Transforming DIY Geiger Counter Kits into Muon Detectors for Education and Scientific Exploration

Particles Pub Date : 2024-07-12 DOI:10.3390/particles7030034
Marco Arcani, D. Liguori, Andrea Frassà, Altea Renata Maria Nemolato, Omar Del Monte, Cesare Guaita
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Abstract

Any Geiger counter can be used as an effective cosmic ray detector on its own. In fact, it is known that even in the absence of a radioactive source, the instrument detects what is known as background radiation, which consists of various types of ionizing particles present in the environment. Remarkably, it is estimated that up to 15% of this background radiation is attributable to cosmic rays, high-energy particles originating from outer space. The remaining radiation detected by the Geiger counter originates from terrestrial sources, such as natural radioactivity in the ground and in the air. The main goal of this project is to build a muon detector for scientific and educational purposes using two commercial DIY Geiger counter kits and just a few additional components. To identify cosmic radiation from terrestrial radiation and improve the accuracy of cosmic ray measurements, the use of a coincident circuit is essential. This coincident circuit was introduced in cosmic ray physics by Walther Bothe and Bruno Rossi in the early 1930s and allows for the detection of a subatomic particle passing through two or more sensors, thereby reducing false positives and enhancing the reliability of cosmic ray detection. The following idea is an alternative replica of our AMD5 detectors, instruments that we have been using for years to teach and perform scientific experiments in the cosmic ray field under the umbrella of the ADA project (2023 Particles, Arcani et al.). The resulting device, named AMD5ALI, offers a reliable and inexpensive solution for the same goal, making it a valuable tool for both educational purposes and scientific surveys. Practical applications range from cosmic ray physics to radioactivity, including the relationship between cosmic ray flux and meteorology, the zenithal effect, the Regener–Pfotzer curve in the atmosphere, and the anti-correlation of cosmic particle intensity with solar activity.
将 DIY 盖革计数器套件改造成用于教育和科学探索的μ介子探测器
任何盖革计数器本身都可以用作有效的宇宙射线探测器。事实上,即使在没有放射源的情况下,盖革计数器也能检测到所谓的本底辐射,本底辐射由环境中存在的各种电离粒子组成。值得注意的是,据估计,在这些本底辐射中,有高达 15%的辐射来自宇宙射线,即来自外太空的高能粒子。盖革计数器检测到的其余辐射来自陆地,如地面和空气中的天然放射性。本项目的主要目标是利用两个商用 DIY 盖革计数器套件和一些额外的组件,制作一个用于科学和教育目的的μ介子探测器。为了从地面辐射中识别宇宙辐射,提高宇宙射线测量的准确性,使用重合电路是必不可少的。这种重合电路是由 Walther Bothe 和 Bruno Rossi 在 20 世纪 30 年代初引入宇宙射线物理学的,它可以检测到通过两个或更多传感器的亚原子粒子,从而减少误报,提高宇宙射线检测的可靠性。下面的想法是我们的 AMD5 探测器的替代复制品,我们多年来一直使用这些仪器在 ADA 项目(2023 粒子,Arcani 等人)的保护伞下进行宇宙射线领域的教学和科学实验。由此产生的设备被命名为 AMD5ALI,为实现同样的目标提供了可靠而廉价的解决方案,使其成为教育目的和科学调查的重要工具。实际应用范围从宇宙射线物理学到放射性,包括宇宙射线通量与气象学的关系、天顶效应、大气中的瑞格纳-普福泽曲线以及宇宙粒子强度与太阳活动的反相关性。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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CiteScore
3.20
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