Planet model using the data from the ak135 1-D model.
Usage
data(model)
Arguments
Format
List with following elements:
z
Sample depths (km)
vp
Sample P wave velocities (km/s)
vs
Sample S wave velocities (km/s)
rho
Sample densities (kg/m^3)
qp
P attenuation
qs
S attenuation
name
Model name
rp
Planet radius
year
Year published
conr
Depth to Conrad (upper crust/lower crust) discontinuity
moho
Depth to Mohorovicic (top of mantle) discontinuity
d410
Depth to top of transition zone
d520
Depth to olivine beta-gamma transition
d660
Depth to top of lower mantle
cmb
Depth to core-mantle boundary
icb
Depth to inner core boundary
References
Kennett, B.L.N. Engdahl, E.R. & Buland R., 1995. Constraints on
seismic velocities in the Earth from travel times, Geophys J Int, 122,
108-124 <doi:10.1111/j.1365-246X.1995.tb03540.x>