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iSPI TM — the improved source parameter imaging method
Author(s) -
Smith Richard S.,
Thurston Jeffrey B.,
Dai TingFan,
MacLeod Ian N.
Publication year - 1998
Publication title -
geophysical prospecting
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.735
H-Index - 79
eISSN - 1365-2478
pISSN - 0016-8025
DOI - 10.1046/j.1365-2478.1998.00084.x
Subject(s) - geology , regional geology , anomaly (physics) , environmental geology , image (mathematics) , economic geology , interpretation (philosophy) , estimation theory , field (mathematics) , algorithm , computer science , artificial intelligence , hydrogeology , mathematics , physics , telmatology , geotechnical engineering , condensed matter physics , pure mathematics , programming language
Interpretation of an anomalous magnetic response involves determining the parameters that characterize the source of the anomaly. The depth to the top of the structure is a parameter that is commonly sought, and the Source Parameter Imaging TM (SPI TM ) method is one way of determining this depth estimate. One advantage of the SPI method is that the depths can be displayed on an image. Typically there can be one image for an assumed contact (fault) model and another image for an assumed dipping thin sheet (dike) model. The depth estimate obtained will depend on the model assumed. An improvement to the source parameter imaging method extends the method to horizontal cylinders and at the same time allows the most appropriate model to be determined automatically. This model can be displayed on an image and the correct depth estimate for each anomaly can also be determined. The depth estimates can therefore be summarized on one map independent of an assumed model. The images generated from synthetic and field data show that the improved SPI method makes the task of interpreting magnetic data significantly easier.