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International Research<br />

greatest topographic gradient. A few much larger spurs occur<br />

(e.g., near 45°31’N, 27°51’W), and usually trend NNE. They<br />

appear to be controlled by underlying oblique tectonic trends<br />

associated with the dextral non-transform offset to the next<br />

segment north.<br />

In some places the hummocky volcanoes of the AVR abut directly<br />

against the major normal faults of the MV walls. Elsewhere,<br />

extensive flat-lying lavas were found and, where possible,<br />

we investigated their contacts with the AVR. In several<br />

places minor faulting revealed the internal structure of these<br />

lavas, including open lava tubes and feeder dykes (Fig. 2).<br />

The TOBI magnetisation map revealed a central anomaly magnetic<br />

high with a width (trough-to-trough) of 7 km, much less<br />

than the 18 km predicted for the Brunhes chron at this spreading<br />

rate. This narrow magnetisation high coincides closely with<br />

the AVR, and suggests there may have been a hiatus between<br />

previous magmatism and construction of the current AVR.<br />

MS2000 bathymetry from the two Isis survey dives has revealed<br />

a wealth of new information, including relationships<br />

between volcanic and tectonic features. It also shows that<br />

TOBI sidescan reliably images all volcanic cones down to a<br />

diameter of ~20 m. One surprising feature was vertical failure<br />

scars, evidence for extensive volcanic flank collapse in young<br />

cones on the AVR. This indicates that tectonic erosion of the<br />

crust begins almost as soon as it is formed, and long before it is<br />

affected by major faulting at the edges of the MV floor (Yeo et<br />

al., 2008). Magnetisation maps from the Isis surveys show more<br />

detail; in particular, that magnetisation highs are not confined<br />

to the AVR crest but also occur on its flanks and lateral spurs,<br />

in various relationships to the volcanic architecture.<br />

Visual estimates of sample ages were made in two ways: 1) by<br />

using the degree of sediment cover around the outcrop, and 2)<br />

estimated from the appearance (degree of freshness, etc.) of the<br />

hand specimen. Both estimates show a considerable amount<br />

of scatter. Although the youngest estimates fall on the axis of<br />

the central and southern AVR crest, young ages also occur in<br />

places on its flanks and south of its southern tip, while some of<br />

the oldest estimates also occur on the AVR crest.<br />

MAPRs on the TOBI survey showed hydrothermal plume<br />

signals in the NE of the survey and on the eastern flank of<br />

the AVR near 45°29’N, 27°51’W. However, despite a detailed<br />

MAPR tow-yo grid and Isis dives in the plume vicinity (one of<br />

which encountered a buoyant plume), we were unable to precisely<br />

locate the plume source on the seafloor.<br />

Future work<br />

Post-cruise analysis at Durham (RS, KA, IY) will focus on analysing<br />

the tectonic and volcanic structure of the AVR, building<br />

a volcano-stratigraphic model of it, and incorporating the<br />

results of the other studies into the model. U-series radiometric<br />

dating will be carried out on selected samples by PVC, LT and<br />

KS. Analysis of magnetic survey data will be led by MT with<br />

additional magnetic palaeointensity measurements conducted<br />

by MC, to provide detailed magnetic age proxies. Geochemical<br />

analyses will be carried out at Southampton (BM, NS), Durham<br />

(JD, YN) and Lisbon (PF) to investigate melt sources,<br />

magma storage and fractionation processes, to fingerprint individual<br />

volcanic units, and to provide the analyses needed to<br />

support the U-series dating. KM will analyse the coral samples,<br />

and BM will analyse the MAPR data with Ed Baker at<br />

NOAA.<br />

Acknowledgements<br />

We are greatly indebted to the Captain, officers and crew of<br />

RRS James Cook cruise JC24 and to the shipboard technicians<br />

for their excellent support. The cruise was funded by the Natural<br />

Environment Research Council.<br />

References<br />

Baker, E.T., and H.B. Milburn (1997), MAPR: A new instrument<br />

for hydrothermal plume mapping, Ridge Events, 8,<br />

23-25.<br />

Ballard, R.D., and T.H. Van Andel (1977), Morphology and<br />

tectonics of the inner rift valley at lat. 36°50'N on the Mid-<br />

Atlantic Ridge, Geological Society of America Bulletin, 88,<br />

507-530.<br />

Barclay, A.H., et al. (1998), Seismic structure and crustal magmatism<br />

at the Mid-Atlantic Ridge, 35°N, J. Geophys. Res.,<br />

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Briais, A., et al. (2000), Accretionary processes in the axial valley<br />

of the Mid-Atlantic Ridge 27°-30°N from TOBI side-scan<br />

sonar images, Marine Geophysical Researches, 21, 87-119.<br />

Flewellen, C., et al. (1993), TOBI, a vehicle for deep ocean<br />

survey, Electronics and Communication Engineering Journal<br />

(April 1993), 85-93.<br />

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and structure: Evidence for dike widths, eruption<br />

rates, and evolution of eruptions and axial volcanic ridges, J.<br />

Geophys. Res., 101(B12), 28,265-228,280.<br />

Hussenoeder, S.A., et al. (1996), Near-bottom magnetic survey<br />

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Keeton, J.A., and R.C. Searle (1996), Analysis of Simrad<br />

EM12 multibeam bathymetry and acoustic backscatter data<br />

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Lawson, K., et al. (1996), Detailed volcanic geology of the<br />

MARNOK area, Mid-Atlantic Ridge north of Kane transform,<br />

in Spec. Publ. 118, edited by C.J. MacLeod, et al.,<br />

<strong>InterRidge</strong> News 14 Vol. 17, 2008

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