Changes between Version 9 and Version 10 of u/erica/CFringanalysis


Ignore:
Timestamp:
07/01/15 19:57:45 (10 years ago)
Author:
Erica Kaminski
Comment:

Legend:

Unmodified
Added
Removed
Modified
  • u/erica/CFringanalysis

    v9 v10  
    7676[[Image(CFrampressure.png, 40%)]]
    7777
    78 Now, the post shock density is comparable to the density of the infalling ambient. However, the velocity is very different, as it should be in retrospect. This leads to large deviations between the ram pressure of the infalling ambient and the ram pressure of the splashed material.
     78Now, the post shock density is comparable to the density of the infalling ambient. However, the velocity is very different, as it should be in retrospect. This leads to large deviations between the ram pressure of the infalling ambient and the ram pressure of the splashed material. So large in fact (3 orders of magnitude), that the ram pressure of the splashed material doesn't make it on this plot; Pram = 1.5*10^-12^ for the post-shock flow.
    7979
    80 The incoming flows have a high speed, and once shocked, though decreased, is still high. The ambient, however, is starting from rest. This means, that by the time the entire simulation has completed (i.e. long after the ring has formed), the ambient has still not acquired enough momentum to make the ram pressures balance.
     80The incoming flows have a very high speed, and once shocked, though decreased, is still high. The ambient, however, is starting from rest. This means, that by the time the entire simulation has completed (i.e. long after the ring has formed), the ambient has still not acquired enough momentum to make the ram pressures balance.
    8181
    82 In hindsight, this was always going to be the case, as the ring is not present in the hydro case, and so the ambient's own dynamics are too weak to constrain outflowing material from the collision region.
     82In hindsight, this was always going to be the case, as the ring is not present in the hydro case, and so the ambient's own dynamics are too weak to constrain outflowing material from the collision region. Next need to include magnetic fields in the ambient pressure.
     83 
    8384----
    8485