On the role of surface tension in the migration of melts and fluids
- Creators
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Stevenson, D. J.
Abstract
It is shown that surface tension can cause redistribution of melt in a partially molten medium, in accordance with a non-linear diffusion equation for the melt fraction. The associated diffusivity D depends on the surface energy and is positive (stable) for dihedral angle <60° and negative (unstable) for dihedral angle >60°. In the more likely stable case, D ∼ 10^(−7) cm^2 .s^(−1) is typical for mantle melts, but a value as high as 10^(−1) cm^2 .s^(−1) is conceivable for volatile-rich fluids. Surface tension may play an important role in creating pathways for meta-somatizing fluids in the Earth, but does not appear likely to affect substantially the existing estimates of large scale melt migration (e.g., beneath mid-ocean ridges).
Additional Information
© 1986 by the American Geophysical Union. Received July 31, 1986; accepted August 26, 1986. I had helpful discussions or correspondence with D.R. Scott, E.B. Watson, and N. von Bargen. Supported by NSF grant EAR-8418353. Contribution number 4358 from the Division of Geological and Planetary Sciences, California InstituteAttached Files
Published - grl3347.pdf
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Additional details
- Eprint ID
- 41945
- Resolver ID
- CaltechAUTHORS:20131016-110233873
- NSF
- EAR-8418353
- Created
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2013-10-16Created from EPrint's datestamp field
- Updated
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2021-11-10Created from EPrint's last_modified field
- Caltech groups
- Division of Geological and Planetary Sciences (GPS)
- Other Numbering System Name
- Caltech Division of Geological and Planetary Sciences
- Other Numbering System Identifier
- 4358