Changes between Version 3 and Version 4 of u/erica/2DShockedClumpsSNR


Ignore:
Timestamp:
01/19/18 11:53:40 (7 years ago)
Author:
Erica Kaminski
Comment:

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  • u/erica/2DShockedClumpsSNR

    v3 v4  
    3131
    3232
    33 The thermodynamics in the simulation are governed by an ideal EOS, and an adiabatic index of gamma = 5/3. The abundances are taken to be solar ($\mu=1.3$). Other parameters of interest are:
     33The thermodynamics in the simulation are governed by an ideal EOS, and an adiabatic index of gamma = 5/3. The abundances are taken to be solar ($\mu=1.3$). Other parameters of interest are the clump radius, clump crushing time, sound crossing time (ambient and clump medium to travel a clump radius), wind crossing time (to travel clump radius):
    3434
    35 T
     35|| $R_{clump}$ || $10^16 ~cm$ ||
     36|| $t_{cc}$ || $5\times 10^8~s$ ||
     37|| $t_{sc}$ (for ambient) || $5\times 10^8~s$ ||
     38|| $t_{sc}$ (for ) || $5\times 10^8~s$ ||
     39|| $t_{wc}$ (for domain of $L=10~R_c$) || $5\times 10^8~s$ ||
     40