Changes between Version 62 and Version 63 of u/erica/2DShockedClumpsSNR

Timestamp:

01/26/18 05:39:57 (7 years ago)

Author:

Erica Kaminski

Comment:

—

u/erica/2DShockedClumpsSNR

@@ -90 +90 @@
 This set of runs is meant to see how to adequately track the shock front with AMR and the clump. As the resolution in the ambient medium goes down with AMR, we wish to provide adequate resolution around the shock front as to not degrade the solution. Am doing a quick test of an AMR simulation of the fiducial initial conditions with the resolution of the ambient medium decreased by a factor of 4, plus two levels of refinement on the clump and refinement triggered by density gradients. 
 
+=== Run 7 - Prelim 3D run ===
+
 === Unresolved thoughts: ===
 
+Q - reflected BC differences - due to pressure/density protection, or position of clump wrt to grid?
 
-Q - estimate on sim runtime?
+Q - size scales needing to resolve (i.e. instabilities and their wavelengths)?
 
-Q - location of clump center wrt grid?
-
-Q - reflected BC differences?
-
-Q - size scales needing to resolve? (instabilities and their wavelengths)
-
-Q - cooling cases (cooling lengths/timescales, temperature ranges for various cooling tables in astrobear, modifying the abundances statically as well as dynamically, what options for tracking ionizations, etc., radiative shock physics -- shock structures in steady state solutions, additional instabilities that arise when cooling is possible)
+Q - examine cooling cases (cooling lengths/timescales, temperature ranges for various cooling tables in astrobear, modifying the abundances statically as well as dynamically, what options for tracking ionizations, etc., radiative shock physics -- shock structures in steady state solutions, additional instabilities that arise when cooling is possible)