Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/13699
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dc.contributor.authorSquire, S.-
dc.contributor.authorHillis, R.-
dc.contributor.authorRutty, M.-
dc.date.issued1995-
dc.identifier.citationExploration Geophysics, 1995; 26(2-3):202-205-
dc.identifier.issn0812-3985-
dc.identifier.issn1834-7533-
dc.identifier.urihttp://hdl.handle.net/2440/13699-
dc.description.abstractAbstract A seismic experiment was undertaken in order to investigate the effect of an observed (outcropping) fracture set on shear-wave propagation, and more specifically whether the observed fracture set induced shear-wave birefringence. The source for the experiment was a hammer swung to impact horizontally on a source block coupled to the ground by two large metal pins. Eight three-component geophones recorded arrivals up to 40m offset from the hammer source. Impacts of opposite polarity in the in-line and cross-line direction were differenced in order to maximise S-wave, and minimise P-wave energy. After vector gain, filtering and rotation of the recorded data into in-line and cross-line directions, Alford rotation was undertaken on selected windowed events in order to detect shear-wave birefringence. In-line and cross-line energy is maximised by a co-ordinate rotation to the north?south direction, parallel to the observed fracture direction, suggesting that the observed fracture direction results in an anisotropy that induces shear-wave birefringence.-
dc.language.isoen-
dc.publisherAustralian Society Exploration Geophysicists - CSIRO-
dc.source.urihttp://www.publish.csiro.au/?act=view_file&file_id=EG995202.pdf-
dc.subjectShear-wave birefringence-
dc.subjectfracture direction-
dc.subjecthammer source experiment-
dc.titleHammer-induced seismic investigations in an area of observed anisotropy-
dc.typeJournal article-
dc.identifier.doi10.1071/EG995202-
pubs.publication-statusPublished-
dc.identifier.orcidHillis, R. [0000-0002-5222-7413]-
Appears in Collections:Aurora harvest 2
Geology & Geophysics publications

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