(Meeting Support) Astrophysical Turbulence Conference at the Institute for Theoretical Physics, University of California, Santa Barbara, May 8-12, 2000

（会议支持）天体物理湍流会议，加州大学圣塔芭芭拉分校理论物理研究所，2000 年 5 月 8-12 日

• 批准号: 0083098
• 负责人: David Gross
• 金额: --
• 依托单位: University of California-Santa Barbara
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2000
• 资助国家: 美国
• 起止时间: 2000-06-15 至 2001-05-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=0083098&HistoricalAwards=false
• 关键词: Meeting; Support; Astrophysical; Turbulence; Conference

Partial support is provided for a meeting to be held at the Institute for Theoretical Physics during May 2000. The focus of the workshop is on evaluating the prospects for advancements in the field of astrophysical turbulence. The talks are organized along several parallel themes:1. Observational properties of astrophysical turbulence, from the Solar atmosphere to the interstellar environment.2. Physics of turbulent processes, with special emphasis on nuclear burning fronts, magnetic reconnection, thermal conduction and radiative fluids.3. Techniques for numerical modeling of turbulent flows.4. Transport of angular momentum via turbulent flows.5. Instabilities and boundary layer effects in turbulent flow regimes.6. Magnetic dynamosFunding for this project was provided by the NSF program for Stellar Astronomy & Astrophysics (AST/SAA).

为 2000 年 5 月在理论物理研究所举行的会议提供了部分支持。研讨会的重点是评估天体物理湍流领域的进展前景。会谈按照几个平行主题组织：1．从太阳大气到星际环境的天体物理湍流的观测特性。 2．湍流过程物理学，特别强调核燃烧前沿、磁重联、热传导和辐射流体。3．湍流数值模拟技术4．通过湍流传递角动量。5．湍流流态中的不稳定性和边界层效应6．磁发电机 该项目的资金由 NSF 恒星天文学和天体物理学 (AST/SAA) 计划提供。