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A multichannel seismic study of lithospheric flexure across the Hawaiian–Emperor seamount chain

Nature volume 315, pages 105–111 (1985)Cite this article

Abstract

Existing models assume that the thickened crust beneath seamounts is the result of a surface volcanic load flexing an elastic plate. New results suggest that flexed oceanic crust beneath the Hawaiian–Emperor seamount chain is underlain by a 4-km thick deep crustal body. We intepret the body as a deep crustal sill complex associated with the tholeiitic stage of volcano building along the chain.

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Authors and Affiliations

  1. Lament-Doherty Geological Observatory, Columbia University, Palisades, New York, 10964, USA

    P. Buhl

  2. Department of Geological Sciences, Columbia University, Palisades, New York, 10964, USA

    A. B. Watts & U. S. ten Brink

  3. Woods Hole Oceanographic Institution, Woods Hole, Massachusetts, 02543, USA

    T. M. Brocher

Authors
  1. A. B. Watts
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  2. U. S. ten Brink
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  3. P. Buhl
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  4. T. M. Brocher
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Watts, A., ten Brink, U., Buhl, P. et al. A multichannel seismic study of lithospheric flexure across the Hawaiian–Emperor seamount chain. Nature 315, 105–111 (1985). https://doi.org/10.1038/315105a0

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