to degree H through \(C_{T^{H}}\). It results:
4 The Italian Case
Italy has three different height systems, one for the peninsula and two for Sicily and Sardinia, the tide gauges being in Genova, Catania and Cagliari respectively, for a total of three unknown biases. To estimate those biases, a set of 1,068 points with known GNSS ellipsoidal heights and leveling derived heights was considered. Among them, 43 points are in Sicily, 48 in Sardinia and the remaining 977 in the mainland. The heights derived from leveling measurements were obtained by a least squares adjustment of the observations without any correction accounting for gravity effects (Betti et al. 2013). GNSS heights are referred to the ETRF89 reference frame, epoch 2006. All the data are made available to us by IGM. The evaluation of normal and orthometric corrections is in progress, also thanks to a cooperation between IGM and the Politecnico di Milano. At the available leveling points, the value of the gravity potential was computed starting from the GOCO-03S satellite-only gravity global model and EGM2008 spherical harmonic coefficients. The GOCO-03S model basically combines the ITG-Bonn GRACE solution with the time-wise GOCE one (release R3, that is the second to the last solution based on 1 year and a half GOCE data) (Pail et al. 2011; Mayer-Gürr 2006); the coefficients were downloaded from the website of the International Center for Global Earth Models (ICGEM). Moreover, we could use the GOCO-03S order-wise block diagonal error covariance matrix, which practically brings the same information as the full error covariance matrix (:̧def:̧def Gerlach and Fecher 2012). As for EGM2008 spherical harmonic coefficients, the error coefficient variances and a global grid of local geoid error variances are available. Consistently with GNSS data, the coefficients of the two global models are tide-free. As for leveling data, they are referred to the mean sea level at the three tide gauges of Genova, Catania and Cagliari.
5 Reference Frame Transformations
GNSS coordinates, GOCO-03S and EGM2008 data are referred to different frames with different epochs. Therefore, before combining those observations, transformations to a common frame and epoch must be performed. In order to evaluate the impact of those transformations in the GNSS observations, we started by updating the given coordinates to the most recent frame of the GOCE model. The Italian GNSS data are given in ETRF89, epoch 2006, while GOCE data are in ITRF2008, with a not specified epoch between 2010 and 2011. Both transformations from ETRF89-2006 to ITRF2008-2010 and from ETRF89-2006 to ITRF2008-2011 were performed in three steps:
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from ETRF89-2006 to ITRF89-2006 using the EUREF online tool ‘ETRS89/ITRS TRANSFORMATION’(http://www.epncb.oma.be/_productsservices/coord_trans/);
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from ITRF89-2006 to ITRF2008-2006 using the transformations and parameters provided by the International Earth Rotation and Reference Systems Service (IERS) (http://itrf.ensg.ign.fr/doc_ITRF/Transfo-ITRF2008_ITRFs.txt);
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from ITRF2008-2006 to ITRF2008 epochs 2010 and 2011, using the mean values of the Italian stations velocities again provided by IERS (http://itrf.ensg.ign.fr/ITRF_solutions/2008/doc/ITRF2008_GNSS.SSC.txt). In particular, the stations of Medicina, Genova, Torino I, Cagliari, Matera, Padova and Perugia were taken into account.
It resulted a change in the planimetric coordinates of about 50 cm and about 1 cm in height. In order to evaluate the impact of such differences in our observations we compared the biased height anomalies \(\tilde{\zeta }= h -\tilde{ h}^{{\ast}}\) computed from GNSS heights referred to the original reference frame ETRF89 at epoch 2006 with the anomalies computed from GNSS heights referred to ITRF2008 at epochs 2010 and 2011. The statistics of the differences are reported in Table 1. The differences between the two considered epochs are negligible and we expect that this is true also when considering the larger time span of GRACE data. Analogous transformations for the EGM2008 data cannot be applied because the time reference of its gravity database is not available.
6 Error Budget and the Choice of the Boundary Degree L
In order to set a proper boundary degree in the combination of GOCO-03S and EGM2008 for the solution of the height datum problem, the biases accuracy was evaluated from the available error models. We assumed the set of differences between GNSS and leveling heights to have an uncorrelated noise with a standard deviation \(\sigma _{\tilde{\zeta }} = 1\) cm, that is
where I is the identity matrix. The error covariance matrix \(C_{T^{L}}\) of the set of potential values {T L} predicted in the GNSS-leveling points from GOCO-03S was obtained by propagation from the given order-wise block diagonal error covariance matrix. The covariance matrix \(C_{T^{H}}\) of the set of potential values {T H}, computed in the same points from EGM2008, was obtained by propagation from the coefficient error variances properly rescaled accordingly to the geographical map of local geoid errors (Gilardoni et al. 2013). The resulting error covariance matrix of Eq. (5) is shown in Fig. 1, for L = 250. In Figs. 2, 3 and 4 the GOCO-03S and EGM2008 mean error standard deviations are plotted as functions of L together with the resulting bias standard deviations, for mainland, Sicily and Sardinia respectively. As it can be better appreciated in Fig. 5, where the standard deviations of the three biases are compared, different values of L do not reflect in significant variations of the parameter accuracies. Therefore, we preferred to use GOCO-03S to its highest degree L = 250, in order to reduce the height datum secondary effects in EGM2008 (cf. Sect. 2).
7 Bias Estimation and Analysis of the Least Squares Residuals
The Italian biases of mainland, Sicily and Sardinia were finally computed via least squares. A first model assessment was then performed by analyzing the adjustment residuals. More specifically, a χ 2 test was done at a significance level of 5%, to verify the null hypothesis \(H_{0}\,:\,\sigma _{0}^{2} = 1\) (Koch 1987). The test was mainly devoted to the evaluation of the observation stochastic model. In particular, we are confident on the global gravity model covariances, but we know that uncorrected leveling derived heights, completely disregarding the effects of gravity, introduce systematic errors. These errors can reach some decimeters in zones like the Alps or the Calabrian Arc, where gravity anomalies undergo to high variations. Although a deeper analysis is required, these values partly justifies the following result. We performed different adjustments of the same observations, each time adopting a different a priori height anomaly accuracy \(\sigma _{\tilde{\zeta }}\), looking for that value for which the χ 2 test verifies the null hypothesis. The result of such an approach is that an accuracy of 12 cm can be accepted. A summary of the trials is reported in Table 2. The residuals of the least squares adjustment corresponding to the last trial are reported in Fig. 6.
8 Discussion
A first experiment in the solution of the Italian height datum problem was performed. The main goal was to understand the feasibility of the adopted solution strategy in terms of expected accuracies of the estimates for the best possible error model currently available. The difference between biased and unbiased height anomalies in one height system region can be modeled as the sum of the unknown bias plus a random error, containing from one side the GNSS and leveling/gravity derived height accuracies, from the other side the two global model commission errors. By assuming an accuracy level of 1 cm in the GNSS/leveling data and by using the best error models nowadays available to evaluate the global model commission error covariances, it resulted an accuracy of the estimated biases below 1. 5 cm, the highest error being in Sardinia for its smallest extension. This proves the feasibility of such an approach. In other words, the combination of GOCO-03S up to its highest degree L = 250 and EGM2008 for the remaining higher degrees proves to have a sufficient resolution to describe the unbiased height anomalies (the omission error is sufficiently low); moreover, the effects of the biases entering EGM2008 through the free air gravity anomalies depending on biased heights can be disregarded. This approach clearly depends on the availability of accurate GNSS and normal heights. The actual Italian height values, in fact, leave high systematic errors in the observation residuals. The poor result obtained in this first estimate could be due also to local errors of the global models especially in areas like the Alps or the Calabrian Arc. In any event a partial confirmation of the proposed approach is given by the difference of biases between Sicily and mainland. This has been estimated by us to have a value of 9. 81 cm, with a standard deviation of 2. 57 cm. A similar value, namely 14. 1 cm (personal communication), was independently derived by IGM, by means of a trigonometric connection across the Messina Strait.
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Acknowledgements
The authors would like to thank Roland Pail and Christian Gerlach for kindly providing us the GOCO-03S order-wise block diagonal error covariance matrices.
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Appendix: Determination of Normal Heights from Spirit Leveling and Gravity Observations
Appendix: Determination of Normal Heights from Spirit Leveling and Gravity Observations
We shortly review here two possible ways for the determination of regional normal heights from gravity and leveling observations. In one case we least squares adjust potential differences of height benchmarks derived from observed gravity g and leveling increments δ L [see Heiskanen and Moritz 1967, Eqs. (4–3), page 161]:
by fixing the potential of the reference regional tide gauge to U 0. This introduces a bias in the adjusted potential values equal to the difference between the unknown actual potential of the reference point and U 0:
From these estimated potentials, biased normal heights will be derived as follows:
where \(\tilde{C}\) are the biased geopotential numbers, and \(\overline{\gamma }\) is average normal gravity between the reference ellipsoid and the telluroid along the normal to the ellipsoid through the considered benchmark.
In the other case we least squares adjust leveling increments properly corrected (Betti et al. 2013)
deriving benchmark normal heights with respect to the biased normal height of the reference point \(P_{0}^{j}\). This height, which we set equal to zero, by assuming that the point is on the geoid, is actually proportional to the potential bias:
It follows that the benchmark normal heights are all biased by the normal height of the reference tide gauge:
By comparing Eqs. (9) and (12) an inconsistency appears: in the first case the bias δ W j does not reflect in a constant bias in normal heights, while in the second case it does. In the first case, in fact, δ W j is divided by \(\overline{\gamma }\), which depends of the point where the height is computed. On the contrary, in the second case, the bias in potential is divided by the average normal gravity of the reference point and the ratio is therefore a constant bias in height. This discrepancy can be attributed to the different approximations done in both formulas and it should be better investigated. Nonetheless, the term \(\frac{\delta W^{j}} {\overline{\gamma }}\) undergoes to variations that are smaller than 1 mm even for heights of 2, 000 m, thus making the two solutions practically equivalent. It is clear that the variation of \(\overline{\gamma }\) does not compromise the solution of the height datum problem as it was presented here: the least squares system, in fact, can be easily modified considering as unknowns only the involved potential biases \(\delta W_{0}^{j}\) and correspondingly modifying the least squares coefficient matrix including the known \(\overline{\gamma }\) coefficients.
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Barzaghi, R., Carrion, D., Reguzzoni, M., Venuti, G. (2015). A Feasibility Study on the Unification of the Italian Height Systems Using GNSS-Leveling Data and Global Satellite Gravity Models. In: Rizos, C., Willis, P. (eds) IAG 150 Years. International Association of Geodesy Symposia, vol 143. Springer, Cham. https://doi.org/10.1007/1345_2015_35
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