--> Tilt-Depth: A Simple Depth-Estimation Method Using First Order Magnetic Derivatives, by James D. Fairhead, Ahmed Salem, and Simon E. Williams; #40390 (2009).
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PSTilt-Previous HitDepthNext Hit: A Simple Previous HitDepthNext Hit-Estimation Method Using First Order Magnetic Derivatives*

James D. Fairhead1, 2, Ahmed Salem1, 2 and Simon E. Williams1, 2

Search and Discovery Article #40390 (2009)
Posted April 8, 2009

*Adapted from poster presentation at AAPG International Conference and Exhibition, Cape Town, South Africa, October 26-29, 2008

1GETECH, Leeds, United Kingdom
2
School of Previous HitEarthNext Hit and Environment, University of Leeds, United Kingdom

Abstract

The Tilt derivative (or angle) is a generalized definition for the local phase. Mapping the magnetic Tilt angle has the advantage of enhancing weak magnetic anomalies, as compared to stronger magnetic anomalies due to the effective automatic gain control (AGC) imposed by the arctan function that restricts the Tilt angle to within the range –90° to +90°, irrespective of the amplitude or wavelength of the magnetic field. We have found that it is possible to simply use the Tilt angle contours of the reduced to pole (RTP) data to estimate both the location and Previous HitdepthNext Hit of magnetic sources.

The method assumes the source is a buried vertical contact model. The zero contours indicate the location of source edges and the half distance between the -45° and +45° contours provides an estimate of the Previous HitdepthNext Hit to top of the buried contact. We present synthetic and field examples to demonstrate the method. When the mapped region between the -45° and +45° contours is high-lighted in grey or in colour, the resulting map provides an intuitive means of spatially identifying the location and Previous HitdepthNext Hit of the magnetic sources. Advantages of the method, called here the ‘Tilt-Previous HitDepthNext Hit’ method, are discussed as well as the effect of errors in RTP and dip-of-contact have on the resulting Previous HitdepthNext Hit estimates.

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Figure 1. Generalized block diagram showing relationship of basin sediment fill to magnetic basement.

Figure 2. Magnetic data for a simple vertical contact model, illustrating the relationship between the Tilt derivative and the Previous HitdepthNext Hit to the magnetic source using Tilt angles ± 45°.

Figure 3A. The contoured RTP field over the 3D model structures (outlined as colour polygons) at 4 km (NW body) with susceptibility 0.002 SI and at 8 km (SE body) with susceptibility 0.001 SI.

Figure 3B. The Tilt anomaly restricted to values lying between ±45°. The colour fill (proprietary GETECH method) between these contours represents the Previous HitdepthNext Hit estimate which varies along the contours due to anomaly interference and non 2D structural effects.

Figure 4. Total magnetic intensity map for southeast Tanzania.

Figure 5. Tilt-Previous HitDepthNext Hit map derived from Figure 7.

Figure 6. Gridded Tilt-Previous HitDepthNext Hit results.

Figure 7. Tilt derivative of RTP magnetic data.

Figure 8. Structural interpretation.

Previous HitIntroductionNext Hit

We provide a rationale for rapidly assessing the Previous HitdepthNext Hit and structure of sedimentary basins from magnetic anomaly data. Our methodology is based on Tilt-Previous HitDepthNext Hit calculated strictly from first-order derivatives of the total magnetic field. We assume a simple buried vertical contact model such as the 0 degree contour of the Tilt derivative of RTP magnetic data closely follows the edge of the vertical contact, while the distance between the ±45° contours provides an estimate of the Previous HitdepthNext Hit to the top of the buried contact. We have applied the Tilt-Previous HitDepthNext Hit method to magnetic data covering various sedimentary basins within the African continent.

Magnetic Data for Basin Mapping

Magnetic data play a crucial role at various stages of hydrocarbon exploration, beginning with the definition of basins in frontier areas (Figure 1). Analysis of magnetic data using special techniques provide estimates of Previous HitdepthNext Hit to basement. The Tilt-Previous HitDepthNext Hit method is a new technique to map variations in basement Previous HitdepthNext Hit directly from magnetic maps.

Magnetic Derived Parameters:

1) Previous HitDepthNext Hit to magnetic basement

2) Strike of contacts/faults

3) Dip of contact

4) Susceptibility contrast

Tilt-Previous HitDepthNext Hit Method: Theory and Simple Examples

The Tilt-Previous HitDepthNext Hit method (Salem et al., 2007), based on a model of a buried 2D vertical contact, provides a relatively simple means to estimate location and strike of geological contacts/faults and Previous HitdepthNext Hit to basement from RTP magnetic anomalies. The horizontal and vertical derivatives of the observed magnetic field are given by:

where h=0 and z are the horizontal and vertical locations of the contact respectively, k is susceptibility contrast and is the magnitude of the magnetic field. The parameter c is given by c=1-cos2i sin2A, where A is the angle between the positive h-axis and magnetic north, i is the ambient field inclination, tanl=tani/cosA, d is the dip (measured from the positive h-axis), and all trigonometric quantities are in degrees. Substituting the above derivative terms into the Tilt equation and assuming a Reduced-to-Pole field, it can be shown that

 formula

The Tilt equation indicates that the horizontal location of the contact (h=0) occurs where Tilt=0°, and h=±qzc when q=±45°, respectively. Thus, Previous HitdepthNext Hit can be estimated directly from a map of the Tilt derivative by measuring the distance between appropriate contours, hence the name Tilt-Previous HitDepthNext Hit. Figure 2 shows the vertical 2D contact model and the resulting Tilt derivative profile for a geomagnetic inclination of 90. The section of the Tilt anomaly between the range 45 is shaded. The value of the Tilt angle above the contact is 0° (h=0), and is +45° when h=zc and -45° when h=-zc.

This suggests that contours of the magnetic Tilt angle can identify both the location and Previous HitdepthNext Hit (half the physical distance between ±45° contours) of contact-like structures. Figure 3A shows the contoured RTP field over 3D model structures (outlined as colour polygons) at 4 km Previous HitdepthNext Hit (NW body) with susceptibility 0.002 SI and at 8 km Previous HitdepthNext Hit (SE body) with susceptibility of 0.001 SI. Figure 3B shows the Tilt anomaly calculated from the polygon anomalies, restricted to values lying between ±45°.

The colour fill between these contours represents the Previous HitdepthNext Hit estimate which varies due to anomaly interference and non 2D structural affects. The examples shown utilize the 45° Tilt derivative contours; other Tilt angles can be used with an appropriate factor to convert the distance between the contours to Previous HitdepthNext Hit.

Application in Tanzania

In this section we demonstrate the Tilt-Previous HitDepthNext Hit method on aeromagnetic data over the Karoo sedimentary rift structures of southeast Tanzania. The regional geological setting is a consequence of the breakup of Gondwana and rifting along the eastern margin of Africa. The Selous Basin is a NNE-SSW trending rift basin infilled with up to ~10 km of mainly non-marine and non-magnetic sediments ranging in age from Permian-Triassic to Tertiary. The basin is bounded to the west and east by shallow basement with the Masasi Spur separating the Selous Basin from the coastal basins of eastern Tanzania. The Rufiji Trough is located to the northeast of the Selous Basin and exhibits E-W extensional structures of Jurassic age superimposed on earlier NNE-SSW trending structures.

A countrywide aeromagnetic grid for Tanzania has been compiled by GETECH from 1 km spaced flight-line data oriented predominantly E-W, with a mean terrain clearance of 120m. The resulting grid has a nodal separation of 0.25 km. Figure 4 shows the TMI anomaly map over the study area and clearly delineates the rift basin outline by the shape change in the frequency content of the magnetic anomalies. Before applying the Tilt-Previous HitDepthNext Hit method, the data were converted to RTP using a magnetic inclination of -40° and a declination of -3.5°, and upward continued to a distance of 1 km.

The Tilt-Previous HitDepthNext Hit map (Figure 5) defines regions of shallow basement (the Masasi Spur, and the region west of the Selous Basin), characterized by numerous closely-spaced lineaments, with corresponding depths shallower than 4 km. Within the Selous Basin and Rufiji Trough, the Tilt ±45° contours are much more widely spaced. These contours define magnetic lineaments within the basin, as well as areas of more chaotic contours which in part could be due to anomaly interference. Basement depths in the Selous Basin range from 3 to 6 km while in the Rufiji Trough they increase to 8 km. These depths show a good correspondence with the regional variation in sediment thicknesses based on seismic and well control data.

Interpolation of the Tilt-Previous HitDepthNext Hit results leads to an initial Previous HitdepthNext Hit to basement map covering the entire basin area, Figure 6, along with other magnetic derivative maps (for example the Tilt derivative itself, Figure 7. These maps, should be viewed as stage products from which structure and Previous HitdepthNext Hit maps can be constructed, Figure 8.

Reference

Salem, A., S. Williams, J. D. Fairhead, D. Ravat and R. Smith, 2007, Tilt-Previous HitdepthNext Hit method; A simple Previous HitdepthTop estimation method using first-order magnetic derivatives: SEG The Leading Edge, v. 26/12, p. 1502-1505.

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