Abstract

Fissure densities and widths have been mapped along the axial zone of the superfast spreading southern East Pacific Rise (EPR) at 17°15′–40′S with the near‐bottom DSL‐120 and Argo II imaging systems. We observe that the youngest lava flows (on a relative age scale) are sparsely fissured and that there is a cumulative increase in fissure abundance with time that produces a strong positive correlation between fissure density and relative age of lava flows. Average fissure widths were used to estimate fissure depths. In the 17°15′–40′S area, calculated fissure depths are estimated to extend below the seismic layer 2A/2B boundary, and fissures are widest/deepest where lava flows are youngest. We interpret these wide fissures in relatively young flows to be eruptive fissures. Relatively young lava flows combined with high average fissure widths south of 17°25′S suggest that there may have been recent dike propagation along the ridge crest in this area. In comparison to the northern EPR at 9°–10°N the density of fissuring on the southern EPR is significantly higher, due in part to the higher occurrence of relatively older, more areally restricted pillow lava flows.

Highlights

  • [3] In this study we present an analysis of fissure characteristics along the superfast spreading southern East Pacific Rise (EPR) and compare the results to those obtained previously along the fast spreading northern EPR

  • [1] Fissure densities and widths have been mapped along the axial zone of the superfast spreading southern East Pacific Rise (EPR) at 17°150– 400S with the near-bottom DSL-120 and Argo II imaging systems

  • We observe that the youngest lava flows are sparsely fissured and that there is a cumulative increase in fissure abundance with time that produces a strong positive correlation between fissure density and relative age of lava flows

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Summary

Introduction

[2] The superfast spreading southern East Pacific Rise (EPR) exhibits a number of features that make it different from slower spreading mid-ocean ridges (MORs), including its relatively long segments, separated by infrequent and small offsets; an inflated cross section; pronounced asymmetry in spreading rate and subsidence; and an abundance of off-axis lava flows and seamounts [Scheirer et al, 1996a, 1998]. 3. Data Acquisition and Analysis [7] In late 1996, the Argo II and DSL-120 seafloor imaging systems [Bowen et al, 1993; Scheirer et al, 2000] were used to conduct a near-bottom survey of the narrow (

Observations and Calculations
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