Description Usage Arguments Details Value Author(s) See Also Examples
Determine arrival times and information for all major phases arriving at a certain epicentral distance, and plot ray trajectories.
1 2 | DistSummary(delta, h, model, phaselist = 'default', prop = "vp",
image.col = heat.colors(500), n = 200, ...)
|
delta |
Epicentral distance (degrees) |
h |
Focal depth (km) |
model |
Planet model |
phaselist |
Either 'default' for all available phases, or a character vector including desired phases |
prop |
Property by which to scale planet image: one of 'vp', 'vs', 'rho'. |
image.col |
Vector of colors for image |
n |
Resolution of image (pixels per side) |
... |
Other parameters for Rayfan |
This function is really just a wrapper for Rayfan to calculate arrivals for many phases at just one epicentral distance. Since each phase must be calculated separately, the use of the default phaselist will result in a long calculation time (minutes), and the plot will probably be crowded. It is generally better to define phaselist as a smaller vector or use Rayfan instead.
Returns a list with the following elements:
p |
Ray parameter for each arrival |
t |
Travel time for each arrival |
dist |
Epicentral distance (should be approximately the input dist) |
phase |
Phase of each arrival |
Jake Anderson
Rayfan, Traveltime, Earthplot
1 2 3 4 5 |
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