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doi:10.2204/iodp.sp.340T.2011

Publisher’s notes

Material in this publication may be copied without restraint for library, abstract service, educational, or personal research purposes; however, this source should be appropriately acknowledged.

Citation:
Blackman, D., and Slagle, A.L., 2011. Atlantis Massif oceanic core complex: velocity, porosity, and impedance contrasts within the domal core of Atlantis Massif: faults and hydration of lithosphere during core complex evolution. IODP Sci. Prosp., 340T. doi:10.2204/iodp.sp.340T.2011

Distribution:
Electronic copies of this series may be obtained from the Integrated Ocean Drilling Program (IODP) Scientific Publications homepage on the World Wide Web at www.iodp.org/​scientific-publications/.

This publication was prepared by the Integrated Ocean Drilling Program U.S. Implementing Organization (IODP-USIO): Consortium for Ocean Leadership, Lamont-Doherty Earth Observatory of Columbia University, and Texas A&M University, as an account of work performed under the international Integrated Ocean Drilling Program, which is managed by IODP Management International (IODP-MI), Inc. Funding for the program is provided by the following agencies:

• National Science Foundation (NSF), United States
• Ministry of Education, Culture, Sports, Science and Technology (MEXT), Japan
• European Consortium for Ocean Research Drilling (ECORD)
• Ministry of Science and Technology (MOST), People’s Republic of China
• Korea Institute of Geoscience and Mineral Resources (KIGAM)
• Australian Research Council (ARC) and GNS Science (New Zealand), Australian/New Zealand Consortium
• Ministry of Earth Sciences (MoES), India

Disclaimer

Any opinions, findings, and conclusions or recommendations expressed in this publication are those of the author(s) and do not necessarily reflect the views of the participating agencies, IODP Management International, Inc., Consortium for Ocean Leadership, Lamont-Doherty Earth Observatory of Columbia University, Texas A&M University, or Texas A&M Research Foundation.

This IODP Scientific Prospectus is based on precruise Science Advisory Structure panel discussions and scientific input from the designated Co-Chief Scientists on behalf of the drilling proponents. During the course of the cruise, actual site operations may indicate to the Co-Chief Scientists, the Staff Scientist/Expedition Project Manager, and the Operations Superintendent that it would be scientifically or operationally advantageous to amend the plan detailed in this prospectus. It should be understood that any proposed changes to the science deliverables outlined in the plan presented here are contingent upon the approval of the IODP-USIO Science Services, TAMU, Director in consultation with IODP-MI.

August 2011

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