Description: Gas hydrates were recovered from a mud diapir (Mound 11) located on the southern continental slope off Costa Rica at a water depth of about 1000 m during expedition M54/2 with RV METEOR in September 2002. A massive layer of solid methane gas hydrate was retrieved from the base of a gravity corer at a sediment depth of 2 m. Several mound-shaped and carbonate-covered mud diapirs were previously discovered off Costa Rica and Nicaragua during the ongoing research within the framework of the Sonderforschungsbereich 574 "Volatiles and Fluids in Subduction Zones" but solid hydrates were recovered only from Mound 11. This structure has a diameter of about 300 m and protrudes the surrounding seafloor by about 20 m. The seamount sits on approximately 1 km of hemipelagic sediment disrupted by normal faults, which could provide fluid and mass transport pathways from greater depth to the sea floor. Video observations of Mound 11 revealed the presence of authigenic carbonates and bacterial mats indicating methane-charged fluids reaching the sediment surface. Water sampling and gas chromatographic analyses showed methane enrichments in the overlying bottom water confirming the release of methane. In-situ temperature measurements indicated elevated heat flow within the hydrate-bearing sediment strata. Pore fluids recovered from the mound were strongly depleted in dissolved chloride and enriched in boron indicating a deep origin of rising fluids and gases. The results of the ongoing isotopic analysis of gas hydrates and pore waters will be used to further constrain the source of methane-rich fluids.

Description: Microseism recordings from four European broadband stations and from three seismic arrays in Scotland, Norway, and Germany are compared with model wave data of the oceanic wave field in the North Atlantic and local ocean wave data from the Norwegian coast at 60�N, both measured during February–March 2000. Two approaches have been tested to locate generation areas of microseismic energy: a new amplitude correlation technique and beam backprojection from the three seismic arrays. Both techniques reveal that the main generation areas are located in specific regions off the coast of Southwest Norway and North Scotland. Seismic stations distant from these generation areas record a superposition of seismic energy from different source regions. Those close to a specific source region also show a high correlation with it. Both techniques give upper limits for the extent of the generation area of the strongest storm on 6/7 March at the southwest Norwegian coast of about 500 km. By using marine X-band radar measurements of the two-dimensional wave height spectrum, we estimate that the relative change of the extension of the generation area off the coast of southwest Norway during several storms is less than a factor of 3. This indicates that the size of the generation area is controlled by static features as coastline or bathymetry, and not by the extent of the storms. Microseism energy appears to be mainly controlled by the wave height in distinct and identifiable generation regions, so that the wave climate in these regions can be studied using historical records of microseisms.

Description: We have performed a 3-D seismic refraction tomography of a 48 × 48 km2 area surrounding ODP site 757, which is planned to host an International Ocean Network (ION) permanent seismological observatory, called the Ninetyeast Ridge Observatory (NERO). The study area is located in the southern part of the Ninetyeast Ridge, the trail left by the Kerguelen hotspot on the Indian plate. The GEOMAR Research Centre for Marine Geosciences and the Federal Institute for Geosciences and Natural Resources acquired 18 wide-angle profiles recorded by 23 ocean bottom hydrophones during cruise SO131 of R/V Sonne in spring 1998. We apply a first arrival traveltime tomography technique using regularized inversion to recover the 3-D velocity structure relative to a 1-D background model that was constructed from a priori information and averaged traveltime data. The final velocity model revealed the crustal structure down to approximately 8 km depth. Resolution tests showed that structures with approximately 6 km horizontal extent can reliably be resolved down to that depth. The survey imaged the extrusive layer of the upper crust of the Ninetyeast Ridge, which varies in thickness between 3 and 4 km. A high-velocity anomaly coinciding with a positive magnetic anomaly represents a volcanic centre from which crust in this area is thought to have formed. A pronounced low-velocity anomaly is located underneath a thick sedimentary cover in a bathymetric depression. However, poor ray coverage of the uppermost kilometre of the crust in this area resulted in smearing of the shallow structure to a larger depth. Tests explicitly including the shallow low-velocity layer confirmed the existence of the deeper structure. The heterogeneity of the upper crust as observed by our study will have consequences for the waveforms of earthquake signals to be recorded by the future seismic observatory.

Description: ottom simulating reflectors (BSRs) were detected in multichannel seismic reflection data acquired in the vicinity of Isla Mocha across the southern Chile margin and near 33°S. Geothermal gradients were determined from the depth of the BSR that is interpreted to mark the thermally controlled base of a gas hydrate layer. Ground truth for the assessment and additional thermal constraints were provided by downhole measurements obtained during Ocean Drilling Program (ODP) Leg 202 in Site 1233 at 41°S and Sites 1234 and 1235 near 36°S. Both BSR-derived data and downhole temperatures were used to calculate heat flow anomalies and provide new constraints on the thermal regime of the continental slope and downgoing slab in Chile between 32°S and 41°S. Downhole chemical logs of Th, U, and K from Site 859 of ODP Leg 141 have been used to assess the radiogenic heat production in the margin wedge. Heat production is low (∼0.8 μW/m3). However, knowledge of this reduces the errors of estimating the contribution from frictional heating along the subduction thrust fault. With respect to the Eocene age of the incoming oceanic lithosphere, heat flow appears to decrease landward of the deformation front as expected due to the advective transport of heat into the subduction zone by the downgoing slab. Calculations of conductive fore-arc heat flow show that the modelled seafloor heat flow agrees with the measured heat flow only if there is negligible frictional heating. At 33°S, temperatures in the fault zone reach 100°C approximately 60 km landward of the deformation front and are coincident with the onset of earthquake activity and hence mark the up-dip limit of the seismogenic zone. The up-dip limit shifts seaward going to the south, reflecting the progressive southward decrease of lithospheric age of the subducting plate.

Description: Sediment cover over mid-ocean ridges is expected generally to thicken with seafloor age and distance from spreading center, reflecting symmetric sediment accumulation on both flanks of the ridge. In high quality reflection seismic records and sediment echosounding measurements recently collected across the East Pacific Rise we find a strong asymmetric distribution of sediments. On the eastern flank in the EXCO (Exchange between Crust and Ocean) area at 15°S sediment thickness increases only slowly with distance from the spreading axis, and hence crustal age, to about 15 m on 4.5 Ma old crust and 30 m on 7 Ma old crust. Sediments are draping the basement rather than ponding. On the western flank sediment was sampled that is already 70 m thick on 4.5 Ma old crust and up to 150 m on about 7 Ma old crust. Sediment ponds imply efficient transport by gravitationally driven turbidity currents. Sediment accumulation on the western ridge flanks and the rather flat seafloor indicate a redistribution of sediments. Accumulation of sediments corresponds with the extreme asymmetry of a helium plume at 15°S in the South Pacific. A tongue of high 3He extending westward from the rise near 2500–2700 m depth and a corresponding tongue of high temperature suggesting that the helium plume introduced by hydrothermal activity on the EPR spreading axis is being carried westward by abyssal currents. Fall-out of hydrothermal plumes may contribute and intensify sedimentation on the western flanks. However, it is reasonable to hypothesize that hydrothermal plumes are important agents in the dispersal of the larvae of hydrothermal vent fauna and may be responsible for the enhancement of pelagic zooplankton biomass resulting in a larger mass of pelagic rain.