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* AWI
Multibeam Echosounder data
* TOBI sidescan sonar data * Sparker seismic data * Calypso piston core MD01-2464 * Multicore PS64/240-1 * Video imagery The
Gollum Channel System in the A
prominent feature in the morphology of the deep-sea channels are the steep
flanks with numerous slides and slumps. These slope
instabilities are often
associated with pockmarks. A
careful attempt of palaeo-climate reconstruction was made using detailed
particle size analyses of the piston core with additional information on
carbonate content, magnetic susceptibility, density, SCOPIX-imagery, grey
scales and luminosity. Using this time-frame, it appears the channels have not
been active in the past 130ka. The deposits of only very few and weak turbidite
currents have been observed during what was interpreted as the glacial
intervals of the core. In the last two interglacial periods bottom currents have
been reworking the sediment. In the Holocene that bottom current is
significantly stronger, represented by a sandy contourite on top of both the
piston core and the multicore. The northwards flowing Mediterranean Outflow
Water is most likely responsible for this deposition. So the Gollum
Channels seem to have been inactive for quite a while, but are still influenced
by bottom currents and tides. Sediment from the many slide and slumps together
with the influx from the
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Updated:
16th of September 2007 |
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