Scaling of Magneto-Quantum-Radiative Hydrodynamic Equations: From   Laser-produced Plasmas to Astrophysics
  We introduce here the equations of magneto-quantum-radiative hydrodynamics. By rewriting them in a dimensionless form, we obtain a set of parameters that describe scale-dependent ratios of all the characteristic hydrodynamic quantities. We discuss how these dimensionless parameters relate to the scaling between astrophysical observations and laboratory experiments. 
Joseph E. Cross, Brian Reville and Gianluca Gregori
astro-ph.IM