117 research outputs found

    Modern trends in American teacher training

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    Thesis (Ed.M.)--Boston University, 1946. This item was digitized by the Internet Archive

    In-situ evidence for dextral active motion at the Arabia-India plate boundary

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    International audienceThe Arabia-India plate boundary--also called theOwen fracture zone--is perhaps the least-known boundary among large tectonic plates1-6. Although it was identified early on as an example of a transform fault converting the divergent motion along the Carlsberg Ridge to convergent motion in the Himalayas7, its structure and rate of motion remains poorly constrained. Here we present the first direct evidence for active dextral strike-slip motion along this fault, based on seafloor multibeam mapping of the Arabia-India-Somalia triple junction in the northwest Indian Ocean. There is evidence for 12km of apparent strike-slip motion along the mapped segment of the Owen fracture zone, which is terminated to the south by a 50-km-wide pull-apart basin bounded by active faults. By evaluating these new constraints within the context of geodetic models of global plate motions, we determine a robust angular velocity for the Arabian plate relative to the Indian plate that predicts 2-4mmyr−1 dextral motion along the Owen fracture zone. This transformfault was probably initiated around 8 million years ago in response to a regional reorganization of plate velocities and directions8-11, which induced a change in configuration of the triple junction. Infrequent earthquakes of magnitude 7 and greater may occur along the Arabia-India plate boundary, unless deformation is in the formof aseismic creep

    Neotectonics of the Owen Fracture Zone (NW Indian Ocean): structural evolution of an oceanic strike-slip plate boundary

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    International audienceThe Owen Fracture Zone is a 800 km-long fault system that accommodates the dextral strike-slip motion between India and Arabia plates. Because of slow pelagic sedimentation rates that preserve the seafloor expression of the fault since the Early Pliocene, the fault is clearly observed on bathymetric data. It is made up of a series of fault segments separated by releasing and restraining bends, including a major pull-apart basin at latitude 20°N. Some distal turbiditic channels from the Indus deep-sea fan overlap the fault system and are disturbed by its activity, thus providing landmarks to date successive stages of fault activity and structural evolution of the Owen Fracture Zone from Pliocene to Present. We determine the durability of relay structures and the timing of their evolution along the principal displacement zone, from their inception to their extinction. We observe subsidence migration in the 20°N basin, and alternate activation of fault splays in the vicinity of the Qalhat seamount. The present-day Owen Fracture Zone is the latest stage of structural evolution of the 20-Myr-old strike-slip fault system buried under Indus turbiditic deposits whose activity started at the eastern foot of the Owen Ridge when the Gulf of Aden opened. The evolution of the Owen Fracture Zone since 3-6 Myr reflects a steady state plate motion between Arabia and India, such as inferred by kinematics for the last 20 Myr period. The structural evolution of the Owen Fracture Zone since 20 Myr- including fault segments propagation and migration, pull-apart basin opening and extinction - seems to be characterized by a progressive reorganisation of the fault system, and does not require any major kinematics change

    Do ridge-ridge-fault triple junctions exist on Earth? Evidence from the Aden-Owen-Carlsberg junction in the NW Indian Ocean

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    International audienceThe triple junctions predicted to be ridge^ridge^fault (RRF) types on the basis of large- scale plate motions are theAzores triple junction between theGloria Fault and theMid-AtlanticRidge, the Juan Fernandez triple junction between the ChileTransform and the East Paci¢c Rise and the Aden^ Owen^Carlsberg (AOC) triple junction between theOwen fracture zone (OFZ) and theCarlsberg and Sheba ridges. In the ¢rst two cases, the expected RRF triple junction does not exist because the transform fault arm of the triple junction has evolved into a divergent boundary before connecting to the ridges.Here, we report the results of a marine geophysical survey of the AOC triple junction, which took place in 2006 aboard the R/VBeautemps-Beaupre¤.We show that a rift basin currently forms at the southern end of theOFZ, indicating that a divergent plate boundary between Arabia and India is developing at the triple junction.The connection of this boundary with the Carlsberg and Sheba ridges is not clearly delineated and the triple junction presently corresponds to awidespread zone of distributed deformation.The AOC triple junction appears to be in a transient stage between a former triple junction of the ridge^fault^fault type and a future triple junction of the ridge^ridge^ridge (RRR) type. Consequently, the known three examples of potential RRF triple junctions are actually of the RRR type, and RRF triple junctions do not presently exist on Eart

    Evolution and dynamics of a fold-thrust belt: The Sulaiman Range of Pakistan

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    We present observations and models of the Sulaiman Range of western Pakistan that shed new light on the evolution and deformation of fold-thrust belts. Earthquake source inversions show that the seismic deformation in the range is concentrated in the thick pile of sediments overlying the underthrusting lithosphere of the Indian subcontinent. The slip vectors of the earthquakes vary in strike around the margin of the range, in tandem with the shape of the topography, suggesting that gravitational driving forces arising from the topography play an important role in governing the deformation of the region. Numerical models suggest that the active deformation, and the extreme plan-view curvature of the range, are governed by the presence of weak sediments in a pre-existing basin on the underthrusting Indian Plate. These sediments affect the stress-state in the over-riding mountain range and allow for the rapid propagation of the nose of the range and the development of extreme curvature and laterally varying surface gradients.This study forms part of the NERC- and ESRC-funded project ‘Earthquakes Without Frontiers’. Our thanks go to Jerome Neufeld for many interesting coffee-time discussions, and James Jackson and Dan McKenzie, for comments on the manuscript. We thank Chris Morley and one anonymous reviewer for helpful comments on the manuscript.This article has been accepted for publication in in Geophysical Journal International ©: (2015) 201(2): 683-710, doi: 10.1093/gji/ggv005 , First published online March 9, 2015, Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved
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