Changes between Version 60 and Version 61 of u/erica/2DShockedClumpsSNR

Timestamp:

01/26/18 05:37:07 (7 years ago)

Author:

Erica Kaminski

Comment:

—

u/erica/2DShockedClumpsSNR

@@ -101 +101 @@
 Q - reflected BC differences?
 
-Q - size scales needing to resolve?
+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)