Terrain Correction
Use the Gravity > Terrain Corrections >Terrain Correction menu option (geogxnet.dll(Geosoft.GX.Gravity.TerrainCorrection;Run)*) to calculate the gravity terrain effect. The terrain correction will be calculated for every station in the database, considering a correction area of 2 x correction distance by 2 x correction distance centered on the station, and saved in the output terrain correction channel.
Terrain Correction dialog options
Application Notes
Gravity terrain correction is a computationally intensive process. Initially, when the Oasis montaj gravity workflow was created, the concept of detailed local terrain contribution versus averaged regional contribution was introduced. The latter was computed once to speed up calculations. This workflow was a compromise between faster computation and the precision related to the contribution of the far field. In the original workflow, users had to ensure that the local and regional grid nodes aligned properly. With increasing computation speeds, the old dual-step model became unnecessary. A regional correction grid calculation was no longer needed as it no longer offered an advantage. As of version 2025.1, the terrain effect at each gravity station should be calculated using a single distance equivalent to the far distance.
Definitions:
- Topography: The rise and fall of landmasses relative to sea level. Topography can extend below the surface of bodies of water.
- DEM: The Digital Elevation Model; it defines the contact of material (rock or water) with air.
Terrain correction accounts for the effects of topography variability. The gravitational attraction of a landmass above the observation station pulls away from Earth, decreasing the gravitational effect of the slab (Figure 1 - a) Solid rock). Similarly, a mass deficiency in the vicinity of the station results in a negative effect due to the lack of material and, consequently, the lack of attraction (Figure 1 - b) Air).
Figure 1: Schematic illustration of Bouguer slab, terrain, and variable water elevations
The magnitude of the terrain effect at each gravity station depends on the variability of the topography, with nearby topography exerting a stronger influence due to the inverse (distance) square law of gravity. Detailed information about nearby topography is necessary as it has a stronger impact on gravity measurements. Distant features, which have a smaller gravitational effect, can be represented more generally with larger cell sizes. The Terrain Correction tool will decimate the grid as it moves outwards from each gravity station for which it calculates the terrain effect.
If you have a detailed local DEM but only a coarse regional DEM, to account for an adequate correction distance, first invoke Boolean Operations and merge the two grids. Select the grid with the smaller cell size as “Grid 1”, select the “Or” logic, opt for the maximum grid size, and use the grid values of Grid 1 in the overlapping area. This will resample the regional grid to the smaller grid increment. The Terrain Correction tool will take care of decimating this finer DEM grid as necessary.
The graph below illustrates the gradual change in the magnitude of the terrain correction as a function of the correction distance for a given gravity survey in ragged topography (in red). The topography was then scaled to produce the other two profiles. The graphs asymptote (thin grey lines) at some distance away from the gravity station. Selecting a correction distance at 95% of the asymptote is reasonable. Asymptotes are indicated with thin grey lines, while the 95% mark is indicated with a dashed line, and the intersections are shown with grey bars.
Figure 2: Profiles of terrain correction versus correction distance for three DEM grids of varying reliefs.
The DEM grid used to produce the terrain effect of the red profile has a maximum vertical topographic range of 300 m with a standard deviation of 67 m. The graph asymptotes around 0.049 mGals. 95% of this amplitude is reached at a distance of 44 km, an adequate distance for this DEM.
The DEM grid used to produce the terrain effect of the blue profile has a maximum vertical topographic range of 660 m with a standard deviation of 135 m (about double the grid above). The graph asymptotes around 0.196 mGals. 95% of this amplitude is reached at a distance of 55 km, an adequate distance for this DEM.
The DEM grid used to produce the terrain effect of the green profile has a maximum vertical topographic range of 165 m with a standard deviation of 32.5 m (half of the first DEM grid). The graph asymptotes around 0.012 mGals. 95% of this amplitude is reached at a distance of 25 km, an adequate distance for this DEM.
Conclusion: There is no one-to-one relationship between the vertical relief of the DEM grid and the correction distance. Set the distance to the maximum distance of the available DEM. It is not necessary to go beyond 100 km for very rugged areas, while for relatively flat areas, much shorter distances would produce reasonable results.
At the edge of a cliff or gorge, the terrain correction is inevitably in error; therefore, it is recommended not to measure gravity at the edge of sharp relief.
In general, for relatively flat regions where the variability of the terrain is in the tens of meters, terrain corrections range from 0.1 to 1 mGal. In hilly regions with variability in the hundreds of meters, the terrain effect is in the order of 1 to 10 mGals, and in mountainous regions, the terrain effect is on the order of several tens of mGals. Bathymetric correction is similar to terrain correction; gravity corrections are determined by a combination of the thickness of the water column and the solid material.
Topography Grid
The topography grid is centered on the gravity survey area and should extend at least by the correction distance beyond the edges of the survey perimeter. Dummy terrain values are interpolated using a weighted average of the surrounding points. If the grid does not extend sufficiently beyond the survey area, and the specified correction distance is greater than the distance between the topography grid outline and the survey perimeter, then the grid is extended to meet this margin. The extension is simply the other edge of the topography grid reflected on the opposite side. This approach, however, is a fallback only and could introduce errors in the terrain effect calculation if the nature of the topography changes significantly or if the survey terrain has a regional slope. The correction distance should be chosen carefully to avoid introducing errors to stations located near the edge of the defined topography grid.
Figure 3: Reflection of terrain elevation on opposite sides
Digital gridded terrain models are often available from government sources and can be used to simplify the application of regional terrain corrections.
Topography grids can be generated by combining DEM and locally surveyed bathymetry data. For surveys over coastal regions, the topography terrain grid would be a merge of the DTM and the bathymetry data.
These grids should not be gridded to a cell size much smaller than the original sampling accuracy of the DEM data. If the topography grid is produced by gridding the elevation of the gravity survey, the grid cell size should be about one-half of the nominal gravity station spacing
Terrain Correction Methods
Terrain corrections are calculated using a combination of the methods described by Nagy (1966) and Kane (1962). The terrain effect is derived based on the annular ring segment approximation to square prisms.
To calculate the correction at each gravity station, the topography grid is resampled, centered on that gravity station, and extended to the correction distance (see Figure 3). The correction is calculated based on a series of square zones, the effects of which are added to produce the terrain correction:
- Near zone: Zone 0 covering a 1-cell radius ring centered on the station.
- Intermediate zones: Zone 1 covering a 2 to 8-cell flat-topped square prism in a square ring. Zone 2 at a distance of 9-16 cells and at double the cell size.
- Far zones: Zone 3 and beyond, covering concentric flat-top square rings beyond 16 cells. The number of far zones depends on the correction distance.
Each zone aligns with the next. For more processing efficiency, the far zones are progressively desampled by a factor of 2 and set to the average of the grid values they cover. In Zone 2 every 4 initial adjacent DEM cells are averaged; in Zone 3, every 16 initial cells, and so on.
Figure 4: Resampling of DEM for each gravity station by zones
Equations:
Zone 0: Sloped triangle (Kane)
Innermost 4 prisms:
Where:
g = the terrain effect
D = the density
G = the gravitation constant
Zones 1 & 2: Right rectangular prism (Nagy)
1 to 8 cells away from station:
The three bars indicate the limiting values x1, x2 – y1, y2 - z1, z2. The above notation expands to 9 terms, each with a combination of xi, yj, zk.
Zone ≥3: Square segment ring (Kane)
Beyond 8 cells away from station up the specified inner distance:
For shipborne and airborne surveys, corrections are calculated as follows:
-
Using the flat-topped square prism approach of [Nagy ,1966]3 for the near and intermediate zones.
-
Using the rod formula [Telford et al.,1976]4 for the far zone.
The water depth in the "Water" channel should be filled with positive values if there is water under the survey station. Particularly for the shipborne survey, the water channel must be filled with positive values; otherwise, the result will be a dummy grid.
Script Mode
The following parameters are only available when running the current GX from a script:
Terrain correction grid: The terrain correction grid contains the correction component beyond the survey areas extended by the correction distance. The magnitude of the correction in the terrain correction grid is normalized and scaled to the provided Earth density, and added to the calculated correction of the more highly sampled topography grid. Script Parameter: GRTERAIN.CORGRD |
Local slope channel: The local slope of the grid is calculated on the fly; however, if local slopes have been measured at each station, you can specify the slope channel. (The slope is only applicable to Zone 0; see the Application Notes section.) Script Parameter: GRTERAIN.SLOPCH |
References
- [1] W. J. Hinze, R.B. Von Frese, A. Saad, Gravity and Magnetic Exploration: Principles, Practices and Applications, (Cambridge University Press, 2013), pp. 134-135.
- [2] M. F. Kane, "A Comprehensive System of Terrain Corrections using a Digital Computer", Geophysics, vol. 27, no. 4 (1962), pp. 455-462.
- [3] D. Nagy, "The Gravitational Attraction of a Right Rectangular Prism", Geophysics, vol. 31, no. 2 (1966), pp. 362–371.
- [4] W. M. Telford, L.P. Geldart, R.E. Sheriff, Applied Geophysics, Second Edition, (Cambridge University Press, 1976), pp. 13-14.
*The GX.NET tools are embedded in the geogxnet.dll file located in the "...\Geosoft\Desktop Applications \bin" folder. If running this GX interactively, bypassing the menu, first change the folder to point to the "bin" directory, then supply the GX.NET tool in the specified format. See the topic Run GX for more details on running a GX.NET interactively.
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