Optical effects of running spacecraft engines in the lower thermosphere

Pub Date : 2022-12-24 DOI:10.12737/stp-84202207
A. Mikhalev, A. Beletsky, V. Lebedev, V. Khakhinov
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Abstract

This paper provides a brief overview on optical effects during operation of spacecraft (SC) onboard engines in the lower thermosphere according to observational data from the ISTP SB RAS Geophyisical Observatory. We present the results of detected disturbances in the night airglow during operation of SC vernier engines in the F2-region of the ionosphere in the “Radar–Progress” space experiment. With weights of combustion products of ≤10 kg injected by SC vernier engines, the atmospheric emission of [OI] 630.0 nm atomic oxygen is enhanced. We also show optical effects from the launches and passages of heavy launch vehicles “Energiya” from the Skif-DM spacecraft on May 15, 1987 and “Proton-M” from the Yamal-601 spacecraft on May 30, 2019 from Baikonur in the zone far from the launch site. We explore the possibility of enhanced [OI] 557.7 nm atmospheric emission due to chemical modification of the ionosphere in the E-region during the flight of the Energiya space system.
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航天器发动机在较低热层中运行的光学效应
本文根据ISTP SB RAS地球物理天文台的观测数据,简要概述了航天器(SC)机载发动机在低热层运行过程中的光学效应。我们介绍了在“雷达-进展”空间实验中,SC游标发动机在电离层F2区域运行期间探测到的夜间气辉干扰的结果。SC游标发动机喷射的燃烧产物重量≤10kg时,[OI]630.0nm原子氧的大气排放增强。我们还展示了1987年5月15日从Skif DM航天器发射的重型运载火箭“Energiya”和2019年5月30日从远离发射场的拜科努尔发射的“质子-M”的发射和通过的光学效果。我们探索了在Energiya空间系统飞行过程中,由于E区电离层的化学修饰,增强[OI]557.7nm大气发射的可能性。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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