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, 1998

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Shoken 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.
 

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Physics of Interstellar Medium
2
Accretion Disks and Jets
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
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