Numerical Astrophysics: Proceedings of the International Conference on Numerical Astrophysics 1998 (NAP98), held at the National Olympic Memorial Youth Center, Tokyo, Japan, March 10–13, 1998Shoken M. Miyama, Kohji Tomisaka, Tomoyuki Hanawa Springer Science & Business Media, 6 dic 2012 - 437 páginas These are the proceedings of international conference on Numerical As trophysics 1998 (NAP98), held at National Olympic Memorial Youth Cen ter, in Tokyo, Japan in the period of March 10 - 13, 1998, and hosted by the National Astronomical Observatory, Japan (NAOJ). In the last decade numerical simulations have grown up as a major tool for astrophysics. Numerical simulations give us invaluable informa tion on complex systems and physical processes under extreme conditions which can be neither realized by experiments nor directly observed. Super computers and special purpose computers may work as very large telescopes and special purpose telescopes for theoretical astrophysics, respectively. Nu merical astrophysics ranks with other tool-oriented astronomy such as ra dio astronomy, infrared astronomy, ultraviolet astronomy, X-ray astronomy, and ')'-ray astronomy. This conference, NAP98, was planned to explore recent advances in astrophysics aided by numerical simulations. The subjects of the confer ence included the large-scale structure formation, galaxy formation and evolution, star and planets formation, accretion disks, jets, gravitational wave emission, and plasma physics. NAP98 had also sessions on numerical methods and computer science. The conference was attended by 184 sci entists from 21 countries. We enjoyed excellent talks, posters, videos, and discussions: there are 40 oral presentations, 96 posters and 16 video pre sentations. We hope that these proceedings and accompanying CD-ROM replay the friendly but inspiring atmosphere of the conference. |
Índice
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4 | |
Exploring RedshiftSpace Clustering with Cosmological Nbody Simulations | 10 |
Nbody Simulation of Dark Matter Halo Formation Using Grape | 29 |
Effects of the UV Background Radiation on Galaxy Formation | 45 |
Primordial Gas Collapsing with H2 Cooling | 53 |
The Formation and Simulation Analysis of a Ring Galaxy | 67 |
Force Distribution and Relaxation Time in Clusters of Galaxies | 81 |
Jets from TimeDependent Accretion Flows onto a Black Hole | 219 |
Dynamics of a Magnetic Flux Tube in Differentially Rotating Disks | 233 |
Supernovae Neutron Stars and Black Holes | 247 |
Supernova Explosions | 265 |
Single | 281 |
Explosion of a Neutron Star below the Minimum Mass with Implicit | 285 |
MHD Simulations of Magnetic Reconnection and Solar Flares | 303 |
3D Nonlinear MHD Wave Heating of Coronal Loops | 319 |
HII Regions and Planetary Nebulae | 85 |
Simulations of MHD Turbulence in Giant Molecular Clouds | 99 |
Simulation of the Ambipolar Filamentation of Turbulent Magnetic Fields | 113 |
Gravitational Collapse and Fragmentation in Molecular Clouds with | 131 |
Bar and Disk Formation | 151 |
X | 161 |
Formation of a Dense Filamentary Core and its Fragmentation into | 165 |
Molecular Evolution in PlanetForming Circumstellar Disks | 179 |
Instability and Turbulence in Accretion Disks | 187 |
5D Nonsteady MHD Simulations of Magnetically Driven Jets from | 203 |
The Extrapolated 3D Solar Magnetic Fields in AR 7321 | 333 |
The 3Dimensional Numerical Simulation of Solar Flares | 341 |
Smoothed Particle Hydrodynamics | 357 |
A 3D Radiative Transfer Solver Using a Massively Parallel Computer | 375 |
Numerical Simulations of the Astrophysical MHD Flows | 389 |
A Stochastic Simulation Method for FokkerPlanck Equations | 399 |
Efficient 3D Data Transfer for Remote Visualization | 415 |
Development of a Special Purpose Computer for Cosmic Hydrodynamics | 429 |
Otras ediciones - Ver todo
Numerical Astrophysics Shoken M. Miyama,Kohji Tomisaka,Tomoyuki Hanawa Vista previa restringida - 1999 |
Numerical Astrophysics: Proceedings of the International Conference on ... Shoken M. Miyama,Kohji Tomisaka,Tomoyuki Hanawa No hay ninguna vista previa disponible - 2013 |
Numerical Astrophysics Shoken M. Miyama,Kohji Tomisaka,Tomoyuki Hanawa No hay ninguna vista previa disponible - 2014 |
Términos y frases comunes
1999 Kluwer Academic accretion disk algorithm angular momentum Ap.J Astronomy Balbus binary black hole Bodenheimer boundary calculations clumps cluster collapse computational core cosmological dark matter density distribution density profiles dynamical energy equations equilibrium evolution Figure filamentary flow flux fragmentation galactic gravitational gravitational collapse grid H II regions halos Hawley hydrodynamics instability interaction ionization isothermal Japan Japan Japan Japan jets Kluwer Academic Publishers linear magnetic field magnetic field lines magnetic reconnection mass Matsumoto method MHD simulations MNRAS molecular clouds N-body simulations neutron stars nonlinear Numerical Astrophysics numerical simulations observed orbital orbital eccentricity panel parameters particles PASJ perturbation phase Phys Physics planet plasma protostar protostellar radiation radiative radius redshift region resolution resonances rotation S. M. Miyama scale Shibata shock shows solar spiral star formation stellar structure temperature thermal Tokyo turbulence Uchida University University of Tokyo velocity wave