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Volumn 281, Issue 5376, 1998, Pages 546-549

A correlation between ultra-low basal velocities in the mantle and hot spots

Author keywords

[No Author keywords available]

Indexed keywords

CORE-MANTLE BOUNDARY; HOT SPOT; LOW VELOCITY ZONE; LOWER MANTLE; SEISMIC TOMOGRAPHY;

EID: 0032563135     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.281.5376.546     Document Type: Article
Times cited : (155)

References (43)
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    • In constructing Fig. 1, we incorporated only those ray paths for which anomalous diffracted P-wave segments of the seismic phase SPdKS could be resolved to lie on either the source or receiver side of the ray path, as derived from different paths containing overlapping diffracted segments (9, 12). The lateral extent of ULVZs was determined by standard Fresnel zone analysis (19) including all regions sampled within the first quarter period. Varying the assumed size of the Fresnel zone affected our statistical correlations, with smaller and larger zones producing somewhat worse correlations between hot spots and the ULVZs. Nevertheless, ULVZs are better correlated with hot spot flux than any contours within tomographic velocity models of the deep mantle (4, 19) for Fresnel zone dimensions between one-eighth and one-half wavelength.
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    • Standardized score (z) is defined as z = (O - E)/σ, where O is the number of hot spots (or flux) inside a velocity contour for a randomly sampled 44% of the tomographic models, E denotes the number (or flux) predicted by a binomial distribution, and σ is the standard deviation of the binomial. Zero corresponds to uncorrelated data; z ≥ 1.0 has an ∼15% likelihood of arising randomly.
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    • Supported by the NSF Geophysics and Presidential Faculty Fellow programs. We thank H. Nataf and the reviewers for comments on the manuscript.


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