月球:月球表面的一个永久高能宇宙射线天文台

IF 4.2 3区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
P.S. Marrocchesi
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引用次数: 0

摘要

在未来的几十年里,我们将看到太空计划的快速发展,目的是在我们的卫星上实现栖息地。因此,评估在月球上建立永久性宇宙射线(CR)观测站的可行性是有意义的。它巨大的敏感区域将允许在几十年的时间跨度内以前所未有的能量范围进行非常丰富的观测计划。深入探索位于几PeV的CR光谱异常周围的能量区域(也称为“膝盖”)将成为可能。在本文中,我们提出了一个模块化月球天文台的创新概念,旨在克服当前一代低地球轨道宇宙射线望远镜的局限性。它由一系列完全独立的模块组成,每个模块的尺寸和重量都有限。这将在逐步部署逐渐增加的活动量方面具有充分的灵活性,同时确保在其执行的中间阶段收集有意义的科学数据。每个独立模块由三个主要仪器组成:一个组合电荷和飞行时间探测器,用于识别从质子到镍(以及其他)的单个元素,一个跟踪器,提供入射粒子的方向和撞击点,以及一个量热计,用于测量其动能。每个仪器的设计都包含创新的解决方案,这些解决方案都在当前技术的范围内。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
MOONRAY: A permanent high-energy cosmic-ray observatory on the surface of the Moon

The forthcoming decades will see a rapid development of space programs aiming at the implementation of habitats on our satellite. Therefore it makes sense to evaluate the feasibility of a permanent cosmic-ray (CR) observatory on the Moon. Its large sensitive area would allow to carry out a very rich observational program over a time span of a few decades with an unprecedented energy reach. A thorough exploration of the energy region around the CR spectral anomaly located at a few PeV, also known as the “knee”, will become possible.

In this paper we propose an innovative concept of a modular lunar observatory designed to overcome the limitations of the present generation of cosmic-ray telescopes in Low Earth Orbit. It consists of an array of fully independent modules with limited individual size and weight. This would allow an ample flexibility in the gradual deployment of a progressively larger active volume, while ensuring the collection of meaningful scientific data during the intermediate stages of its implementation. Each independent module consists of three main instruments: a combined Charge and Time-of-Flight detector to identify individual elements from proton to nickel (and beyond), a tracker providing the direction and impact point of the incident particle, and a calorimeter to measure its kinetic energy. The design of each instrument contains innovative solutions that are well within the reach of the present technology.

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来源期刊
Astroparticle Physics
Astroparticle Physics 地学天文-天文与天体物理
CiteScore
8.00
自引率
2.90%
发文量
41
审稿时长
79 days
期刊介绍: Astroparticle Physics publishes experimental and theoretical research papers in the interacting fields of Cosmic Ray Physics, Astronomy and Astrophysics, Cosmology and Particle Physics focusing on new developments in the following areas: High-energy cosmic-ray physics and astrophysics; Particle cosmology; Particle astrophysics; Related astrophysics: supernova, AGN, cosmic abundances, dark matter etc.; Gravitational waves; High-energy, VHE and UHE gamma-ray astronomy; High- and low-energy neutrino astronomy; Instrumentation and detector developments related to the above-mentioned fields.
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