首页> 外文期刊>Tectonophysics: International Journal of Geotectonics and the Geology and Physics of the Interior of the Earth >Segmentation and morphology of the Central Indian Ridge between 3°S and 11°S, Indian Ocean
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Segmentation and morphology of the Central Indian Ridge between 3°S and 11°S, Indian Ocean

机译:印度洋中部3°S和11°S之间的中印度洋脊线的分割和形态

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The segmentation pattern of 750. km long Central Indian Ridge (CIR) between 3°S and 11°S latitudes in the Indian Ocean has been studied using multibeam bathymetry and magnetic data. Twelve ridge segments were identified that are separated by well defined transform faults and non-transform discontinuities. Magnetic model studies qualify the ridge as a slow spreading ridge with average full spreading rates varying from 26 to 38. mm/yr. The disposition of the magnetic anomalies suggests that the plate opening direction has not changed during the last 0-4. Ma period. Along axis variations in the magnetic anomalies, presence of axial volcanic ridges on the inner valley floor, variations in the depth and geometry of the rift valley, suggest distinct variati'ons in the accretionary processes along the ridge. Based on these characteristics and the segmentation pattern, we suggest that ten ridge segments are undergoing less magmatic phase of extension, while two segments have shown characteristics of magmatic accretion. The linear segments with narrow and shallow rift valley floor and near symmetric magnetic anomalies are identified as segments with magmatic accretion. The influence of diffuse plate boundary zone on the young seafloor fabric generated by the CIR has been examined. The seafloor topography different from the normal ridge parallel fabric observed at few places over the NE flank of the CIR is suggested to be the consequence of gradual and progressive influence of the distributed diffuse plate boundary (between the Indian-Capricorn plates), on the newly generated oceanic lithosphere. Further, we documented distinct ridge-transform intersection (RTI) highs, three of these RTI highs are identified as oceanic core complexes/megamullion structures. Megamullion structures are found to be associated with less magmatic sections. Increased seismicity has been observed at the less magmatic segment ends suggesting the predominance of tectonic extension prevalent at the sparsely magmatic sections.
机译:利用多波束测深和磁数据研究了印度洋在3°S和11°S纬度之间长750. km的中印度洋脊(CIR)的分割模式。识别出十二个脊段,这些脊段被定义良好的转换断层和非转换间断所分隔。磁性模型研究将脊定为缓慢扩张的脊,平均平均扩张速率在26至38. mm / yr之间。磁异常的位置表明板的打开方向在最后的0-4期间没有变化。马时期。沿着磁异常中的轴变化,内谷底存在轴向火山脊,裂谷的深度和几何形状的变化表明沿该脊的增生过程有明显的变化。根据这些特征和分割模式,我们认为十个脊段正经历较少的岩浆伸展阶段,而两个段则显示出岩浆增生的特征。具有狭窄和浅谷底裂谷和接近对称磁异常的线性段被识别为具有岩浆增生的段。研究了扩散板边界区对CIR生成的年轻海底织物的影响。海平面形貌不同于在CIR的NE侧面上的几个地方观察到的正常脊平行结构,这是由于散布的板块边界(印度-摩ri座板块之间)对新近分布的渐进影响的结果。生成的海洋岩石圈。此外,我们记录了不同的岭变换相交(RTI)高点,其中这些RTI高点中的三个被确定为海洋核心复合体/巨型竖框结构。发现巨型竖框结构与较少的岩浆剖面有关。在较少的岩浆段末端观察到地震活动性增加,这表明在稀疏的岩浆段普遍存在构造扩展。

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