Upper mantle structure beneath the Hawaiian swell: Constraints from the ocean seismic network pilot experiment

被引:40
作者
Collins, JA [1 ]
Vernon, FL
Orcutt, JA
Stephen, RA
机构
[1] Woods Hole Oceanog Inst, Dept Geol & Geophys, Woods Hole, MA 02543 USA
[2] Univ Calif San Diego, Scripps Inst Oceanog, Cecil H & Ida M Green Inst Geophys & Planetary Ph, La Jolla, CA 92093 USA
关键词
D O I
10.1029/2001GL013302
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
[1] Data from two broadband, ocean-bottom seismographic stations deployed similar to 225 km southwest of Oahu, Hawaii during the Ocean Seismic Network Pilot Experiment provide constraints on upper mantle structure beneath the Hawaiian swell. Receiver functions show that the mantle transition zone is thinned by >50 km relative to reference model PA5, which, in the absence of compositional changes, implies excess temperatures of >350 K in the transition zone. The combination of the measurements reported here and the thickness variations reported by Li et al. [2000] imply that the transition zone is thinned by 30 +/- 15 km over an along-swell dimension of at least 700 km. At similar to80 km depth, P-to-S converted phases are identified from the Gutenberg discontinuity marking the lid of the oceanic low-velocity zone and the base of the lithosphere. Shear-wave splitting measurements imply that fast-polarization azimuths are intermediate between the absolute plate-motion vector and the fossil spreading direction; multi-event stacked values of o and deltat are -80degrees and 1.5 s, respectively.
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页码:17 / 1
页数:4
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