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2DShockedClumpsSNR

-              v1
+              v2
 '''Shocked Clump (2D)'''
 Would like to study the interaction between a cold clump a supernovae remnant and a shock. To model this am injecting a supersonic wind into the boundary, whose properties are specified by the jump conditions across an adiabatic shock. The jump conditions are calculated using the following parameters in the ambient medium:
+Am investigating the interaction between a cold clump in a supernovae remnant and a shock. To model this, am injecting a supersonic wind into the boundary, whose properties are specified by the jump conditions across an adiabatic shock. The jump conditions are calculated using the following parameters in the ambient medium:
 || $T_{amb}$ || 10^4^ K ||
 …
 || $v_{wind}$ || 2,000 km s^-1^ ||
 The clump is in pressure equilibrium with the ambient medium, and its properties are given by:
+The clump is initially in pressure equilibrium with the ambient medium, and its properties are given by:
+Adiabatic gamma = 5/3, ideal EOS (no cooling)
+|| $T_{clump}$ || 10^4^ K ||
+||$n_{clump}$ || 10^4^ cm^-3^ ||
+||$v_{clump}$|| 0 ||
+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:
+T