1. Flux Corrected Transport I: SHASTA A fluid transport algorithm that works;Boris;J. Comput. Phys.,1973
2. solwnd: A 3D compressible MHD code for Solar Wind studies. version 1.0: Cartesian coordinates;Deane,1996
3. Computations of Three-Dimensional Compressible Rayleigh-Taylor Instability on SGI/Cray T3E;Deane,1999
4. The Effects of Streams and Microstreams on Alfv ic Fluctuations in the Solar Wind;Goldstein,2002
5. Numerical simulation of turbulence in the Solar Wind;Goldstein;J. Geophys. Res.,1999