Laser Plasma Interactions in Extreme Conditions
Laboratory Astrophysics by High-Power Laser Experiments
Computational Magnetohydrodynamics and Plasma Particle Simulations
instability in protoplanetary disks. II. Ionization state and
unstable regions. T. Sano, S. M. Miyama, T. Umebayashi, and
T. Nakano, Astrophysical Journal, 543, 486 (2000).
momentum transport by magnetohydrodynamic turbulence in
accretion disks: Gas pressure dependence of the saturation
level of the magnetorotational instability. T. Sano,
S. Inutsuka, N. J. Turner, and J. M. Stone, Astrophysical
Journal, 605, 321 (2004).
compression and Hugoniot measurements of liquid hydrogen to
55 GPa. T. Sano et al., Physical Review B, 83, 054117
field amplification associated with the Richtmyer-Meshkov
instability. T. Sano, K. Nishihara, C. Matsuoka and T. Inoue,
Astrophysical Journal, 758, 126 (2012).
magnetic field strength for suppression of the
Richtmyer-Meshkov instability in plasmas. T. Sano, T. Inoue,
and K. Nishihara, Physical Review Letters, 111, 205001
Full List of Publications:
Takayoshi Sano is an assistant professor at Institute of Laser Engineering, Osaka University since 2003. He received a Ph.D. degree from University of Tokyo in 1998. Prior to coming to Osaka, he has been a postdoctoral research associate at National Astronomical Observatory of Japan, University of Maryland, and University of Cambridge.