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sano[atmark]ile.osaka-u.ac.jp
Hydrodynamical Instabilities and Turbulence in Astrophysical and Laboratory Plasmas Laser Plasma Interactions in Extreme Conditions Laboratory Astrophysics by High-Power Laser Experiments Computational Magnetohydrodynamics and Plasma Particle Simulations
Unstable growth of the Richtmyer-Meshkov instability (top) and freeze-out of the instability by a compressible effect (bottom).
Magnetorotational
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).
DOI: 10.1086/317075
Angular
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).
DOI: 10.1086/382184
Laser-shock
compression and Hugoniot measurements of liquid hydrogen to
55 GPa. T. Sano et al., Physical Review B, 83, 054117
(2011).
DOI: 10.1103/PhysRevB.83.054117
Magnetic
field amplification associated with the Richtmyer-Meshkov
instability. T. Sano, K. Nishihara, C. Matsuoka and T. Inoue,
Astrophysical Journal, 758, 126 (2012).
DOI: 10.1088/0004-637X/758/2/126
Critical
magnetic field strength for suppression of the
Richtmyer-Meshkov instability in plasmas. T. Sano, T. Inoue,
and K. Nishihara, Physical Review Letters, 111, 205001
(2013).
DOI: 10.1103/PhysRevLett.111.205001
Full List of Publications:
Researcher ID, Astrophysics Data System
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.