Record Details

Heat flow on hot spot swells: Evidence for fluid flow

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Field Value
Title Heat flow on hot spot swells: Evidence for fluid flow
Names Harris, Robert N. (creator)
McNutt, Marcia K. (creator)
Date Issued 2007-03-23 (iso8601)
Note Copyrighted by American Geophysical Union.
Abstract We examine variability observed in heat flow determinations collected on hot spot
swells. We find substantial scatter in heat flow at wavelengths of a few hundred kilometers
and less at both Hawaii and Reunion, where closely spaced data exist, and large variability
in the regional heat flow surveys at Cape Verde, Bermuda, and Crozet. Our preferred
interpretation is that the observed variability is due to fluid flow. The presence of fluid
flow admits the possibility that some heat is lost through advection such that the mean
observed heat flow is less than the actual mantle flux. If so, the full magnitude of
sublithospheric thermal variations may not be observed. This interpretation has important
implications for understanding heat flow determinations made on hot spot swells and
resulting geodynamic inferences. We suggest fluid flow may be masking variations in
sublithospheric heat flux making available surface heat flow values a poor discriminator
between geodynamic models for hot spot swells. Future field programs, methods of data
analysis, and models should be designed to help extract a low-frequency mantle flux
disguised by a high-noise surface filter.
Genre Article
Topic heat flow
Identifier Harris , R. N. and M. K. McNutt (2007), Heat flow on hot spot swells: Evidence for fluid flow, J. Geophys. Res., 112, B03407.

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