Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Aleksandr Beletsky"'
Publikováno v:
Solar-Terrestrial Physics. 8:73-77
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 di
Publikováno v:
Solar-Terrestrial Physics, Vol 7, Iss 3, Pp 53-67 (2021)
Peculiarities of 557.7 and 630.0 nm emissions observed in the second step of the magnetic storm main phase at the mid-latitude observatory Tory (52° N, 103° E) on March 17, 2015 are compared with the changes in ionospheric parameters above this sta
Autor:
Artem Setov, Aleksandr Beletsky, Roman Vasilyev, Konstantin Ratovsky, Aleksey Oinats, V. L. Frolov, Andrey Medvedev, Yury Yasyukevich
Publikováno v:
Solar-Terrestrial Physics, Vol 6, Iss 2, Pp 49-62 (2020)
The development of new devices for research in physics of the upper atmosphere and near-Earth space, which can be used to carry out controlled experiments on the modification of the ionosphere by powerful short-wave radiation, is an urgent task of mo
Autor:
Aleksandr Beletsky, Mikhail Tashchilin, Irina Medvedeva, Olga Zorkaltseva, Stepan Podlesny, Tatyana Syrenova, Ivan D. Tkachev, Aleksandr Mikhalev, Evgeniya Komarova, Maksim Artamonov, Roman Vasilyev, Konstantin Ratovsky
Publikováno v:
Solar-Terrestrial Physics, Vol 6, Iss 2, Pp 84-97 (2020)
Studies of the upper atmosphere have to be performed using optical photometric and spectrometric means. Modern devices allow precise photometry of the glow of the night atmosphere — airglow — with high temporal spatial and spectral resolution. As
Autor:
Evgeniya Komarova, Aleksey Podlesnyi, Tatyana Syrenova, Stepan Podlesny, Roman Vasilyev, Maxim Eselevich, Kirill Ivanov, Aleksandr Beletsky, Aleksandr Mikhalev
Publikováno v:
Solar-Terrestrial Physics, Vol 5, Iss 3, Pp 109-116 (2019)
The paper presents data on long-lived (~20–40 min) meteor trails. We describe a group of soliton-type meteor trails expanding at transonic speeds. Radio sounding data evidences that the latter include ~7–8 min ionization trails. We also consider
Autor:
Nozomu Nishitani, Ravil Rakhmatulin, Roman Vasilyev, Kazuo Shiokawa, Tatyana Syrenova, Aleksandr Beletsky, Aleksandr Pashinin, Aleksandr Mikhalev
Publikováno v:
Solar-Terrestrial Physics, Vol 5, Iss 2, Pp 39-44 (2019)
The paper presents the results on first synchronous observations of variations in auroral luminosity and geomagnetic field, made with high temporal resolution at the ISTP SB RAS high-latitude station Istok (70° N, 88° E) in September–December 201
Autor:
Maksim Artamonov, Mikhail Tashchilin, Stepan Podlesny, Geliy Zherebtsov, Roman Vasilyev, Aleksandr Beletsky, Aleksandr Mikhalev
Publikováno v:
Solar-Terrestrial Physics, Vol 4, Iss 4, Pp 42-47 (2018)
We study the spatiotemporal dynamics of mid-latitude aurora from observations in the south of Eastern Siberia during St. Patrick’s severe geomagnetic storm on March 17, 2015. We perform a morphological analysis of characteristics of the observed au
Autor:
Maksim Artamonov, G.A. Zherebtsov, Aleksandr Beletsky, Irina Medvedeva, Tatyana Syrenova, Aleksandr Mikhalev, Roman Vasilyev
Publikováno v:
Solar-Terrestrial Physics, Vol 3, Iss 3, Pp 61-75 (2017)
We describe the Fabry—Perot interferometer designed to study Earth’s upper atmosphere. We propose a modification of the existing data processing method for determining the Doppler shift and Doppler widening and also for separating the observed li
Publikováno v:
Solar-Terrestrial Physics, Vol 2, Iss 4, Pp 107-117 (2016)
This paper presents results of optical observations made during Radar-Progress Experiment performed on April 17, 2013 and July 30, 2014 after approach-correction engines (ACE) of Progress M-17M and Progress M-23M cargo spacecraft in the thermosphere