首页> 外文期刊>Journal of geophysical research. Solid earth: JGR >Deep-sea magnetic vector anomalies over the Hakurei hydrothermal field and the Bayonnaise knoll caldera, Izu-Ogasawara arc, Japan
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Deep-sea magnetic vector anomalies over the Hakurei hydrothermal field and the Bayonnaise knoll caldera, Izu-Ogasawara arc, Japan

机译:日本伊豆小gas原弧的羽田热液场和贝纳瓦兹峰破火山口的深海磁矢量异常

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[1] We conducted deep-sea magnetic measurements using autonomous underwater vehicles in the Bayonnaise knoll caldera, the Izu-Ogasawara island arc, which hosts the large Hakurei hydrothermal field. We improved the conventional correction method applied for removing the effect of vehicle magnetization, thus greatly enhancing the precision of the resulting vector anomalies. The magnetization distribution obtained from the vector anomaly data shows a~2 km wide belt of high magnetization, trending NNW-SSE going through the caldera, and a low-magnetization zone~300 m by ~500 m in area, extending over the Hakurei site. Comparison between the results obtained using the vector anomaly and the total intensity anomaly shows that the magnetic field is determined more accurately, especially in areas of sparse data distribution, when the vector anomaly rather than the total intensity anomaly is used. We suggest a geologically motivated model that basaltic volcanism associated with the back-arc rifting occurred after the formation of the caldera, resulting in the formation of the high-magnetization belt underneath the silicic caldera. The Hakurei hydrothermal field lies in the intersection of the basaltic volcanism belt and the caldera wall fault, suggesting a mechanism that hot water generated by the heat of the volcanic activity has been spouting out through the caldera wall fault. The deposit apparently extends beyond the low-magnetization zone, climbing up the caldera wall. This may indicate that hot water rising from the deep through the alteration zone is transported laterally when it comes near the seafloor along fissures and fractures in the caldera wall.
机译:[1]我们在拥有大型Hakurei热液场的伊豆岛-小gas原岛弧线上的Bayonnaise丘陵破火山口中使用水下自动驾驶仪进行了深海磁场测量。我们改进了用于消除车辆磁化影响的常规校正方法,从而大大提高了产生的矢量异常的精度。从矢量异常数据获得的磁化分布显示,高磁化带宽约2 km,NNW-SSE穿过火山口,低磁化带约300 m,约500 m,延伸到了Hakurei站点。使用矢量异常和总强度异常获得的结果之间的比较表明,当使用矢量异常而不是总强度异常时,可以更准确地确定磁场,尤其是在稀疏数据分布区域。我们建议采用地质动机模型,在破火山口形成后发生与后弧裂谷有关的玄武质火山作用,从而导致硅质破火山口下方形成高磁化带。 Hakurei热液场位于玄武质火山岩带和破火山口壁断层的交汇处,这表明由火山活动热产生的热水已经通过破火山口壁断层喷出。沉积物显然延伸到低磁化区域以外,攀爬了火山口壁。这可能表明,从深处穿过变化带上升的热水在靠近海床时沿着火山口壁的裂缝和裂缝横向输送。

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