How does small-scale convection manifest in surface heat flux?
Small-scale convection in the suboceanic mantle, if present, is commonly thought to manifest in surface heat flux, and the steady-state scaling of sublithospheric convection has often been used to interpret heat flow data from old ocean basins. Relations among small-scale convection, surface heat fl...
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Published in | Earth and planetary science letters Vol. 287; no. 3; pp. 329 - 332 |
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Main Author | |
Format | Journal Article |
Language | English |
Published |
Elsevier B.V
15.10.2009
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Subjects | |
Online Access | Get full text |
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Summary: | Small-scale convection in the suboceanic mantle, if present, is commonly thought to manifest in surface heat flux, and the steady-state scaling of sublithospheric convection has often been used to interpret heat flow data from old ocean basins. Relations among small-scale convection, surface heat flux, and the steady-state scaling, however, have been vague. A series of transient cooling modeling are conducted here to quantify such relations. Given the strong temperature-dependency of mantle viscosity, results suggest that small-scale convection could take place without noticeably disturbing surface heat flux, and that the use of steady-state scaling may not be warranted for the present-day suboceanic mantle. |
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Bibliography: | ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 23 ObjectType-Article-2 ObjectType-Feature-1 |
ISSN: | 0012-821X 1385-013X |
DOI: | 10.1016/j.epsl.2009.08.015 |