罗蒙诺索夫任务上的空间实验研究伽玛射线暴和探测器

A. Amelushkin, V. Bogomolov, V. Benghin, G. Garipov, E. Gorbovskoy, B. Grossan, P. Klimov, B. Khrenov, J. Lee, V. Lipunov, G. Na, M. Panasyuk, I. Park, V. Petrov, G. Smoot, S. Svertilov, Y. Shprits, N. Vedenkin, I. Yashin
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引用次数: 3

摘要

罗蒙诺索夫飞船上的一些实验现在正在与其他组织合作,在密歇根州立大学SINP进行准备。罗蒙诺索夫任务的主要思想是研究极端天体物理现象,如宇宙伽马射线暴和超高能量宇宙射线。这些现象与早期宇宙中非常遥远的天体发生的过程有关,并为我们提供了关于宇宙演化第一阶段的信息。因此,罗蒙诺索夫任务的科学设备包括若干仪器,用于光学、紫外线、x射线和伽马射线方面的伽马射线暴观测,以及大口径望远镜,用于通过探测大气中的电离光轨迹来研究超高能量粒子。介绍了这些仪器的主要参数和简要说明。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
SPACE EXPERIMENTS ON-BOARD OF LOMONOSOV MISSION TO STUDY GAMMA-RAY BURSTS AND UHECRS
The number of experiments on-board Lomonosov spacecraft are preparing now at SINP MSU in co-operation with other organisations. The main idea of Lomonosov mission is to study extreme astrophysical phenomena, such as cosmic gamma-ray bursts and ultra-high energy cosmic rays. These phenomena connect with processes occurred in very distant astrophysical objects of the Early Universe and give us information about first stages of Universe evolution. Thus, the Lomonosov mission scientific equipment includes several instruments for gamma-ray burst observation in optics, ultra-violet, X-rays and gamma-rays and the wide aperture telescope for ultra-high energy particle study by detection of ionisation light along its tracks in the atmosphere. The main parameters and a brief description of these instruments are presented.
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