SB4L18 shows the typical features commonly found in mantle tomographic models:
SB10L18 shows some interesting features that can be found in other joint models as
well:
S16B30 is basically a smoothed version of SB4L18 as these models correlate very well,
except in the transition zone (picture).
The rms amplitudes in P16B30 vary very much like those of Vp in SB10L18 with depth
though the correlation of these models is not quite as good as between
S16B30 and SB4L18.
(picture).
Models SB4L18 and SB10L18 are described in:
Masters G., Laske, G., Bolton, H. and Dziewonski, A., 2000.
"The Relative Behavior of Shear Velocity, Bulk Sound Speed, and Compressional
Velocity in the Mantle: Implications for Chemical and Thermal Structure"
in: S. Karato, A.M. Forte, R.C. Liebermann, G. Masters and L. Stixrude (eds.)
"Earth's Deep Interior", AGU Monograph 117, AGU, Washington D.C.
Model S16B30 is described in:
Masters, G., Johnson, S., Laske, G. and Bolton H., A shear-velocity model
of the mantle. Phil. Trans. R. Soc. Lond. A, 354, 1385-1411, 1996.
Model P16B30 is described in:
Bolton H., Long Period Travel Times and the Structure of the Mantle.
PhD Thesis, La Jolla, 204 pages, 1996.
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