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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