Changes between Version 8 and Version 9 of CollidingFlows


Ignore:
Timestamp:
06/29/11 10:17:54 (14 years ago)
Author:
Jonathan
Comment:

—

Legend:

Unmodified
Added
Removed
Modified

  • CollidingFlows

    v8 v9  
    3737||  [attachment:233_1_Sinks.gif movie]  ||  [attachment:233_4_Sinks.gif movie]  ||   [attachment:233_10_Sinks.gif movie]  ||  [attachment:233_20_Sinks.gif movie]  ||
    3838|| [[Image(233_1_Sinks.png, width=200)]] || [[Image(233_4_Sinks.png, width=200)]] || [[Image(233_10_Sinks.png, width=200)]] || [[Image(233_20_Sinks.png, width=200)]] ||
     39
     40== Discussion ==
     41  All of these runs had poorly resolved cooling lengths (fractions of a cell).  The fastest growing modes were therefore at the nyquist frequency.  This is however much larger than the cooling length of the shocked layer.  I suspect that at higher resolutions the size of the condensations from the TI will much smaller and more prone to evaporation (or clump destruction) in the turbulent background flow...