The surface of the Amazon fan is covered by a distributary network of meandering channels that has been mapped with GLORIA side-scan sonar (Damuth et al., 1988). They are bounded by high natural levees and are perched atop their own overbank deposits (Pirmez and Flood, 1995). In 1994, during ODP Leg 155, 17 sites were drilled. At several sites, the uppermost approximately 100 m of the succession was cored several times with the advanced piston corer to ensure sufficient sediment for detailed sedimentary studies. However, seismic lines across across the ODP sites were average in quality. Their resolution was not sufficient for a detailed correlation with ODP cores. In mud-dominated submarine fans, the nature and distribution of sandy deposits are critical for oil companies and also to understanding the sedimentary dynamics of fan development, in particular the initiation, growth, and abandonment of channel-levee systems but also understanding the sediment spreading in distal lobes. Channel patterns similar to those of the Amazon Fan are seen on other mud-rich fans, which have been acoustically imaged to varying degrees of detail. However, sampling of the fan sediments generally has been limited to the upper 10 m, and the lithofacies and/or sedimentary processes associated with the acoustic units observed on seismic reflection data are mostly conjectural. During the Lobestory cruise, we used a new multichannel HR seismic streamer to collect high resolution seismic lines across the ODP sites and explored the distal part of the most recent Amazon turbidite system, which was unmapped and unknown.

West: -50.0000 East: -44.0000 North: 9.0000 South: 3.0000

West: NaN East: NaN North: NaN South: NaN

Expedition: 155

Provider: SEDIS Publication Catalogue

Data set link: http://sedis.iodp.org/pub-catalogue/index.php?id=2009-055738 (c.f. for more detailed metadata)

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