Planet model using the data from the IASP91 1-D model.
Usage
data(iasp91)
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
Kennet BLN, Engdahl ER, 1991. Traveltimes for global earthquake
location and phase identification. Geophysical Journal International
105(2) 429-465. doi:10.1111/j.1365-246X.1991.tb06724.x