Transient Astronomical Sources at Radio Frequencies

无线电频率瞬态天文源

• 批准号: DP0559613
• 负责人: Prof John Dickey
• 金额: $ 22.02万
• 依托单位: University of Tasmania
• 依托单位国家: 澳大利亚
• 项目类别: Discovery Projects
• 财政年份: 2005
• 资助国家: 澳大利亚
• 起止时间: 2005-02-01 至 2008-12-31
• 项目状态: 已结题
• 来源: https://dataportal.arc.gov.au/RGS/Web/Grants/DP0559613
• 关键词: Transient; Astronomical; Sources; Radio; Frequencies

Australian radio telescopes are among the finest and most modern anywhere in the world, and they are the only such instruments that can study the Southern Hemisphere sky. The University of Tasmania operates two radio observatories, at Hobart, Tas, and Ceduna, SA, that are used together to detect astronomical pulses arriving simultaneously at the two sites. The techniques of interference suppression, dispersion searching, fast sampling over broad bandwidths, and high speed data transmission between Ceduna and Hobart that will be implemented in this project have direct applications in science and the communications industry. The students who will develop this equipment will carry over their expertise to the private sector.

澳大利亚射电望远镜是世界上最好、最现代化的射电望远镜之一，它们是唯一可以研究南半球天空的此类仪器。 塔斯马尼亚大学在塔斯马尼亚州霍巴特和南澳州塞杜纳设有两个射电天文台，它们一起用于探测同时到达两个地点的天文脉冲。 该项目将实施的干扰抑制、色散搜索、宽带宽快速采样以及Ceduna和Hobart之间的高速数据传输技术在科学和通信行业具有直接应用。 开发该设备的学生将把他们的专业知识带到私营部门。