@techreport{oai:nifs-repository.repo.nii.ac.jp:00010198,
 author = {"Sato,  T. and Hayashi,  T. and Watanabe,  K. and Horiuchi,  R. and Tanaka,  M. and Sawairi,  N. and Kusano,  K."},
 month = {Aug},
 note = {"Whether it is induced by an ideal (current driven) instability or by an external force, plasma flow causes a change in the magnetic field configuration and often gives rise to a current intensification locally, thereby a fast driven reconnection being driven there. Many dramatic phenomena in magnetically confined plasmas such as magnetospheric substorms, solar flares, MHD self-organization and tokamak sawtooth crash, may be attributed to this fast driven reconnection. Using a fourth order MHD simulation code it is confirmed that compressibility of the plasma plays a crucial role in leading to a fast (MHD time scale) driven reconnection. This indicates that the incompressible representation is not always applicable to the study of a global dynamical behavior of a magnetically confined plasma."},
 title = {Role of Compressibility on Driven Magnetic Reconnection},
 year = {1991}
}