Optical effects of the operation of the onboard engine of the Progress M-17M spacecraft at thermospheric heights


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This paper presents the results of optical observations in the active space experiment “Radar-Progress” on April 17, 2013, after switching on the approach-correction engine of the Progress M-17M cargo spacecraft at thermospheric heights (412 km), are presented in this paper. During engine operation, a region of enhanced emission intensity has been recorded. It was presumably related to the scatter of twilight solar emission at the engine exhausts in the cargo spacecraft orbit and, probably to the occurrence of an additional emission in the atomic oxygen line [OI] 630 nm. The maximum observed dimensions of the emission region were ~350 and ~250 km along the orbit and across it, respectively. The velocity of the expansion of the emission region at the first moments after the initiation of engine operation was ~7 and ~3.5 km/s along the orbit and across it, respectively. The maximum intensity of the disturbed region is estimated to be a value equivalent to ~40–60 R within the spectral band of 2 nm. No optical manifestation, which would exceed the natural variations in brightness of the night airglow and which would be related to possible large-scale modification of the ionosphere, was detected in the natural emission lines [O] 557.7 and 630.0 nm in a zone remote from the place of injection of engine exhausts.

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A. Mikhalev

Institute of Solar–Terrestrial Physics, Siberian Branch

编辑信件的主要联系方式.
Email: mikhalev@iszf.irk.ru
俄罗斯联邦, ul. Lermontova 126a, Irkutsk, 664033

V. Khakhinov

Institute of Solar–Terrestrial Physics, Siberian Branch

Email: mikhalev@iszf.irk.ru
俄罗斯联邦, ul. Lermontova 126a, Irkutsk, 664033

A. Beletskii

Institute of Solar–Terrestrial Physics, Siberian Branch

Email: mikhalev@iszf.irk.ru
俄罗斯联邦, ul. Lermontova 126a, Irkutsk, 664033

V. Lebedev

Institute of Solar–Terrestrial Physics, Siberian Branch

Email: mikhalev@iszf.irk.ru
俄罗斯联邦, ul. Lermontova 126a, Irkutsk, 664033

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