Passive seismic studies show configuration of Paleoproterozoic subduction zones and their role in craton assembly in Western Australia

Ruth Murdie, Huaiyu Yuan, Michael C. Dentith, Simon P. Johnson, Klaus Gessner

Research output: Contribution to journalConference paperpeer-review

Abstract

The Capricorn Orogen Passive source Array (COPA) is the passive source seismic component of a major Science and Industry Endowment Fund (SIEF) project, "The distal footprints of giant ore systems: Capricorn case study". COPA focuses on the deep crustal and shallow lithospheric structure in the Capricorn Orogen with the aim to better understand the tectonic amalgamation of the Western Australian Craton. The objective of COPA is to produce 3D multiple scale seismic images across the orogeny, that together with other geological and geophysical datasets help constrain the timing and kinematic evolution of Capricorn Orogen’s fault zones, and their role in the metallogenic history.
Original languageEnglish
Pages (from-to)1-5
Number of pages5
JournalASEG Extended Abstracts
Volume2016
Issue number1
DOIs
Publication statusPublished - 2016
EventInternational Geophysical Conference and Exhibition in Adelaide (25th : 2016): Interpreting the Past, Discovering the Future - Adelaide, Australia
Duration: 21 Aug 201624 Aug 2016

Keywords

  • Capricorn Orogen
  • passive seismic monitoring
  • receiver function
  • ambient noise
  • common conversion point

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