Gallary
[↑ click the figure to see the movie ] Results of MHD simulation of CME. The sphere shows the surface of the Sun (colors: magnetic field) and tubes displays magnetic field lines.

cloud1.gif[↑ click the figure to see the movie ] Cloud formation and rainfall simulated by the coupled model of SDM and non-hydrostatic model.
[↑ click the figure to see the movie ] Cloud formation and rainfall simulated by the coupled model of SDM and non-hydrostatic model.

We have applied our interlocked plasma simulation model to the shock problem in the space plasma. In the area of 0 to 10,000 in X axis, the fluid model is performed. And in the area of 10,000 to 15,000, the particle model is performed. Then both models are self-consistently connected. We can see the physics in the extended area with the detailed physics around the shock transition layer.

nucl.gif[↑ click the figure to see the movie ] Homogeneous vapor-liquid nucleation of water.