Segmentation and cycles of crustal accretion at mid-ocean ridges: a study of the Reykjanes Ridge
Early studies of mid-ocean ridges suggest a fundamental difference between crustal accretionary processes at slow- and fast-spreading ridges. Accretion, and the supply of melt to the crust itself, is thought to be highly episodic at slow-spreading ridges but steady-state at fast-spreading ridges. Ho...
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| Format: | Thesis |
| Language: | unknown |
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2003
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| Online Access: | http://etheses.dur.ac.uk/4121/ http://etheses.dur.ac.uk/4121/1/4121_1640.pdf |
| Summary: | Early studies of mid-ocean ridges suggest a fundamental difference between crustal accretionary processes at slow- and fast-spreading ridges. Accretion, and the supply of melt to the crust itself, is thought to be highly episodic at slow-spreading ridges but steady-state at fast-spreading ridges. However, recent studies are beginning to question this model, with evidence for the temporal variation in crustal accretionary processes at all spreading rates emerging. This study provides evidence from bathymetry, TOBI sidescan, gravity and magnetic data, collected during different cruises to the Reykjanes Ridge, for the temporal nature of crustal accretion and its relationship to segmentation. Interpretation of TOBI images indicates that individual adjacent axial volcanic ridges (AVRs) vary in relative age, suggesting that they are at various stages of an evolutionary lifecycle, with episodic cycles of magmatic and tectonic activity. However, prior to investigating the possible effects of tectonomagmatic cycles on the crustal structure of AVRs, the effect of the Iceland hotspot on the ridge is examined. The along-axis free-air gravity anomaly is forward modelled in 2-D, revealing an along-axis increase in crustal thickness towards Iceland from 7.5 km to 10.5 km and a decrease in mantle densities from 3.30 to 3.23 g cm"^ between 57 30'N and 62 N. Calculation of the residual mantle Bouguer Anomaly (RMBA) and inversion of magnetic anomaly data, reveal intermediate-wavelength fluctuations in RMBA amplitude and magnetization intensity respectively that are attributed to hotspot pulses, with 59 N marking the southern most extent of the most recent pulse. Removal of the hotspot effect on the gravity data reveals short-wavelength RMBA lows, associated with individual AVRs, superimposed on a broad ridge-trending low. Along-AVR-axis gravity modelling shows that a number of these RMBA lows can be explained by a 200-800 m thickening of the crust and/or by the presence of 5-20% partial melt in the mid-crust. A correlation between ... |
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