为太空飞行器定向传感器设计星表的特点

IF 0.6 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS
G. A. Avanesov, Ya. D. Elyashev
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引用次数: 0

摘要

摘要 简要介绍了俄罗斯科学院空间研究所(IKI RAS)创建恒星方位传感器和为其编制恒星目录的历史。介绍了 20 世纪 70 年代初从载人空间站 Salyut-2 号和-3 号对恒星和地球表面进行同步拍摄的实验。说明了当时将照片输入电子计算机(计算机)的困难。在 SAO、Hipparcos 和 Gaia 星表的基础上,围绕天球中最亮的恒星编制了大约 11000 个微型星表。每个微目录的中心包含一颗星等最高为 7.8 米的恒星,半径为 15′的范围内包含周围所有星等最高为 13 米的恒星。这些微型星表被合并成 "基本星表",在不久的将来将用于为 BOKZ 系列航天器的方位传感器编制星表。为了使用基本星表,开发了两个程序,并在测试模式下使用:星表指南和星空管理器。第一个程序用于查看基础星表,显示其碎片,并根据指定参数编制恒星列表。第二个程序具有计算和分析性质。它包含 BOKZ 系列恒星方位传感器的数学模型,以及可对星载数据处理中最微妙的元素进行详细建模的数学装置。这两个程序都可以在手动和自动模式下运行。在几颗恒星上手动完成的一连串操作可以在大量恒星上自动执行。文章介绍了基本目录的结构和内容,还说明了如何使用专门为此开发的程序来处理该目录。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Features of Designing a Star Catalog for Orientation Sensors of Space Vehicles

Features of Designing a Star Catalog for Orientation Sensors of Space Vehicles

Abstract

A brief history of the creation of star orientation sensors at the Space Research Institute of the Russian Academy of Sciences (IKI RAS) and star catalogs for them is presented. An experiment carried out in the early 1970s on synchronous photography of stars and the Earth’s surface from the manned stations Salyut-2 and -3 is described. The difficulties of entering photographs into electronic computers (computers) of that time are shown. Based on the SAO, Hipparcos and Gaia star catalogs, about 11000 microcatalogs have been compiled around the brightest stars in the celestial sphere. Each of them contains in the center one star with a magnitude of up to 7.8m and all the surrounding stars up to 13m within a radius of 15′. The microcatalogs are combined into the “Basic Star Catalog,” which in the near future will be used to compile onboard star catalogs for the orientation sensors of the BOKZ family of spacecraft. To work with the base catalog, two programs have been developed and are used in test mode: Catalog Guide and Star Manager. The first program is designed to view the base catalog, visualize its fragments and compile lists of stars with specified parameters. The second program is of a computational and analytical nature. It contains mathematical models of star orientation sensors of the BOKZ family, as well as a mathematical apparatus that allows for detailed modeling of the most subtle elements of onboard data processing. Both programs can operate in manual and automatic modes. A sequence of actions worked out manually on several stars can then be performed automatically for large lists of stars. The article describes the structure and content of the base directory, and also illustrates working with it using programs specially developed for this purpose.

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来源期刊
Solar System Research
Solar System Research 地学天文-天文与天体物理
CiteScore
1.60
自引率
33.30%
发文量
32
审稿时长
6-12 weeks
期刊介绍: Solar System Research publishes articles concerning the bodies of the Solar System, i.e., planets and their satellites, asteroids, comets, meteoric substances, and cosmic dust. The articles consider physics, dynamics and composition of these bodies, and techniques of their exploration. The journal addresses the problems of comparative planetology, physics of the planetary atmospheres and interiors, cosmochemistry, as well as planetary plasma environment and heliosphere, specifically those related to solar-planetary interactions. Attention is paid to studies of exoplanets and complex problems of the origin and evolution of planetary systems including the solar system, based on the results of astronomical observations, laboratory studies of meteorites, relevant theoretical approaches and mathematical modeling. Alongside with the original results of experimental and theoretical studies, the journal publishes scientific reviews in the field of planetary exploration, and notes on observational results.
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