11.3.11 GPS Heighting

GPS AND THE GEOID IN AUSTRALIA

 

	

The Australian Height Datum


The Australian Height Datum (AHD) was implemented on mainland Australia in 1971, and in Tasmania in 1979 (ROELSE et al, 1971; MITCHELL, 1990). This was the first attempt to define a continent-wide levelling datum. Prior to this, Australia had a multitude of levelling datums, each of which was adopted by a government utility to suit its own purpose in a region. These datums were usually based on a local tide gauge (HOLLOWAY, 1988).

The levelling data used in the AHD was largely of third order standard, observed during the previous decade and a half. In addition, some earlier first and second order levelling was included, as was a significant amount of one-way levelling in Queensland and the Northern Territory. Hence the standard of levelling throughout the network was not uniform. A total of almost 100,000 km of levelling in 261 loops was adjusted (ROELSE et al, 1971). The estimated internal precision of the AHD is about 8mm per , where k is the length of the level run in kilometres. That is, a height difference between points 100km apart should have a precision of the order of a decimetre.

In the 1971 adjustment, AHD was tied to Mean Sea Level (MSL) at 30 tide gauges distributed fairly uniformly around the Australian mainland coast. The MSL at each of these tide gauges was derived from several years of readings. These 30 MSL estimates acted as a constraint in the levelling adjustment by being assigned a "fixed" height of 0.000 metres. In Tasmania, the AHD is connected to MSL at two tide gauges, Burnie and Hobart. The AHD (Tasmania) is independent of AHD (Mainland), with no connection ever being made between them.

Is the AHD an orthometric height system? The answer is NO, for several reasons, the most important of which are:

The second point is of particular concern for GPS heighting, as eqn (11.3-1) is no longer strictly valid as far as the AHD is concerned (refer to the early discussion regarding the insensitivity of the geometric method of geoid modelling to weaknesses in the height datum definition). Hence an understanding of the nature and magnitude of errors in the AHD is important if GPS is to used for heighting.

	

Geoid Studies


Astro-Geodetically Determined Geoids

The first such determination was carried out in 1967, using 600 astro-geodetic deflections of the vertical. In 1971 a new geoid was prepared, relative to the AGD, but based on almost double the number of astro-geodetic data (Figure 1 below). In classical geodetic practice the preparation of an astro-geodetic geoid was a necessary part of the process of datum definition known as the "development method", by which the assigned ellipsoidal coordinates of the datum origin station (in Australia's case, the Johnston Trig datum station) were altered in such a way as to ensure an astro-geodetic geoid that minimised the absolute values of the geoid undulations across the datum. The value of N at the Johnston station for a geoid that satisfied this "best-fit" condition should have been -6m. However, due to the legislated value of h at Johnston Origin of 571.2m on the one hand, and the levelled height H of 566.3m on the other, the implied geoid height is in fact +4.9m. Hence the geoid in Figure 5 has a datum shift of +10.9m relative to a "best-fit" geoid. Such a geoid map can be used for converting AHD heights to ellipsoid heights on the AGD, and hence transforming to the Cartesian formulation.



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Figure 1. Astro-geodetic geoid of Australia (mapped relative to the AGD).

	

Geoids from Geopotential Models

High degree spherical harmonic models such as OSU91 and EGM96 provide a very convenient representation of the geoid (Figure 2 shows an earlier OSU89A model).

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Figure 2. Geoid of Australia from OSU89A (relative to the WGS84 ellipsoid).

 

Table 1 shows the difference between two OSU geoid models: OSU89A and OSU91A for a small Sydney network. Note that although there is an approximately 0.25m difference, there is also a small grade and hence the relative geoid heights between points in the network will be slightly different (though only at the few centimetre level), depending upon which geoid model is used.

Table 1. The Sydney GPS network, OSU89A and OSU91A geoid models.
Name Latitude Longitude NOSU89A NOSU91A
B402 S33°54'56.567" E151°13'52.399" 22.454 22.710 .256
BOTY S33°58'23.355" E151°14'10.566" 22.217 22.432 .215
CETS S33°55'05.557" E151°13'57.743" 22.443 22.696 .253
CPDH S33°55'06.198" E151°14'03.196" 22.440 22.692 .252
G106 S33°55'13.377" E151°13'56.767" 22.435 22.687 .252
GLEB S33°52'15.439" E151°11'05.280" 22.679 22.988 .309
KYMA S33°56'45.707" E151°09'39.054" 22.448 22.725 .277
LAKE S33°56'18.011" E151°12'40.436" 22.398 22.654 .256
MBTS S33°56'28.596" E151°15'53.198" 22.297 22.511 .214
MMCH S33°51'33.954" E151°13'18.439" 22.679 22.972 .293
PETE S33°54'36.572" E151°10'31.635" 22.551 22.846 .295
Q744 S33°54'02.521" E151°15'03.756" 22.485 22.735 .250
Q855 S33°54'01.506" E151°14'56.739" 22.489 22.740 .251
ROSE S33°54'49.779" E151°12'18.046" 22.498 22.774 .276
UNSW S33°55'08.060" E151°13'52.148" 22.442 22.697 .255
UU33 S33°55'02.962" E151°13'40.084" 22.452 22.710 .258
WBTS S33°51'10.704" E151°17'09.094" 22.618 22.876 .258

: NOSU91A - NOSU89A

 

Although the evaluated series (eqn (11.3-2)) gives N relative to a geocentric ellipsoid, the procedure described by eqn (11.3-8) can be used to transform the geoid height so that it may refer to a local (non-geocentric) ellipsoid such as that implicit for the AGD, as in the case of Figure 1.

 

Gravimetric Geoids

The first gravimetrically-determined geoid was computed in 1969. Subsequent to that, several refinements to the computational procedures have occurred over the last two decades, but it is only in the last few years has there been a revival of interest in an Australia-wide gravimetric geoid. The task of computing a national geoid (to support GPS activities) was formally assumed in July, 1989, by Australia's national geodetic agency: the Geodetic Services Section of the Australian Surveying and Land Information Group (KEARSLEY & GOVIND, 1991). AUSLIG generated the AUSGEOID93, and most recently the AUSGEOID98 models. These computations were based on the combined gravimetric and geopotential method (based on eqn (11.3-4)). The latest geoid model, AUSGEOID98, is available in electronic form, either as point values or grids, for map sheets at several scales, or over the Internet.

	

Geometric Methods

By their nature these geoid models are local, computed by the GPS surveyor, and have relevance only in the area of the GPS survey. HOLLOWAY (1988) describes several tests using this method of GPS heighting. In addition, the algorithm for obtaining the plane surface fit to the geoid "spot" heights is also described. Figure 3 is an example of the geoid height map that can be derived using such an interpolation method, in this case for a GPS network in South Australia. There were 45 stations in this network that had both GPS and AHD heights. This is far more than would normally be available. Hence the contour map of the geoid shows considerable detail. (It must be emphasised however that the map is not an independent determination of the geoid separation in this area as it also contains errors in the AHD.)

 

 

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Figure 3. Geoid map derived from interpolating spot values of GPS height minus levelled height for a network in South Australia. (HOLLOWAY, 1988)

	

Example of GPS-Derived Orthometric Height in the Sydney GPS Net


A variety of geoid height information was available: OSU89, AUSGEOID93 and AHD minus GPS-derived ellipsoidal height. Table 2 summarises the results of the comparisons. Note that the datum for the GPS network is the Mather pillar at the University of New South Wales. Any error in the height of this fixed station will influence (in an absolute sense) all the derived GPS heights.

Table 2. The Sydney GPS network, a comparison of some geoid models.
Name NOSU89A NGRAV 1 hGPS H NGPS 2
B402 22.454 22.498 .044 59.008 36.410 22.598 -.100
BOTY 22.217 22.269 .052 41.407 19.003 22.404 -.135
CETS 22.443 22.482 .039 109.199 86.605 22.594 -.112
CPDH 22.440 22.486 .046 90.837
G106 22.435 22.470 .035 81.777 59.075 22.702 -.232
GLEB 22.679 22.646 -.033 24.225 1.45* 22.77* -.12*
KYMA 22.448 22.412 -.036 24.336 1.812 22.524 -.112
LAKE 22.398 22.406 .008 59.685 37.15* 22.53* -.12*
MBTS 22.297 22.300 .003 47.437 24.962 22.475 -.175
MMCH 22.679 22.705 .026 33.206 10.375 22.831 -.126
PETE 22.551 22.531 -0.020 29.272 6.604 22.668 -.137
Q744 22.485 22.521 .036 99.863 77.206 22.657 -.156
Q855 22.489 22.519 .030 78.809 56.15* 22.66* -.14*
ROSE 22.498 22.520 .022 82.964
UNSW 22.442 22.480 .038 88.192 65.579 22.613 -.133
UU33 22.452 22.505 .053 50.332 27.623 22.709 -.202
WBTS 22.618 22.652 .034 108.506 85.748 22.758 -.106

1: NGRAV - NOSU89A

2: NGRAV - NGPS

NGPS = hGPS - H

NGRAV computed from OSU91A + observed gravity data (AUSGEOID93)

* implies accuracy of orthometric height is weak


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© Chris Rizos, SNAP-UNSW, 1999