Changes between Version 27 and Version 28 of u/madams/WireTurbulenceStudies


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Timestamp:
04/22/15 13:26:13 (10 years ago)
Author:
madams
Comment:

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  • u/madams/WireTurbulenceStudies

    v27 v28  
    9292
    9393|| '''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. ||
    95 {{{#!comment
    96 ||  || 20 ||  || [[Image(, width=500)]] || [ GIF] || - Strongest magnetic pressure $(\beta = 0.1)$, thickness = 0.03, Ma = 20 [[br]] ||
     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. || 
     95||  || 20 || 67 || [[Image(betaP1_thicknessP03_mach20_to67_0067.png, width=500)]] || [https://astrobear.pas.rochester.edu/trac/attachment/wiki/u/madams/WireTurbulenceStudies/betaP1_thicknessP03_mach20.gif GIF] || - Strongest magnetic pressure $(\beta = 0.1)$, thickness = 0.03, Ma = 20 [[br]] - May need to check boundary conditions, increased the min density for this run ||
     96{{{#!comment
    9797|| 10 || 20 ||  || [[Image(, width=500)]] || [ GIF] || - Weak magnetic pressure $(\beta = 10)$, thickness = 0.01, Ma = 20 [[br]] ||
    9898||  || 20 ||  || [[Image(, width=500)]] || [ GIF] || - Weak magnetic pressure $(\beta = 10)$, thickness = 0.03, Ma = 20 [[br]] ||