# Thermal impact of magmatism in subduction zones

**Authors:** David W. Rees Jones, Richard F. Katz, Meng Tian, and John F. Rudge

arXiv: 1701.02550 · 2017-11-22

## TL;DR

This paper demonstrates that magma transport significantly influences the thermal structure of subduction zones, explaining observed heat flow and temperature discrepancies with traditional models, and affecting volcanic activity.

## Contribution

It introduces numerical models showing magma transport's role in altering subduction zone thermal structures, resolving previous temperature prediction discrepancies.

## Key findings

- Magma transport raises local temperatures by ~300 K.
- Heat transported by magma explains higher observed heat flow.
- Magma advection dominates latent heat deposition.

## Abstract

Magmatism in subduction zones builds continental crust and causes most of Earth's subaerial volcanism. The production rate and composition of magmas are controlled by the thermal structure of subduction zones. A range of geochemical and heat flow evidence has recently converged to indicate that subduction zones are hotter at lithospheric depths beneath the arc than predicted by canonical thermomechanical models, which neglect magmatism. We show that this discrepancy can be resolved by consideration of the heat transported by magma. In our one- and two-dimensional numerical models and scaling analysis, magmatic transport of sensible and latent heat locally alters the thermal structure of canonical models by $\sim$300 K, increasing predicted surface heat flow and mid-lithospheric temperatures to observed values. We find the advection of sensible heat to be larger than the deposition of latent heat. Based on these results we conclude that thermal transport by magma migration affects the chemistry and the location of arc volcanoes.

## Full text

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## Figures

13 figures with captions in the complete paper: https://tomesphere.com/paper/1701.02550/full.md

## References

36 references — full list in the complete paper: https://tomesphere.com/paper/1701.02550/full.md

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Source: https://tomesphere.com/paper/1701.02550