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Geological interpretation of near-surface IP and SPM effects in AEM data.

conference contribution
posted on 2024-10-31, 21:05 authored by James MacnaeJames Macnae, Tim Munday
All available inversion software for airborne electromagnetic (AEM) data can fit a non-dispersive conductivity model to the observed responses. Recent research has attempted to permit this conductivity model to be frequency dependent, commonly using a Cole-Cole parameterisation of the induced polarization (IP) effect; but this parameterisation both slows down and destabilises the inversion. Fundamental inductive responses are controlled by the product of conductivity, magnetic permeability and frequency. Little has been published on inverting data affected by frequency dependent magnetic permeability, or super-paramagnetism (SPM), best characterised by a Chikazumi model, which effects are also seen in AEM. Because both IP and SPM effects are small, and usually only obvious at late delay times, the aim of this research was to determine if these IP and SPM effects can be stripped from the data after being approximated with simple dispersive models. We were able to use a thin sheet model to automatically do this. The stripped data can be inverted using a non-dispersive conductivity model. The IP and SPM parameters fitted independently at each fiducial proved to be spatially coherent, and geologically sensible, and as such are very useful in interpretation in their own right.

History

Start page

1

End page

4

Total pages

4

Outlet

Proceedings of the 16th SAGA Biennial Conference and Exhibition (SAGA 2019)

Name of conference

SAGA 2019

Publisher

South African Geophysical Association

Place published

South Africa

Start date

2019-10-06

End date

2019-10-09

Language

English

Copyright

© 2019 SAGA Conference. All rights reserved.

Former Identifier

2006095081

Esploro creation date

2021-08-11

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