OLVE-HERO轨道实验的蒙特卡罗模拟

IF 0.5 4区物理与天体物理 Q4 PHYSICS, PARTICLES & FIELDS

Physics of Particles and Nuclei Pub Date : 2025-05-20 DOI:10.1134/S1063779624701260

Kh. Karatash, I. Satyshev, L. G. Tkachev

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引用次数: 0

摘要

高能射线天文台（HERO）是一个基于电离量热计的空间实验项目，用于测量宇宙射线的光谱和成分。对于质子，装置的有效几何因子不小于12m2 sr，对于原子核和电子，装置的有效几何因子不小于16m2 sr。在大约5-7年的暴露期间，该任务将以高能量分辨率测量能量范围为1012 -1016 eV/粒子的宇宙射线的逐元素光谱。给出了用硼化闪烁体作为量热计一部分的蒙特卡罗模拟实验。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

Monte Carlo Simulation of the OLVE-HERO Orbital Experiment

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Monte Carlo Simulation of the OLVE-HERO Orbital Experiment

The High Energy Ray Observatory (HERO) is a project for a space experiment based on an ionization calorimeter to measure the spectrum and composition of cosmic rays. The effective geometric factor of the installation is not less than 12 m² sr for protons and not less than 16 m² sr for nuclei and electrons. During ~5–7 years of exposure, this mission will measure the element-by-element spectra of cosmic rays in the energy range 10¹² –10¹⁶ eV/particle with a high energy resolution. A Monte Carlo simulation of the experiment using a borated scintillator as a part of the calorimeter is presented.

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来源期刊

Physics of Particles and Nuclei 物理-物理：粒子与场物理

CiteScore

1.00

自引率

0.00%

发文量

116

审稿时长

6-12 weeks

期刊介绍： The journal Fizika Elementarnykh Chastits i Atomnogo Yadr of the Joint Institute for Nuclear Research (JINR, Dubna) was founded by Academician N.N. Bogolyubov in August 1969. The Editors-in-chief of the journal were Academician N.N. Bogolyubov (1970–1992) and Academician A.M. Baldin (1992–2001). Its English translation, Physics of Particles and Nuclei, appears simultaneously with the original Russian-language edition. Published by leading physicists from the JINR member states, as well as by scientists from other countries, review articles in this journal examine problems of elementary particle physics, nuclear physics, condensed matter physics, experimental data processing, accelerators and related instrumentation ecology and radiology.