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Distribution and Origin of Seamounts in the Central Indian Ocean Basin

机译:中印度洋海盆海山的分布与起源

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Approximately 200 seamounts of different dimensions have been Identified, from multi-beam bathymetry maps of the Central Indian Ocean Basin (CIOB) (9°S to 16°S and 72°E to 80°E), of which 61% form eight chains that trend N-S. The seamounts are clustered above and below 12°S latitude. Area II (9°-12°S) shows a concentration of smaller seamounts (≤ 400 m height), and area I (12°-15°S) has a mixed population (including both less and more than 400 m height). Inspite of the differences in their height, the seamounts of these eight chains are morphologically (slope angle, flatness, basal width) corelatable. Furthermore, we suggest that height-width ratio could be useful in identifying the style of seamount eruption. The seamount chains in the CIOB probably originated frompropagative fractures and were produced between 61 and 52 Ma (chrons A26 to A23) as a result of the interaction between the conjugate crusts of the Central Indian and Southeast Indian Ridges during the Indo-Eurasian collision event.
机译:从中印度洋海盆(CIOB)的多波束测深图(9°S到16°S和72°E到80°E)中,已经识别出大约200个不同尺寸的海山。趋势NS。海山聚集在12°S纬度以上和以下。 II区(9°-12°S)显示出较小的海山(≤400 m高),而I区(12°-15°S)则具有混合种群(包括小于和大于400 m的高度)。尽管它们的高度有所不同,但是这八条链的海山在形态上(坡度,平坦度,基部宽度)是可定型的。此外,我们建议高宽比可能有助于识别海山喷发的样式。 CIOB中的海山链可能起源于传播性裂缝,是由于印度-欧亚碰撞事件期间中印度洋脊和东南印度洋脊的共轭壳之间相互作用而产生的,在61至52 Ma(A26至A23年代)之间产生。

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