| 93 | | || '''Beta''' || '''Ma''' ||'''Picture at Final Frame (200)''' || '''GIF''' || '''Notes, Questions, Observations''' || |
| 94 | | || 0.1 || 20 || |
| | 93 | || '''Beta''' || '''Ma''' || '''Last Frame Completed''' ||'''Picture at Final Frame''' || '''GIF''' || '''Notes, Questions, Observations''' || |
| | 94 | || 0.1 || 20 || 200 || [[Image(betaP1_thicknessP01_mach20restartfrom1840016.png, width=500)]] || [https://astrobear.pas.rochester.edu/trac/attachment/wiki/u/madams/WireTurbulenceStudies/betaP1_thicknessP01_mach20.gif GIF] || - Strong magnetic pressure $(\beta = 0.1)$, wire radius, i.e. thickness = 0.01, Ma = 20 [[br]] - "Clumps" seem to grow in density over the evolution of the simulation. Starting with a wire radius of 0.01, it clearly grows to a larger radius (~0.03 cm). This seems to start once the clump moves past x = 0.6 cm. [[br]] - The clumps get pushed back incredibly far. Starting at $x_{i} = 0.25 \text{cm}$, ending at $x_{f} = 2.75 \text{cm}$. Perhaps this is due to the high magnetic pressure. [[br]] - A low density $(0.5 \text{dynes}/\text{cm}^2)$ region forms behind the clump at around x = 0.7 cm. [[br]] - Unclear when the clump stops accreting. || |
| 96 | | || || 20 || |
| 97 | | || 10 || 20 || |
| 98 | | || || 20 || |
| 99 | | || || 20 || |
| 100 | | || || 3 || |
| 101 | | || || 3 || |
| 102 | | || || 3 || |
| | 96 | || || 20 || || [[Image(, width=500)]] || [ GIF] || - Strongest magnetic pressure $(\beta = 0.1)$, thickness = 0.03, Ma = 20 [[br]] || |
| | 97 | || 10 || 20 || || [[Image(, width=500)]] || [ GIF] || - Weak magnetic pressure $(\beta = 10)$, thickness = 0.01, Ma = 20 [[br]] || |
| | 98 | || || 20 || || [[Image(, width=500)]] || [ GIF] || - Weak magnetic pressure $(\beta = 10)$, thickness = 0.03, Ma = 20 [[br]] || |
| | 99 | || || 20 || || [[Image(, width=500)]] || [ GIF] || - Weak magnetic pressure $(\beta = 10)$, thickness = 0.06, Ma = 20 [[br]] || |
| | 100 | || || 3 || || [[Image(, width=500)]] || [ GIF] || - Weak magnetic pressure $(\beta = 10)$, thickness = 0.01, Ma = 3 [[br]] || |
| | 101 | || || 3 || || [[Image(, width=500)]] || [ GIF] || - Weak magnetic pressure $(\beta = 10)$, thickness = 0.03, Ma = 3 [[br]] || |
| | 102 | || || 3 || || [[Image(, width=500)]] || [ GIF] || - Weak magnetic pressure $(\beta = 10)$, thickness = 0.06, Ma = 3 [[br]] || |
| 107 | | || '''Ma''' || ''' |
| 108 | | || 20 || |
| 109 | | || 20 || |
| 110 | | || 20 || |
| | 107 | || '''Ma''' || '''last Frame Completed ''' || '''Picture at Final Frame (200)''' || '''GIF''' || '''Notes, Questions, Observations''' || |
| | 108 | || 20 || 200 || [[Image(hydro_thickp01_mach20restartfrom1400059.png, width=500)]] || [https://astrobear.pas.rochester.edu/trac/attachment/wiki/u/madams/WireTurbulenceStudies/hydro_thickp01_mach20.gif GIF] || - Hydro (MHD off), thickness = 0.01, Ma = 20 [[br]] - Clump seems to end at position $x_{f} = .725 \text{cm}$ || |
| | 109 | || 20 || 200 || [[Image(hydro_thickp03_mach20restartfrom1780022.png, width=500)]] || [https://astrobear.pas.rochester.edu/trac/attachment/wiki/u/madams/WireTurbulenceStudies/hydro_thickp03_mach20.gif GIF] || - Hydro (MHD off), thickness = 0.03, Ma = 20 [[br]] - Clump seems to end at position $x_{f} = .4 \text{cm}$ || |
| | 110 | || 20 || 200 || [[Image(hydro_thickp06_mach20restartfrom1880012.png, width=500)]] || [https://astrobear.pas.rochester.edu/trac/attachment/wiki/u/madams/WireTurbulenceStudies/hydro_thickp06_mach20.gif GIF] || - Hydro (MHD off), thickness = 0.06, Ma = 20 [[br]] - Clump seems to end at position $x_{f} = .325 \text{cm}$ [[br]] - At - x = 0.3cm, the clump seems to "flatten" -- not sure if this is physical, to be expected, or a problem with the code. || |
