INTERFACIAL TURBULENT MIXING IN STRATIFIED MAGMA RESERVOIRS

Citation
Sss. Cardoso et Aw. Woods, INTERFACIAL TURBULENT MIXING IN STRATIFIED MAGMA RESERVOIRS, Journal of volcanology and geothermal research, 73(3-4), 1996, pp. 157-175
Citations number
59
Categorie Soggetti
Geosciences, Interdisciplinary
ISSN journal
03770273
Volume
73
Issue
3-4
Year of publication
1996
Pages
157 - 175
Database
ISI
SICI code
0377-0273(1996)73:3-4<157:ITMISM>2.0.ZU;2-S
Abstract
We analyse the interfacial turbulent mixing of molten magmas in a two- layer stratified convecting magma chamber. We examine situations where convection is driven by the heat and/or compositional flux associated with the melting of a solid boundary. The model applies to the case i n which the Rayleigh number is sufficiently large that the effect of a viscosity difference on turbulent entrainment is negligible and so th e model predictions represent an upper bound for interfacial mixing. O ur results suggest that the extent of mixing induced by the thermal bu oyancy flux is relatively small. However, the compositional buoyancy f luxes associated with phase change may be much larger and the mixing t hey induce may significantly affect the evolution of the reservoir. Ou r analysis of the melting of the floor of a two-layer stratified magma chamber shows that turbulent mixing at the interface between the two magmas may suppress the melting, and decrease the final amount of melt produced when the system reaches thermal equilibrium. It is also show n that, although floor melting tends to decrease the density of the lo wer layer of magma, somewhat counterintuitively, turbulent interfacial mixing with the overlying layer of smaller density may inhibit large scale overturn and preserve the stratified state of the chamber. In th e case in which both the floor and roof of a chamber melt, turbulent m ixing at the interface between the newly formed light melt at the roof and the lower layer of dense magma induces a shift of the melting pro cess from the floor to the roof. For typical parameter values in a bas altic magma chamber, we estimate that under conditions of very large R ayleigh number, the amount of crustal melt produced al the roof may be as high as 50% of that produced at the floor.