Glacial update for non-vertical rays #3
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Glacial update
Should be 'quiet' not 'silent'
Rather than calculating the isotropic velcoty from the isotropic component of the poly-xtal anisotropic tensor (the norm of which changes with texture) use simple VRH mean of the single xtal tensor. This gives values that are just a function of the temperature and do not vary with texture. Also split the velocity graph into two graphs.
Choose the format based on the first word in the first line of the EBSD files. Data is the same in both, but colomn order changes.
These are still straight but have a inclination that is not 90 degrees. Plot as a function of source polrization (otherwise we end up with chaos as we sweep around the azimuth) and inclnation for different azimuths. Some cleanup is needed.
If 'fname' is a real (rather than a string) write to that assuming it is an fid (and avoid opening a new file). In this case the file is not closed prior to exiting MS_save. This can be used when either several Cijs must be written to the same file or to create parts of larger reports. Note that 'fname' = 1 will write data to the terminal.
Create an input file for MODSIMPLE - a model builder for the ATRAK anisotropic ray tracer.
Aparanlty we had the wrong units for modsimple. According to Mike this is correct.
Add these to the summary plot. We should probably refactor MS_plot and make this an MS_summary or something.
These should correspond to SKS, local events and icequakes.
We do not need a depth for the top of the model - so just print the depth, not zero.
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These commits fix a number of issues and introduce the calculation of effective splitting for non-vertical rays. Specifically they: