| 85 | | || '''Beta''' || ''' Picture at Final Frame (200)''' || '''GIF''' || '''Notes & Questions''' || |
| 86 | | || 0.1 (Strongest Magnetic Pressure) || [[Image(betaP1_thicknessP01_mach20restartfrom1840016.png, width=500)]] || [https://astrobear.pas.rochester.edu/trac/attachment/wiki/u/madams/WireTurbulenceStudies/betaP1_thicknessP01_mach20.gif GIF] || - Strongest 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. || |
| 87 | | || Hydro (MHD Off) || [[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]] || |
| 88 | | || || [[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]] || |
| 89 | | || || [[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]] || |
| | 85 | === MHD === |
| | 86 | |
| | 87 | || '''Beta''' || '''Ma''' ||'''Picture at Final Frame (200)''' || '''GIF''' || '''Notes, Questions, Observations''' || |
| | 88 | || 0.1 || 20 || [[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. || |
| | 89 | {{{#!comment |
| | 90 | || || 20 || [[Image(, width=500)]] || [ GIF] || - Strongest magnetic pressure $(\beta = 0.1)$, thickness = 0.03, Ma = 20 [[br]] || |
| | 91 | || 10 || 20 || [[Image(, width=500)]] || [ GIF] || - Weak magnetic pressure $(\beta = 10)$, thickness = 0.01, Ma = 20 [[br]] || |
| | 92 | || || 20 || [[Image(, width=500)]] || [ GIF] || - Weak magnetic pressure $(\beta = 10)$, thickness = 0.03, Ma = 20 [[br]] || |
| | 93 | || || 20 || [[Image(, width=500)]] || [ GIF] || - Weak magnetic pressure $(\beta = 10)$, thickness = 0.06, Ma = 20 [[br]] || |
| | 94 | || || 3 ||[[Image(, width=500)]] || [ GIF] || - Weak magnetic pressure $(\beta = 10)$, thickness = 0.01, Ma = 3 [[br]] || |
| | 95 | || || 3 || [[Image(, width=500)]] || [ GIF] || - Weak magnetic pressure $(\beta = 10)$, thickness = 0.03, Ma = 3 [[br]] || |
| | 96 | || || 3 || [[Image(, width=500)]] || [ GIF] || - Weak magnetic pressure $(\beta = 10)$, thickness = 0.06, Ma = 3 [[br]] || |
| | 97 | }}} |
| | 98 | |
| | 99 | === Hydro === |
| | 100 | |
| | 101 | || '''Ma''' || '''Picture at Final Frame (200)''' || '''GIF''' || '''Notes, Questions, Observations''' || |
| | 102 | || 20 || [[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]] || |
| | 103 | || 20 || [[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]] || |
| | 104 | || 20 || [[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]] || |
