spreading ridges is increasingly controlled by the uprising
asthenosphere. This is visible in their morphology and
their large-scale tectonics. There is some evidence from
ophiolites (Nicolas et al., 1999) and slow spreading ridges,
based on seismic anisotropy (Li and Detrick, 2003;
Nowacki et al., 2012), suggesting that mantle flow is ridge
parallel and not more ridge perpendicular. As discussed
above, ultraslow ridge morphology and crustal composition respond to variations in mantle upwelling and associated melt delivery.
The combined study of ophiolites and geophysical data
at oceanic ridges has allowed to comprehend the inner
working of ocean spreading processes. The ophiolites
allowed us to image deep accreted lithosphere and, indirectly, to investigate accretion processes, whereas the geophysics provide direct images of the accreting ridge
systems. These observations showed that these accreting
systems are different depending firstly on spreading rates
and sometimes displaying significant variations along
the same segment of a ridge axis. For example, along the
most studied 9
N segment of the EPR, the width of the
AML changes significantly and so does the melt-mush
distribution along the ridge axis. Along slow spreading
ridges, the crust is normally thickest at the center of a segment and thinnest at segment ends. The crustal accretion
process at slow spreading centers is further complicated
by the presence of ocean core complexes, which are not
just present at segment ends, but could be present along
a significant part of a segment (Escartin et al., 2008).
The ultraslow spreading ridges, a special class of ridges,
show extreme variations in seafloor morphology, crustal
thickness, and geochemistry; more geophysical studies
of ultraslow spreading ridges are required to fully appreciate the diversity of ridge processes on earth.
Acknowledgments
We would like to thank F. Boudier and M. Cannat for fruitful discussions and M.R. Perfit for a very comprehensive
and thoughtful review.
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