Changes between Version 29 and Version 30 of CollidingFlows

Timestamp:

11/23/11 17:19:50 (13 years ago)

Author:

Jonathan

Comment:

—

CollidingFlows

@@ -27 +27 @@
 ||   || [[Image(20_30_big.png, width=400)]] || || ||
 
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 === Mixing Histograms ===
 || ||  20 pc  ||  40 pc  ||  60 pc  ||
@@ -36 +78 @@
 
 
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 === Fixed a few bugs and added multipole expansion for phi ===
   Previously only the first particle did any accreting.  Successive particles remained massless
@@ -45 +128 @@
 
 
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 Here's the mixing ratio histogram both volume weighted (red) and mass weighted (blue) for the various resolutions at a constant time (before the first particle forms).  Note that the particles form at frame 13 for the lowest resolution run, and then at frames 14, 15, & 16 as the resolution increases.  The brighter color the higher the resolution.  Notice that the lower resolution has larger bins because there are few data points to sample.  In general the number of bins is proportional to the resolution (and not the number of cells as might be expected).  This is because the structure that develops and the region containing non-zero mixing ratios is essentially 1D.
 
@@ -50 +163 @@
 ||  [[Image(40_15_mix_hist.png, width=600)]]  ||
 
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+Also looked at 2D PDFs of Density and Pressure as well as Density vs Mixing (Upper left and lower right are mass weighted, while lower left and upper right are volume weighted)
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+||  Log Density vs. Log Pressure   ||   Log Density vs. Mixing  ||
+||  [attachment:40_15_densPress_PDF.gif movie]  ||  [attachment:40_15_densMixing_PDF.gif movie]  ||
+|| [[Image(40_15_densPress_PDF.png, width=400)]]  ||  [[Image(40_15_densMixing_PDF.png, width=400)]] ||