Open lynlyf opened 5 hours ago
Yes, it should work but may require using the "nd" format as tvel doesn't let you specify layer boundaries. Just let bottom of mantle be same as radius of planet for no core and leave out liquid outer core if not needed.
For example:
0.000 6.2000 3.7000 3.3198
35.000 6.2000 3.7000 3.3198
mantle
35.000 8.2000 4.7000 3.3198
2889.000 13.6908 7.3015 5.5515
outer-core
inner-core
2889.000 11.0914 3.4385 12.7037
6371.000 11.2409 3.5645 13.0122
Phase naming is still the same, but with a solid core you would use S
for mantle only S waves and SJS
for S waves crossing into the (inner) core.
For example:
taup time --mod noOuterCore.nd -ph S,SJS -deg 35
Model: noOuterCore
Distance Depth Phase Travel Ray Param Takeoff Incident Purist Purist
(deg) (km) Name Time (s) p (s/deg) (deg) (deg) Distance Name
-----------------------------------------------------------------------------------
35.00 0.0 S 781.38 19.120 39.51 39.51 35.00 = S
taup time --mod noOuterCore.nd -ph S,SJS -deg 170
Model: noOuterCore
Distance Depth Phase Travel Ray Param Takeoff Incident Purist Purist
(deg) (km) Name Time (s) p (s/deg) (deg) (deg) Distance Name
-----------------------------------------------------------------------------------
170.00 0.0 SJS 3076.87 7.983 15.40 15.40 190.00 = SJS
Hello,
Can Taup calculate travel time and ray parameter tables and wavefronts for models having no core? For example, the simplest case, a homogeneous sphere.
And how to calculate time table for phases with S legs in models with a solid core, since there is no such naming convention in the FDSN standard?
Thanks.