Changes between Version 20 and Version 21 of u/madams/WireTurbulenceStudies

Timestamp:

04/20/15 13:43:27 (10 years ago)

Author:

madams

Comment:

—

u/madams/WireTurbulenceStudies

@@ -8 +8 @@
 '''List of simulations'''
 
-|| '''Beta''' || '''Ma''' || '''Thickness (cm)''' || '''MinDensity (cu)''' (dynes/cm^2) || ''Completed as of 04-20'' ||
+|| '''$\beta$''' || '''$Ma$''' || '''Thickness $(\text{cm}^2)$''' || '''MinDensity $(\text{cu})$''' or $(\text{dynes}/\text{cm}^2)$ || ''Completed as of 04-20'' ||
 || 10 || 20 || 0.01 || 1d-10 || Frame 184 ||
 ||  ||  || 0.03 || 0.01, after frame 90 || Frame 101 ||
@@ -84 +84 @@
 
 || '''Beta''' || ''' Picture at Final Frame (200)''' || '''GIF''' || '''Notes & Questions''' ||
-|| 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] || ||
-|| 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] || ||
-||  || [[Image(hydro_thickp03_mach20restartfrom1780022.png, width=500)]] || [https://astrobear.pas.rochester.edu/trac/attachment/wiki/u/madams/WireTurbulenceStudies/hydro_thickp03_mach20.gif GIF] || ||
-||  || [[Image(hydro_thickp06_mach20restartfrom1880012.png, width=500)]] || [https://astrobear.pas.rochester.edu/trac/attachment/wiki/u/madams/WireTurbulenceStudies/hydro_thickp06_mach20.gif GIF] || ||
+|| 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. ||
+|| 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]] ||
+||  || [[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]] ||
+||  || [[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]] ||
 
 [[CollapsibleEnd]]