2018
DOI: 10.1130/ges01660.1
|View full text |Cite
|
Sign up to set email alerts
|

Effects of fluid influx, fluid viscosity, and fluid density on fluid migration in the mantle wedge and their implications for hydrous melting

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
3
1
1

Citation Types

0
22
0

Year Published

2019
2019
2023
2023

Publication Types

Select...
6
1

Relationship

0
7

Authors

Journals

citations
Cited by 24 publications
(22 citation statements)
references
References 90 publications
0
22
0
Order By: Relevance
“…It is under this assumption that the up‐slab flows in Figure are necessary to produce the melt feeding arc volcanism. However, two‐phase geodynamic models of the mantle wedge suggest that the melt and fluid transport through the wedge is more complex than simply vertical, and depends on many factors including solid rheology and grain size in the wedge (Cerpa et al, , ; Wilson et al, ). In addition, the coincidence of flux peaks and the projected volcanic arc position in Figures and is premised on the hot thermal structure of the 10 Ma slab.…”
Section: Discussionmentioning
confidence: 99%
“…It is under this assumption that the up‐slab flows in Figure are necessary to produce the melt feeding arc volcanism. However, two‐phase geodynamic models of the mantle wedge suggest that the melt and fluid transport through the wedge is more complex than simply vertical, and depends on many factors including solid rheology and grain size in the wedge (Cerpa et al, , ; Wilson et al, ). In addition, the coincidence of flux peaks and the projected volcanic arc position in Figures and is premised on the hot thermal structure of the 10 Ma slab.…”
Section: Discussionmentioning
confidence: 99%
“…At shallow depths, the low permeability due to the small grain size at the base of the mantle wedge causes trapped aqueous fluid to be entrained toward the sub‐arc mantle, where the enlarged grain size leads to a relatively high permeability (Cerpa et al, 2017). The temperature‐dependent viscosity of the aqueous fluid results in a similar effect of the grain size evolution; high‐viscosity aqueous fluid is trapped at the base of the mantle wedge and dragged into the sub‐arc mantle (Cerpa et al, 2018). The effect of dynamic pressure on aqueous fluid flow may be minor for the low viscosity of the mantle wedge (Cerpa et al, 2018).…”
Section: Discussionmentioning
confidence: 99%
“…The temperature‐dependent viscosity of the aqueous fluid results in a similar effect of the grain size evolution; high‐viscosity aqueous fluid is trapped at the base of the mantle wedge and dragged into the sub‐arc mantle (Cerpa et al, 2018). The effect of dynamic pressure on aqueous fluid flow may be minor for the low viscosity of the mantle wedge (Cerpa et al, 2018). Wilson et al (2014) showed that the compaction pressure deflects aqueous fluid in the back‐arc mantle toward the sub‐arc mantle.…”
Section: Discussionmentioning
confidence: 99%
See 2 more Smart Citations