“MilkyWay@home”的版本间差异
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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 | |
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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: |
官方网址 | MilkyWay@home |
[{{{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.