Zobrazeno 1 - 10
of 23
pro vyhledávání: '"O. I. Bugaenko"'
Autor:
N. K. Sukhodrev, S. N. Oparin, T. A. Shergina, Yu. S. Ivanov, A. A. Pertsov, Sergey A. Bogachev, L. A. Goncharov, S. G. Popov, A. M. Zykov, A. A. Reva, A. V. Mitrofanov, S. V. Shestov, I. A. Zhitnik, Sergey Kuzin, V. A. Solov’ev, A. S. Ulyanov, Vladimir Slemzin, O. I. Bugaenko, A. P. Ignat'ev
Publikováno v:
Solar System Research. 45:162-173
On February 26, 2009, the first data was obtained in the TESIS experiment on the research of the solar corona using imaging spectroscopy. The TESIS is a part of the scientific equipment of the CORONAS-PHO-TON spacecraft and is designed for imaging th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1b2fa609996f08f2250d4e5996dfaa91
https://doi.org/10.1134/s0038094611020110
https://doi.org/10.1134/s0038094611020110
Autor:
T. A. Shergina, A. L. Goncharov, S. G. Popova, A. V. Ignat’ev, S. V. Shestov, A. S. Ulyanov, V. A. Solov’ev, Sergey Kuzin, Vladimir Slemzin, A. M. Urnov, O. I. Bugaenko, M. S. Zykov, Yu. S. Ivanov, A. A. Reva, A. V. Mitrofanov, I. A. Zhitnik, Sergey A. Bogachev, A. A. Pertsov, N. K. Sukhodrev, S. N. Oparin
Publikováno v:
Bulletin of the Russian Academy of Sciences: Physics. 74:33-37
The CORONAS-Photon spacecraft was successfully launched in January 2009. Its scientific payload included the TESIS complex of telescopes and spectrometers, designed to obtain high spectral, temporal and spatial resolution solar corona images in soft
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3fa3e044c66916ec3ff666ab659a581e
https://doi.org/10.3103/s1062873810010090
https://doi.org/10.3103/s1062873810010090
Autor:
I. A. Zhitnik, O. I. Bugaenko, S. V. Shestov, Sergey A. Bogachev, A. P. Ignatiev, Sergey Kuzin, A.M. Mitrofanov, N. K. Sukhodrev, A. A. Pertsov, Vladimir Slemzin
Publikováno v:
Advances in Space Research. 43:1001-1006
TESIS is a set of solar imaging instruments in development by the Lebedev Physical Institute of the Russian Academy of Science, to be launched aboard the Russian spacecraft CORONAS-PHOTON in December 2008. The main goal of TESIS is to provide complex
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2997d1ef6cfcd3523fd47e1186c512b6
https://doi.org/10.1016/j.asr.2008.10.021
https://doi.org/10.1016/j.asr.2008.10.021
Autor:
A. I. Stepanov, A. A. Afanas’ev, O. I. Bugaenko, I. A. Zhitnik, A. A. Pertsov, A. P. Ignat'ev, Vladimir Slemzin, D. V. Lisin, Sergey Kuzin, V. A. Solov’ev, Yu. S. Ivanov
Publikováno v:
Instruments and Experimental Techniques. 51:702-710
The scientific purpose of the SPIRIT experiment is to study the space-time structures of phenomena of the solar activity using a set of X-ray instruments aboard the Koronas-F satellite. The system consists of the SRT-C six-channel telescope and the R
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ff5d218948965837f5b6a76c00ad994c
https://doi.org/10.1134/s0020441208050096
https://doi.org/10.1134/s0020441208050096
Autor:
A. A. Pertsov, V. G. Zandanov, I. M. Chertok, Sergey Kuzin, S. N. Oparin, A. I. Stepanov, V. V. Krutov, A. M. Uralov, Vladimir Slemzin, A. M. Urnov, M. A. Livshits, V. V. Grechnev, I. A. Zhitnik, A. P. Ignat'ev, Sergey A. Bogachev, O. I. Bugaenko
Publikováno v:
Solar System Research. 40:286-293
Large-scale hot features were detected and observed several times high in the solar corona in the high-temperature Mg XII line (T = 5–20 MK, T max = 10 MK) with the soft X-ray telescope of the SPIRIT instrumentation complex onboard the CORONAS-F sp
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3521630923670542575e49511aea6cfc
https://doi.org/10.1134/s0038094606040046
https://doi.org/10.1134/s0038094606040046
Autor:
V. Grechnev, S. Kuzin, O. I. Bugaenko, I. Chertok, A. A. Pertsov, A. P. Ignat'ev, Vladimir Slemzin, Igor A. Zhitnik
Publikováno v:
Advances in Space Research. 38:451-455
Based on observations with the EUV SPIRIT telescope aboard the CORONAS-F spacecraft, we analyze large-scale dimmings on the solar disk initiated by halo-type coronal mass ejections (CMEs). We address four powerful geo-effective eruptive events of Nov
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c456c8c22c31dc72fa6ded4c8b3ca0ba
https://doi.org/10.1016/j.asr.2004.12.024
https://doi.org/10.1016/j.asr.2004.12.024
Autor:
N. K. Sukhodrev, O. I. Bugaenko, A. A. Pertsov, V. A. Slemzin, Igor I Sobel'man, S. N. Oparin, A. P. Ignat'ev, A. M. Urnov, A. V. Mitrofanov, I. A. Zhithik, S. V. Kuzin
Publikováno v:
Solar System Research. 39:442-452
The main results of the SPIRIT experiment on imaging spectroscopy of the Sun in the soft X-ray and extreme vacuum UV range are presented. The results were obtained onboard the CORONAS-F satellite, which has been operating since July 2001. More than 4
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::dec9a7be5effe1528a2d5029337db79f
https://doi.org/10.1007/s11208-005-0057-7
https://doi.org/10.1007/s11208-005-0057-7
Autor:
Sergey Kuzin, G. P. Marchenko, Yu. I. Velikodskii, Viktor Korokhin, A. A. Pertsov, S. A. Beletskii, O. I. Bugaenko, A. P. Ignat'ev, Igor A. Zhitnik, I. L. Belkina, L. A. Akimov
Publikováno v:
Astronomy Reports. 49:579-586
A spectral analysis of a series of integrated MgXII 8.42 A X-ray intensities recorded by the CORONAS-F SPIRIT spectroheliometer is presented. Statistically significant peaks for periods in the intervals 12–30 min and 40–200 min were found in the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0febf97df6192d191d906f6447041231
https://doi.org/10.1134/1.1985955
https://doi.org/10.1134/1.1985955
Autor:
O. I. Bugaenko, V. Mikerov, E. Bogolubov, A. A. Pertsov, Sergey Kuzin, A. Monitch, E. Monitch
Publikováno v:
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 542:187-191
Two new types of luminescent CCD-detectors intended for fast neutron radiography and tomography with a cone neutron beam are described in the paper. A 6 cm thick luminescent screen made of polystyrene is used in the first one to convert fast neutrons
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f9cb65ed074c21fdeafc7cc173aa73b9
https://doi.org/10.1016/j.nima.2005.01.098
https://doi.org/10.1016/j.nima.2005.01.098