Observation of High Gamma Ray Sources from the South Pole

南极高伽马射线源的观测

• 批准号: 9022723
• 负责人: James Gaidos
• 金额: $ 22万
• 依托单位: Purdue Research Foundation
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 1991
• 资助国家: 美国
• 起止时间: 1991-06-15 至 1993-11-30
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=9022723&HistoricalAwards=false
• 关键词: Observation; Gamma; Ray; Sources; South

This is a continuation of a project to develop and operate air Cherenkov telescopes at South Pole Station for the purpose of studying discreet astrophysical sources of very high energy (VHE) gamma rays. The project is called Gammas At South Pole (GASP), and this second phase is GASP II. The primary instrument consists of an array of parabolic mirrors, with photomultiplier tubes at their foci, which can detect light from VHE interactions in a small volume of the atmosphere. The experiment will shed light on the origin of cosmic rays and possibly on sources of exotic radiation, if such radiation exists. GASP complements the pre-existing South Pole Air Shower Experiment (SPASE), which is operated by the Bartol Research Institute of the University of Delaware and Leeds University (UK), and extends downward by two to three orders of magnitude the energy threshold of SPASE. SPASE can survey most of the southern sky, and GASP will be able to focus on small regions of suspected activity. The location at South Pole allows GASP to view a single object for extended periods (weeks to months) through a constant thickness of atmosphere, while mid-latitude locations allow only a few hours of viewing at a time of a given object. The Polar location also means that the very interesting high declination southern sky is always within view, which gives GASP a great advantage over any mid- latitude observatory. The project is a collaboration of the University of Wisconsin, Purdue University, Bartol Research Institute of the University of Delaware and Smithsonian Astrophysical Observatory. It is jointly funded by NSF's Divisions of Polar Programs, the Wisconsin Alumni Research Foundation and the Smithsonian Astrophysical Observatory.

这是在南极站开发和操作空气切伦科夫望远镜的项目的继续，目的是研究非常高能量伽马射线的谨慎天体物理来源。该项目被称为南极伽马(GAP)，第二阶段是GAP II。主要仪器由一系列抛物面反射镜组成，在焦点处有光电倍增管，可以探测到小体积大气中VHE相互作用产生的光。这项实验将阐明宇宙射线的起源，如果存在外来辐射的话，还可能揭示这种辐射的来源。GAP是对先前存在的南极空气簇射实验(SPASE)的补充，该实验由特拉华大学和利兹大学(英国)巴托尔研究所运营，并将SPASE的能量阈值向下扩展了两到三个数量级。Spase可以探测南方大部分天空，而Gap将能够专注于疑似活动的小区域。南极的位置允许GASP通过恒定的大气厚度在较长的时间内(几周到几个月)观察单个物体，而中纬度位置一次只允许观察给定物体的几个小时。极地位置也意味着非常有趣的高赤纬南方天空总是在视野中，这使GASP比任何中纬度天文台都有很大的优势。该项目由威斯康星大学、普渡大学、特拉华大学巴托尔研究所和史密森天体物理天文台合作完成。该项目由美国国家科学基金会极地项目部、威斯康星州校友研究基金会和史密森天体物理天文台共同资助。