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Potential Fields SIG

Thursday 18-Mar-10 5:30 PM to 8:30 PM CDT

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Total Seats: 100
Reserved: 4

Hess Club

5430 Westheimer Rd
Houston TX 77056
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Speaker Dr. Philip Ball

Position: Senior Geologist, GoM South Deepwater
Company: Global Exploration (GEX) North America

Event Description

Constraints on continental break-up within the Great Australian Bightfrom seismic reflection, gravity and magnetic data analyses

 

Weakly magmatic passive margins record large amounts of extensional strain prior to breakup, but the role of magma intrusion and the along-strike variability of strain remain poorly understood.  This study utilized existing onshore and offshore gravity, magnetic, seismic reflection, and well data to probe the evolution of rifting, continental breakup, and seafloor spreading across the Australo-Antarctic margins.  Continental rifting along the largely non-volcanic southern margin of Australia occurred during two discrete phases, Syn-rift 1 (165-140 Ma) and Syn-rift 2 (100-83 Ma), but existing data are too sparse to map their spatial extent.

The crustal thickness and structure onshore varies between tectonic domains, thinning from 35-40 km onshore to approximately 10 km beneath the magnetic quiet zone offshore.  Euler deconvolution solutions calibrated with seismic reflection data reveal two discrete sub-parallel rift systems.  Rift Structures of the western rift system overlap that of the eastern rift system, but they are separated by approximately 200 km.  Each system terminates at or near to the boundary of the Gawler craton, suggesting that the craton served as an obstacle to rift propagation. 
The Ceduna sub-basin, which contains up to 15 km of primarily post-rift strata, lies between the two rift zones.  During Syn-rift II, a new rift zone developed oceanward of the Syn-Rift I along the western rift zone.  Minor magmatism and possible mantle exhumation is observed during the second rifting stage and within ~10 My prior to the first well-defined seafloor spreading anomaly. The asymmetry of the conjugate Australian and Antarctic margins may be explained by the along-axis propagation of two spatially separated rifts that eventually linked via a NW-striking system of faults, or through discrete rift jumps to the NE within the rift-overlap zone.  Using observations of the location and distribution of basement related structures, a revised model for breakup between Australia and Antarctica is proposed.

 

 

HESS Club

5:30 - 6:30 Social Hour

6:30 Dinner

Talk After dinner


Comments

HESS Club

5:30 - 6:30 Social Hour

6:30 Dinner

Talk After dinner

Attachments
 

 Event Contact

 Event Coordinator

Greg Jorgensen Greg Jorgensen
(435) 313-1950 (435) 313-1950
   

Potential Fields SIG

Thursday 18-Mar-10 5:30 PM to 8:30 PM CDT

Speaker Dr. Philip Ball

Position: Senior Geologist, GoM South Deepwater
Company: Global Exploration (GEX) North America

Biography

Born in Stafford, England Philip was educated at King Edward VI Stafford before studying geology at Keele University 1994-1998 where he received a B.Sc. Hons degree.  In 1998 he moved to Guildford, UK where he joined ARCO British Limited. 
In 1999 following the takeover/merger of ARCO by BP, he returned to academia joining Royal Holloway University of London.  In 2000 he completed the Basin Evolution and Dynamics M.Sc and in 2005 under the supervision of Cindy Ebinger & Ken McClay he completed a Ph.D on the Break-up history and evolution of the southern passive margin of Australia. 
 
During 2005 he worked as a consultant with Serica Energy (UK) before taking up a post-doctorate research position at NGU, Trondheim, Norway where he worked with Trond Torsvik and Carmen Gaina.  Six months later he joined Statoil as a structural specialist in their Technology division.  In 2007 he joined their Global Exploration group and in 2009 he moved to Houston where he currently resides and works within Statoil's Gulf of Mexico exploration team.

 

Potential Fields SIG

Thursday 18-Mar-10 5:30 PM to 8:30 PM CDT

Hess Club

5430 Westheimer Rd
Houston TX 77056
Google Maps | Hotels Near | Yahoo! Maps | Weather Forecast

Potential Fields SIG

Thursday 18-Mar-10 5:30 PM to 8:30 PM CDT

 
Before 17-Mar-10
After 17-Mar-10
Member:
$30.00
$30.00
Non-Member:
$30.00
$30.00

 


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