Changes between Version 13 and Version 14 of u/madams/3DCDMVisualizationInstructions
- Timestamp:
- 10/09/14 11:49:17 (10 years ago)
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u/madams/3DCDMVisualizationInstructions
v13 v14 63 63 = Projecting Sinks = 64 64 65 Given that our data deals with colliding flows and how their interaction can induce star formation, it is pert ainent that we discuss the formation of sink particles. To learn more about sink particles, see Fedderath et al. in [https://astrobear.pas.rochester.edu/trac/wiki/u/EricasLibrary#no2 Erica's Library]. Here we present two ways of projecting the sinkonto a bov.65 Given that our data deals with colliding flows and how their interaction can induce star formation, it is pertinent to discuss the formation of sink particles. To learn more about sink particles, see Fedderath et al. in [https://astrobear.pas.rochester.edu/trac/wiki/u/EricasLibrary#no2 Erica's Library]. Here we present two ways of projecting and aligning the sink particles onto a bov. 66 66 67 67 == Using Chombos == 68 68 == Using a Script == 69 The script used (okc_to_curve.sh) can be found in the attachments below, along with the original sink file and its three projections.69 The script used (okc_to_curve.sh) can be found in the attachments below, along with the original sink file for frame 0 and its three projections. To run the script, copy it into your run directory with the .okc files and execute it. Immediately new curve files should be produced. With this method we simply plot the sinks as a curve file instead of as a pseudocolor variable inherent in the chombo (pmass).