NUMERICAL ASTROPHYSICS BY ULTRA-HIGH SPEED COMPUTER (SUPERCOMPUTER AND SPATIAL PURPOSE COMPUTER)
超高速计算机数值天体物理学(超级计算机和空间计算机)
基本信息
- 批准号:02302014
- 负责人:
- 金额:$ 2.88万
- 依托单位:
- 依托单位国家:日本
- 项目类别:Grant-in-Aid for Co-operative Research (A)
- 财政年份:1990
- 资助国家:日本
- 起止时间:1990 至 1992
- 项目状态:已结题
- 来源:
- 关键词:
项目摘要
In many astronomical phenomena, self-gravity plays very important roles. Then phenomena are usually non-linear, non-stationary and non-uniform by the self-gravity. So in order to analyze them, numerical simulations by ultra-high speed computer are very effective tools. Recently, the speed of supercomputer becomes very high and the capacity of memory storage becomes very large. Hence we can analyze new complicated astronomical phenomena which could not be analysed so far. Therefore using the merit of these new computers, we must produce new software to analyze the phenomena which are based by gravity. In the case of physics in gravitational many body system, for example, globular clusters and galaxies, the basic formula in equations of motion are quite simple. Then producing special purpose computer for many body system are better choice than using general purpose computer. Therefore the main purpose of this grant-in aid for co-operative research is to produce basic software and special purpose machine in order to make numerical simulation of various astronomical phenomena.In this three-years project, the symposium was held three times. Many researches (over 200 people) attended the meeting, showed original results of astrophysics numerical simulation, reported new computational methods and had reports of newly produced special purpose computers. We also published the proceeding of the meeting as well as the collected paper of this research.
在许多天文现象中,自引力起着非常重要的作用。自引力作用下的现象通常是非线性、非平稳和非均匀的。因此,利用超高速计算机进行数值模拟是对其进行分析的有效工具。近年来,超级计算机的运行速度越来越快,存储容量也越来越大。因此,我们可以分析到目前为止无法分析的新的复杂天文现象。因此,利用这些新计算机的优点,我们必须开发新的软件来分析基于重力的现象。在物理学的引力多体系统中,例如球状星团和星系,运动方程的基本公式是相当简单的。因此,为多体系统生产专用计算机是比使用通用计算机更好的选择。因此,本次合作研究资助的主要目的是开发基础软件和专用机器,以便对各种天文现象进行数值模拟。在这个为期三年的项目中,研讨会举办了三次。许多研究人员(200多人)参加了会议,展示了天体物理数值模拟的原创成果,报告了新的计算方法,并报告了新生产的专用计算机。我们还发表了会议纪要以及本次研究的论文选集。
项目成果
期刊论文数量(141)
专著数量(0)
科研奖励数量(0)
会议论文数量(0)
专利数量(0)
Miyama,S.M.& Nagasawa,M: "Proceedings of Supercomputing Astronomy and Astrophysics Symposium in Japan" NAO-TAPS Repqrts, 380 (1991)
美山,S.M.
- DOI:
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- 影响因子:0
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- 通讯作者:
Ohtsuki,K.: "Planetary Accretion in the Solar Gravitational Field" ¨Protostars and Planets III¨ed.Black,D.D.and Mtthews,M.,Univ.Arisona press. (1992)
Ohtsuki, K.:“太阳引力场中的行星吸积”“原恒星和行星 III”,Black,D.D. 和 Mtthews,M.,亚利桑那大学出版社。
- DOI:
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- 影响因子:0
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Kiguchi,M.: "Rrimordial Solar Nebula Embeded in Corona" Science and Technology. 4. 87-93 (1992)
Kiguchi,M.:“日冕中嵌入的太阳星云”科学与技术。
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- 影响因子:0
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Nozawa,S.: "Emergence of Magnetic Flux from the Convection Zone into the Solar Atmosphere,I.Linear and Nonlinear Adiabatic Evolution of the Convectivi-Parker Instability." Astrophys.J.Suppl.78. 267-282 (1992)
Nozawa,S.:“磁通量从对流区进入太阳大气,I.对流-帕克不稳定性的线性和非线性绝热演化”。
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- 影响因子:0
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Hanawa,T.: "Giant Molecular Cloud Formation through the Parker Instability in a Skewed Magnetic Field" Astrophys.J.Lett.L71-L74 (1992)
Hanawa,T.:“通过偏磁场中的帕克不稳定性形成巨型分子云”Astrophys.J.Lett.L71-L74 (1992)
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MIYAMA Shoken其他文献
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{{ truncateString('MIYAMA Shoken', 18)}}的其他基金
Numerical Astronomy using molecular and atomic line transfer calculations in the ALMA-era.
ALMA 时代使用分子和原子线传输计算的数值天文学。
- 批准号:
16204012 - 财政年份:2004
- 资助金额:
$ 2.88万 - 项目类别:
Grant-in-Aid for Scientific Research (A)
Theoretical Research for Chemical Evolution of Molecular Abundance in Protoplanetary Disks
原行星盘分子丰度化学演化的理论研究
- 批准号:
07640363 - 财政年份:1995
- 资助金额:
$ 2.88万 - 项目类别:
Grant-in-Aid for Scientific Research (C)
Theoretical Investigation about a Protoplanetary Disk around a T Tauri Star
关于金牛座 T 星周围原行星盘的理论研究
- 批准号:
04835015 - 财政年份:1992
- 资助金额:
$ 2.88万 - 项目类别:
Grant-in-Aid for General Scientific Research (C)
The Theoretical Study on the Non-1inear Growing Process of Perturbations in the Astrophysical Systems including the Shear Flow.
包括剪切流在内的天体物理系统扰动非线性增长过程的理论研究。
- 批准号:
01540220 - 财政年份:1989
- 资助金额:
$ 2.88万 - 项目类别:
Grant-in-Aid for General Scientific Research (C)
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