Changes between Version 25 and Version 26 of u/erica/JeansTest

Timestamp:

07/25/13 10:32:02 (12 years ago)

Author:

Erica Kaminski

Comment:

—

u/erica/JeansTest

@@ -161 +161 @@
 
 
-[[Image(rhoInit.png, 35%)]]
+[[Image(rhoInit.png, 20%)]]
 t=0
 
 
-[[Image(RhoFinal.png, 35%)]]
+[[Image(RhoFinal.png, 20%)]]
 t=1/omega
 
@@ -172 +172 @@
 These next plots show AstroBEAR's output using density, velocity, and pressure perturbations described earlier:
 
-[[Image(JeansInit23July2013.png, 35%)]]t=0
+[[Image(JeansInit23July2013.png, 20%)]]t=0
 
 Vx is in red, rho is in green. The density peaks at the zero's of Cos(kx). E.g., a local max is at 1. The vx perturbation is a Sin(x) function, and it has minima that corresponds with the density maxima. This produces converging flows at the max in density, as you would expect you need to develop the Jeans instability.
 
-[[Image(JeansFinal23July2013.png, 35%)]]t=5/omega
+[[Image(JeansFinal23July2013.png, 20%)]]t=5/omega
 
 By the end of the sim, the density perturbation has grown a little, but velocity has grown a lot.
@@ -184 +184 @@
 Now, a query-over-time of rho at r = (1,0,0) produces the following output when compared to the analytical result:
 
-[[Image(GrowthRate.png, 35%)]]
+[[Image(GrowthRate.png, 30%)]]
 
 Pretty tight fit!