Changes between Version 11 and Version 12 of u/erica/2DShockedClumpsSNR
- Timestamp:
- 01/22/18 05:08:43 (7 years ago)
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u/erica/2DShockedClumpsSNR
v11 v12 31 31 32 32 33 The thermodynamics in the simulation are governed by an ideal EOS (specified by $\gamma$). The abundances are taken to be solar ($\mu=1.3$). Other parameters of interest are the clump radius ($ r_c$), clump-ambient density contrast ($\chi$), clump crushing time ($t_{cc}=\sqrt{\chi} R_c/v_s$), sound crossing time (ambient and clump medium to travel a clump radius; $t_{sc}$), wind crossing time (to travel clump radius; $t_{wc}$):33 The thermodynamics in the simulation are governed by an ideal EOS (specified by $\gamma$). The abundances are taken to be solar ($\mu=1.3$). Other parameters of interest are the clump radius ($R_c$), clump-ambient density contrast ($\chi$), clump crushing time ($t_{cc}=\sqrt{\chi} R_c/v_s$), sound crossing time (ambient and clump medium to travel a clump radius; $t_{sc}$), wind crossing time (to travel clump radius; $t_{wc}$): 34 34 35 || $R_{c lump}$ || $10^{16} ~cm$ ||35 || $R_{c}$ || $10^{16} ~cm$ || 36 36 || $t_{cc}$ || $5\times 10^8~s$ || 37 37 || $t_{sc}$ (for ambient) || $5\times 10^8~s$ ||
