| 103 | | [[br]]'''''Ram pressure profiles over time of a collapsing uniform sphere.''''' '''You can track the passage of time by the shrinking outer radius of the sphere, and the growing ram pressure. A horizontal line (from the shock conditions of the flow) will be placed on this plot, and where it intersects the ram pressure profile(s) will be a prediction of where the ring will form in the splash region of the sims ([https://astrobear.pas.rochester.edu/trac/wiki/u/erica/CFringanalysis see description here]). If the horizontal line were to cross 2 profiles, we would have to check whether given the speed of the splashed material, if there has been time enough for that material to have reached the splash radius.''' |
| | 103 | [[br]]'''''Ram pressure profiles over time of a collapsing uniform sphere.''''' '''You can track the passage of time by the shrinking outer radius of the sphere, and the growing ram pressure. A horizontal line (from the shock conditions of the flow) will be placed on this plot, and where it intersects the ram pressure profile(s) will be a prediction of where the ring will form in the splash region of the sims ([https://astrobear.pas.rochester.edu/trac/wiki/u/erica/CFringanalysis see description here]). If the horizontal line were to cross 2 profiles, we would have to check whether given the speed of the splashed material, if there has been time enough for that material to have reached the splash radius.''' |
| | 104 | |
| | 105 | Note, the full plot range for the ram pressure plot is not shown here -- if it were the tremendous growth of density and velocity as the sphere approached the freefall time would overwhelm everything else.''' |
