Shocked Clump (2D)

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}	104 K
n_{amb}	104 cm-3
v_{amb}	0
v_{wind}	2,000 km s-1

The clump is initially in pressure equilibrium with the ambient medium, and its properties are given by:

T_{clump}	104 K
n_{clump}	104 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