Hawaii Institute of Geophysics and Planetology, University of Hawaii at Manoa, Honolulu, HI 96822, USA.
Science. 2009 Dec 4;326(5958):1388-90. doi: 10.1126/science.1180165.
Defining the mantle structure that lies beneath hot spots is important for revealing their depth of origin. Three-dimensional images of shear-wave velocity beneath the Hawaiian Islands, obtained from a network of sea-floor and land seismometers, show an upper-mantle low-velocity anomaly that is elongated in the direction of the island chain and surrounded by a parabola-shaped high-velocity anomaly. Low velocities continue downward to the mantle transition zone between 410 and 660 kilometers depth, a result that is in agreement with prior observations of transition-zone thinning. The inclusion of SKS observations extends the resolution downward to a depth of 1500 kilometers and reveals a several-hundred-kilometer-wide region of low velocities beneath and southeast of Hawaii. These images suggest that the Hawaiian hot spot is the result of an upwelling high-temperature plume from the lower mantle.
确定位于热点下方的地幔结构对于揭示其起源深度非常重要。通过海床和陆地地震仪网络获得的夏威夷群岛下方横波速度的三维图像显示,上地幔低速异常呈链状延伸,周围环绕着抛物线形的高速异常。低速一直延伸到 410 到 660 公里深度的地幔转换带,这一结果与先前观察到的转换带变薄的结果一致。SKS 观测结果的加入将分辨率向下扩展到 1500 公里深度,并揭示了夏威夷下方和东南部几百公里宽的低速区域。这些图像表明,夏威夷热点是来自下地幔的上升高温羽流的结果。