JEM-EUSO计划框架下的EUSO@TurLab项目

IF 2.7 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
P. Barrillon, M. Battisti, A. Belov, M. Bertaina, F. Bisconti, S. Blin-Bondil, R. Bonino, F. Capel, R. Caruso, M. Casolino, G. Contino, G. Cotto, S. Dagoret-Campagne, F. Fenu, C. Fornaro, R. Forza, P. Gorodetzky, N. Guardone, A. Jung, P. Klimov, M. Manfrin, L. Marcelli, M. Mignone, H. Miyamoto, R. Mulas, M. Onorato, E. Parizot, L. Piotrowski, Z. Plebaniak, G. Prevot, J. Szabelski, G. Suino, Y. Takizawa, P. Tibaldi, C. Vigorito, A. Youssef
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引用次数: 4

摘要

EUSO@TurLab项目旨在进行实验,再现JEM-EUSO计划任务从低地球轨道看到的地球紫外线辐射。它利用TurLab设施,这是一个实验室,配备了直径5米,深度1米的旋转水箱,位于都灵大学物理系。所有的实验都是基于对即将在太空中飞行的探测器的预期响应的模拟来设计和执行的。2016年4月,作为JEM-EUSO计划的一部分,TUS探测器和最近的2019年10月的Mini-EUSO实验已被放置在轨道上,以绘制地球紫外线辐射图。因此,现在可以将TurLab进行的复制与在太空中检测到的实际图像进行比较,以了解预期信号再现的保真程度。我们表明,在考虑大气瞬变事件、漫射夜间背景光和人工光源的情况下,实验室测试在数量级上再现了从空间发射的紫外光的空间延伸和时间持续时间方面的测量结果,以及从单位时间每像素的预期计数方面的强度。因此,TurLab被发现是一个非常有用的设施,用于测试JEM-EUSO计划当前和未来任务的探测器的采集逻辑,以便在实验室中重现大气信号。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

The EUSO@TurLab project in the framework of the JEM-EUSO program

The EUSO@TurLab project in the framework of the JEM-EUSO program

The EUSO@TurLab project aims at performing experiments to reproduce Earth UV emissions as seen from a low Earth orbit by the planned missions of the JEM-EUSO program. It makes use of the TurLab facility, which is a laboratory, equipped with a 5 m diameter and 1 m depth rotating tank, located at the Physics Department of the University of Turin. All the experiments are designed and performed based on simulations of the expected response of the detectors to be flown in space. In April 2016 the TUS detector and more recently in October 2019 the Mini-EUSO experiment, both part of the JEM-EUSO program, have been placed in orbit to map the UV Earth emissions. It is, therefore, now possible to compare the replicas performed at TurLab with the actual images detected in space to understand the level of fidelity in terms of reproduction of the expected signals. We show that the laboratory tests reproduce at the order of magnitude level the measurements from space in terms of spatial extension and time duration of the emitted UV light, as well as the intensity in terms of expected counts per pixel per unit time when atmospheric transient events, diffuse nightlow background light, and artificial light sources are considered. Therefore, TurLab is found to be a very useful facility for testing the acquisition logic of the detectors of the present and future missions of the JEM-EUSO program and beyond in order to reproduce atmospheric signals in the laboratory.

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来源期刊
Experimental Astronomy
Experimental Astronomy 地学天文-天文与天体物理
CiteScore
5.30
自引率
3.30%
发文量
57
审稿时长
6-12 weeks
期刊介绍: Many new instruments for observing astronomical objects at a variety of wavelengths have been and are continually being developed. Furthermore, a vast amount of effort is being put into the development of new techniques for data analysis in order to cope with great streams of data collected by these instruments. Experimental Astronomy acts as a medium for the publication of papers of contemporary scientific interest on astrophysical instrumentation and methods necessary for the conduct of astronomy at all wavelength fields. Experimental Astronomy publishes full-length articles, research letters and reviews on developments in detection techniques, instruments, and data analysis and image processing techniques. Occasional special issues are published, giving an in-depth presentation of the instrumentation and/or analysis connected with specific projects, such as satellite experiments or ground-based telescopes, or of specialized techniques.
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