Changes between Version 56 and Version 57 of u/BonnorEbertMatched

Timestamp:

06/26/12 11:22:52 (12 years ago)

Author:

Erica Kaminski

Comment:

—

u/BonnorEbertMatched

@@ -42 +42 @@
 :[[Image(vradLineOutMatched1.gif, 37%)]]
 
-A comparison between the B&P(2004) setup I just ran and the matched condition for radial velocity is [CompareOldandNew here]. The sphere parameters are the same, except that in the B&P setup, collapse was induced by a 10% over density of the grid. Additionally one can make the comparison between the light ambient case and the B&P setup, as there the comparison would be 10% over density of the grid vs. no density enhancement, follow link [OldandLight here]
 
 ==== Density-'''''
@@ -58 +57 @@
 :[[Image(rhoLineOutMatched1.gif, 36%)]]
 
-It may be interesting to compare these plots to those of a similar collapse study in which the critical BE sphere in a light medium (same density and homogeneity as in the light ambient of this study) was triggered to collapse with a density enhancement above equilibrium values [https://clover.pas.rochester.edu/trac/astrobear/wiki/u/BonnorEbert#Collapse (click here)] -- <<put a comparison between the times seen in these plots and the times seen there>>.
 
 '''Pressure Plots'''
@@ -83 +81 @@
 
 === Discussion'''
+
+-It may be interesting to compare these plots to those of a similar collapse study in which the critical BE sphere in a light medium (same density and homogeneity as in the light ambient of this study) was triggered to collapse with a density enhancement above equilibrium values [https://clover.pas.rochester.edu/trac/astrobear/wiki/u/CompareOldandNew (click here)]. The sphere parameters are the same, except that in the B&P setup, collapse was induced by a 10% over density of the grid. 
 
 -The ram pressure does not seem to be as dominant a factor in inducing collapse, rather the thermal pressure almost immediately exceeds Pcrit.. Thus it may be better to approximate tc as much earlier on.