Changes between Version 5 and Version 6 of u/SurfacePressureApprox

Timestamp:

10/18/13 17:14:08 (11 years ago)

Author:

Erica Kaminski

Comment:

—

u/SurfacePressureApprox

@@ -3 +3 @@
 There are 2 limits we identify, the first is the sparse ambient limit in which we treat the ambient as a collection of parcels of gas that are attracted to the BE sphere only, and the 2nd is the dense ambient limit where we treat the ambient as a collapsing uniform sphere. Our approximations should explain the data in this table,
 
-[[]]
+http://astrobear.pas.rochester.edu/trac/astrobear/blog/erica10152013
 
 = Sparse Cases = 
@@ -33 +33 @@
 Using this expression gives the following results,
 
-[[Image(Pressderiv.png)]]
+[[Image(sparsederiv.png, 90%)]]
 
 Vertical lines indicate when a sink formed for the corresponding run. The horizontal line is the initial external pressure on the BE sphere, which since the sphere is a critical BE sphere, equals the critical pressure. 
@@ -41 +41 @@
 Plotting denser ambient mediums skews the graph, as they increase much more rapidly on the y-axis.
 
-Here is a table of the runs summary, 
-
-[[Image(runssummary.png)]]
 
 = Dense Case = 
@@ -81 +78 @@
 Here are the results,
 
+[[Image(logplotall.png, 90%)]]
+
 = Compare the 2 approximations side by side = 
 
-[[]]
+[[Image(logplotall.png, 90%)]]
 
-[[]]
+[[Image(sparsederiv.png, 90%)]]