1887
24th International Geophysical Conference and Exhibition – Geophysics and Geology Together for Discovery
  • ISSN: 2202-0586
  • E-ISSN:

Abstract

Remanent magnetisation is an important consideration in magnetic interpretation. In some cases failure to properly account for remanence can lead to completely erroneous interpretations. In general the strength and orientation of remanence are unknown. Two main strategies have been pursued for “unconstrained” inversion of large data sets. One strategy is to invert quantities, such as total magnetic gradient (3D analytic signal), which are insensitive to magnetisation direction. The inverted property is then magnetisation amplitude. Another strategy is to invert for the magnetisation vector, allowing its three components to vary freely. These approaches are useful, but the resulting magnetisation models are highly non-unique.

When interpreting magnetic data in tandem with geological modelling there is greater potential to infer remanence parameters. Non-uniqueness is reduced if the shape of magnetic domains is constrained, especially if the susceptibility is known and if remanence can be assumed uniform. Accordingly, inverting for the remanent magnetisation of individual homogeneous geological units of arbitrary 3D shape is the subject of this paper. Our remanent magnetisation inversion (RMI) approach can be regarded as a generalisation of parametric inversion of simple geometric bodies.

If susceptibility is known, the optimal remanent magnetisation vector within each selected unit is determined via iterative inversion. Sensitivity to change in magnetisation is determined in the x-, y-, and z-directions, and the perturbation vector is found via the method of steepest descent. If the susceptibility is unknown, the optimal susceptibility of each unit (subject to bounds) can be determined via a similar inversion procedure. The geological units can carry remanent magnetisation, but it is fixed during this stage. The susceptibility and/or remanence inversions can be repeated, if necessary, to refine the magnetic parameters. Self-demagnetisation and interactions are taken into account when susceptibilities are high.

The application of the RMI algorithm is illustrated in examples for both known and unknown susceptibility.

Loading

Article metrics loading...

/content/journals/10.1071/ASEG2015ab188
2015-12-01
2026-01-14
Loading full text...

Full text loading...

References

  1. Clark, D.A., Saul, S.J., and Emerson, D.W., 1986, Magnetic and gravity anomalies of a triaxial ellipsoid: Exploration Geophysics, 17, 189-200.
  2. Ellis, R.G., de Wet, B., and Macleod, I.N., 2012, Inversion of magnetic data from remanent and induced sources: Extended Abstract, ASEG 22nd International Geophysical Conference and Exhibition, Brisbane.
  3. Fullagar, P.K., and Pears, G.A., 2013, 3D magnetic modelling and inversion incorporating self-demagnetisation and interactions: Extended Abstract, ASEG 23rd International Geophysical Conference and Exhibition, Melbourne.
  4. Lelievre, P.G., and Oldenburg, D.W., 2009, A 3D total magnetization inversion applicable when significant, complicated remanence is present: Geophysics, 74, L21-L30.
  5. Li, Y., Shearer, S.E., Haney, M.M., and Dannemiller, N., 2010, Comprehensive approaches to 3D inversion of magnetic data affected by remanent magnetization: Geophysics, 75, L1-L11.
  6. Paine, J., Haederle, M., and Flis, M., 2001, Using transformed TMI data to invert for remanently magnetised bodies: Exploration Geophysics, 32, 238-242.
  7. Schaa, R., and Fullagar, P.K., 2010, Rapid, approximate 3D inversion of transient electromagnetic (TEM) data: Expanded Abstract, SEG 80th Annual International Meeting, Denver.
  8. Shearer, S., and Y. Li., 2004, 3D Inversion of magnetic total-gradient data in the presence of remanent magnetization: 74th Annual International Meeting, SEG, Expanded Abstracts,774-777.
/content/journals/10.1071/ASEG2015ab188
Loading
  • Article Type: Research Article
Keyword(s): 3D magnetic inversion; constraints; non-uniqueness; remanent magnetisation
This is a required field
Please enter a valid email address
Approval was a Success
Invalid data
An Error Occurred
Approval was partially successful, following selected items could not be processed due to error