The program  

read.mk12wm13.f

is a fortran program that asks you for the coordinates and depth of 
a point in the mantle and gives you as output percent perturbation 
in mu over rho, kappa over rho, bulk sound velocity, S velocity, 
P velocity, as predicted by MK12WM13 (Su and Dziewonski, PEPI 1997).
You can compile it by simply doing f77 read.mk12wm13.f

mk12wm13_kappa.dat

and
 
mk12wm13_mu.dat

are just the MK12WM13 model.

Please note that these .dat files contain the spherical harmonic
coefficients of our images of relative (not percent) perturbations
in kappa/rho and mu/rho (not S). Our definition of spherical harmonics is
given in the fortran program read.mk12wm13.f provided here.


foanis05.mod is PREM and velpert.h is a header file that accompanies
read.mk12wm13.f
