FLASH - FLuorescence in Air SHowers

FLASH - 空气淋浴中的荧光

• 批准号: 0400053
• 负责人: Charles Jui
• 金额: $ 12万
• 依托单位: University of Utah
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2005
• 资助国家: 美国
• 起止时间: 2005-04-01 至 2007-03-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=0400053&HistoricalAwards=false
• 关键词: FLASH; FLuorescence; Air; SHowers

This proposal requests funds to carry out a spectrally resolved measurement of air fluorescence produced by electromagnetic showers at Stanford Linear Accelerator Center (SLAC). The group expects that this experiment will shed light on the apparent differences between the results reported by two ultra high energy cosmic ray (UHECR) experiments, HiRes and AGASA, and will provide reliable and much needed tests of shower-induced fluorescence for future UHECR experiments.The group aims to achieve an accuracy of 8% in the total fluorescence yield and in the individual spectral lines. The experiment will also verify that our understanding of the energy dependence of the yield is correct down to the lowest energies effective in showers, ~100 keV. The Final Focus Test Beam (FFTB) electron line at SLAC will be used at intensities of 10^7 to 10^9 per pulse. They propose to use both thin target and thick target approaches. A thin target run will allow them to measure the total fluorescence yield per beam track, and the spectrum, to 8%. It will also allow a precise measurement of the dependences of the yield and spectrum on pressure and on atmospheric impurities. The interaction of the beam in a thick target mimics the distribution of electron energies found deep in cosmic ray induced air showers. A beam with 10^8 electrons (~28 GeV /electron) has an energy per bunch equal to that of a 2.8 x10^18 eV shower. The superposition of the showers can be modeled by software such as EGS and GEANT. In the thick target experiment the fluorescent yield will be measured at various depths in the shower development, allowing detailed comparison with the Monte Carlo simulations. Measurements on air or nitrogen mixed with various concentrations of CO2, Ar and water vapor will also be performed.

该提案要求提供资金，对斯坦福大学直线加速器中心（SLAC）电磁簇射产生的空气荧光进行光谱分辨测量。 该小组预计，该实验将揭示两个超高能宇宙射线（UHECR）实验，HiRes和AGASA报告的结果之间的明显差异，并将为未来的UHECR实验提供可靠和急需的荧光诱导荧光测试。该小组的目标是在总荧光产额和单个光谱线中达到8%的准确度。 实验还将验证我们对产率的能量依赖性的理解是正确的，直到簇射中有效的最低能量，~100 keV。 SLAC的最终聚焦测试束（FFTB）电子线将以每脉冲10^7至10^9的强度使用。他们建议同时使用薄目标和厚目标方法。一个薄的目标运行将允许他们测量每个光束轨道的总荧光产率和光谱，达到8%。它还将允许精确测量产率和光谱对压力和大气杂质的依赖性。 束在厚靶中的相互作用模拟了在宇宙射线诱导的空气簇射中发现的电子能量分布。一束具有10^8电子（约28 GeV /电子）的电子束，每束团的能量等于2.8 x10^18 eV簇射的能量。簇射的叠加可以通过诸如EGS和GEANT的软件来模拟。在厚靶实验中，将在簇射发展的不同深度测量荧光产率，从而与蒙特卡罗模拟进行详细比较。还将对混合有各种浓度的CO2、Ar和水蒸气的空气或氮气进行测量。