“MilkyWay@home”的版本间差异

来自中国分布式计算总站
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| website =http://milkyway.cs.rpi.edu/milkyway/
 
| website =http://milkyway.cs.rpi.edu/milkyway/
 
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MilkyWay@home is an internet-based public distributed computing project employing the BOINC software platform. It attempts to generate highly accurate three-dimensional dynamic models of stellar streams in the immediate vicinity of our Milky Way galaxy. With SETI@home and Einstein@home, it is the third computing project of this type that has the investigation of phenomena in interstellar space as its primary purpose. Its secondary objective is to develop and optimize algorithms for distributed computing.
  
 
[[category:分布式计算项目]][[category:物理化学类项目]][[category:BOINC 平台上的项目]][[category:MilkyWay@home]]
 
[[category:分布式计算项目]][[category:物理化学类项目]][[category:BOINC 平台上的项目]][[category:MilkyWay@home]]

2009年6月28日 (日) 19:06的版本

MilkyWay@home

MilkyWay@home logo.png
MilkyWay@home logo
无屏保图形

开发者 Rensselaer Computer Science Department
版本历史 2007年9月
运算平台 Windows/Linux/Mac
项目平台 BOINC
程序情况
任务情况
项目状态 运行中/开放注册
项目类别 天文学/物理类
优化程序 CPUs/GPUs 优化程序
计算特点 CPU密集:

支持0分享率

支持GPU计算

官方网址 MilkyWay@home
{{{rss}}} [{{{rss}}} 通过 RSS 获取项目新闻]


MilkyWay@home is an internet-based public distributed computing project employing the BOINC software platform. It attempts to generate highly accurate three-dimensional dynamic models of stellar streams in the immediate vicinity of our Milky Way galaxy. With SETI@home and Einstein@home, it is the third computing project of this type that has the investigation of phenomena in interstellar space as its primary purpose. Its secondary objective is to develop and optimize algorithms for distributed computing.