A mantle wedge is a triangular shaped piece of mantle that lies above a Subduction tectonic plate and below the overriding plate. This piece of mantle can be identified using seismic velocity imaging as well as earthquake maps.
Water in mantle wedge
Magmas produced in subduction zone regions have high volatile contents. This water is derived from the breakdown of hydrous minerals in the subducting slab, as well as water in the oceanic plate from
percolation of seawater. This water rises from the subducting slab to the overriding mantle wedge. The water lowers the melting temperature of the wedge and leaves behind melt inclusions that can be measured in the associated arc volcanic rocks.
Structure of the mantle wedge
The
forearc mantle extends from where the subducting slab meets the cold nose of the mantle wedge, this occurs at depths from 10–40 km.
Low seismic attenuation, and high seismic velocities characterize this region. There is a boundary between this low attenuation region and a high attenuation region on the forearc side of the arc volcanoes.
To image the mantle wedge region below volcanic arcs P-wave, S-wave and seismic attenuation images should be used in coordination. These tomographic images show a low velocity, high attenuation region above the subducting slab. The slowest velocities in these volcanic arc regions are Vp= 7.4 km·s
−1 and Vs= 4 km·s
−1.
Mantle wedge regions that do not have associated arc volcanism do not show such low velocities. This can be attributed to the melt production in the mantle wedge.
Mantle wedge flow
Flow in mantle wedges has important effects on the thermal structure, overall mantle circulation and melt within the wedge.
are
anisotropic and have the ability to align themselves within the mantle when exposed to strain.
These mineral alignments can be seen using
seismic imaging, as waves will travel through different orientations of a mineral at different speeds.
Shear strain associated with mantle flow will align the
fast direction of
pyroxene and
olivine grains in the direction of flow. This is the most common theory on flow within the mantle, although opposing theories do exist (6). Flow within the mantle wedge is parallel to the crust until it reaches the relatively cooler nose of the wedge, then is overturned and is parallel to the subducting slab. The nose of the wedge is generally isolated from the overall mantle flow.
Oxidation in the mantle wedge
Studies have shown that
that produce island arcs are more
oxidized than the magmas that are produced at
mid-ocean ridges. This relative degree of oxidation has been determined by the iron oxidation state of
fluid inclusions in glassy volcanic rocks. It has been determined that this state of oxidation is correlated with the water content of the mantle wedge. Water itself is a poor oxidant and therefore the oxidizing agent must be transported as a dissolved ion in subducting slab.
