Seismic structure of the mantle ; from subduction zone to craton
Publication date
1998
Authors
Kennett, B.L.N.
Hilst, R.D. van der
Editors
Advisors
Supervisors
DOI
Document Type
Part of book or chapter of book
Metadata
Show full item recordCollections
License
Abstract
Seismological techniques have provided much of the currently available information
on the internal structure of the Earth, and in particular on the mantle. Early
studies revealed the need for an increase in seismic velocity with depth in the Earth,
and by 1915 Gutenberg was able to make a good estimate of the radius of the core.
Knowledge of the Earth's internal structure was refined by iterative improvement of
earthquake locations and the travel times for seismic phases through the Earth, so
that in 1940 Jeffreys and Bullen were able to publish an extensive set of travel-time
tables based on a model of both P-wave and S-wave velocities in the mantle. Their
velocity profile was intentionally as smooth as possible, but it was not possible to
avoid introducing a sharp change in velocity gradient near a depth of 400 km to
account for the distinct change in the slope of travel-time curves at a distance of
approximately 20' from the source, for both P and S waves. Subsequent studies
have refined our conception of mantle structure to reveal the presence of discontinuities
in velocity and zones of strong velocity gradients, which have been correlated
with mineralogical phase changes.