Zobrazeno 1 - 10
of 25
pro vyhledávání: '"S. N. Oparin"'
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
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
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
Autor:
O. V. Morozov, I. A. Zhitnik, Yu. I. Logachev, I. P. Tindo, A. A. Pertsov, Yu. I. Denisov, A. V. Bogomolov, S. I. Svertilov, S. N. Kuznetsov, S. N. Oparin, S. S. Kavanosyan, A. P. Ignat'ev, Irina Myagkova
Publikováno v:
Solar System Research. 40:93-103
The SPR-N polarimeter onboard the CORONAS-F satellite allows the X-ray polarization degree to be measured in energy ranges of 20–40, 40–60, and 60–100 keV. To measure the polarization, the method based on the Thompson scattering of solar X-ray
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
Autor:
I. A. Zhitnik, Andrei Zhukov, J.-P. Delaboudiniere, A. A. Pertsov, V. A. Slemzin, A. N. Afanas'ev, R. A. M. Van der Linden, S. V. Kuzin, A. P. Ignat'ev, A. V. Mitrofanov, O. Bugaenko, S. N. Oparin, A. I. Stepanov, F. Auchere
Publikováno v:
Solar System Research. 39:489-500
The SPIRIT complex onboard the CORONAS-F satellite has routinely imaged the Sun in the 171, 175, 195, 284, and 304 A spectral bands since August 2001. The complex incorporates two telescopes. The Ritchey-Chretien telescope operates in the 171, 195, 2
Autor:
Irina Myagkova, A. K. Svirzhevskaya, A. V. Bogomolov, Igor Veselovsky, Sergey Kuzin, A. A. Nusinov, V. N. Ishkov, V. D. Kuznetsov, Karel Kudela, Vladimir Slemzin, Victor V. Grechnev, Y.I. Denisov, A. K. Markeev, S. I. Avdyushin, V. L. Shishov, R. V. Gorgutsa, Z. Smith, Alexei Dmitriev, A. V. Mitrofanov, A. A. Pertsov, G. S. Ivanov-Kholodnyi, M. A. Zeldovich, E. A. Eroshenko, Volker Bothmer, G. A. Zherebtsov, Georgy Zastenker, G. Lawrence, O. S. Yakovchouk, Yu. I. Stozhkov, P. M. Svidsky, A. P. Ignat'ev, I. I. Sobel'man, Alla Suvorova, A. N. Podorolsky, V. I. Vlasov, B. M. Kuzhevsky, O. P. Kolomiytsev, I. A. Zhitnik, Eduard Vashenyuk, V. G. Kurt, N. K. Sukhodrev, S. I. Svertilov, I. G. Mitrofanov, N. S. Svirzhevsky, O. V. Morozov, V. V. Fomichev, M. L. Litvak, I. M. Chertok, B.Y. Yushkov, M. I. Panasyuk, Victor Yanke, I. P. Tindo, S. N. Oparin, Olga Panasenco, Andrei Zhukov, S. N. Kuznetsov, M. Dryer, E. P. Romashets, Igor A. Krasheninnikov, A. A. Gnezdilov, S. K. Tokhchukova, I. V. Chashey, V. S. Makhmutov, Anatoli Petrukovich, Leonid Lazutin, G. A. Bazilevskaya, Yu. I. Logachev, A. V. Belov, L. N. Leshchenko, Lev Zelenyi, D. E. Sobolev, Yu. I. Yermolaev, K. A. Boyarchuk, Sergey A. Bogachev, V. M. Bogod
Publikováno v:
Cosmic Research. 42:435-488
We present new observational data on the phenomena of extremely high activity on the Sun and in the heliosphere that took place in October-November 2003. A large variety of solar and heliospheric parameters give evidence that the interval under consi
Autor:
V. V. Krutov, O. Bugaenko, A. Afanas'ev, S. Kuzin, Alexander V. Mitrofanov, Vladimir Slemzin, A. A. Pertsov, A. Umov, N. K. Sukhodrev, A. P. Ignat'ev, Igor A. Zhitnik, S. N. Oparin
Publikováno v:
Advances in Space Research. 32:473-477
The images of the solar corona from the limb out to the distance of about 5 solar radii have been obtained for the firs time in the XUV narrow spectral bands and monochromatic lines in the current experiment SPIRIT (SPectroheliographIc soft X-Ray Ima
Autor:
Yu. I. Logachev, O. V. Morozov, Karel Kudela, A. A. Pertsov, A. P. Ignat'ev, S. N. Kuznetsov, S. N. Oparin, Irina Myagkova, A. V. Bogomolov, B. Yu. Yushkov, S. I. Svertilov
Publikováno v:
Astronomy Letters. 29:199-204
We consider temporal, spectral, and polarization parameters of the hard X-ray and gamma-ray radiation observed during the solar flare of May 20, 2002, in the course of experiments with the SONG and SPR-N instruments onboard the Coronas-F spacecraft.
Autor:
V. A. Slemzin, A. M. Urnov, O. Bugaenko, S. N. Oparin, A. I. Stepanov, A. V. Mitrofanov, A. P. Ignat'ev, S. V. Kuzin, I. A. Zhitnik, A. A. Pertsov, V. V. Krutov
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 338:67-71
High-resolution temporal series of monochromatic full-Sun images in the L Mg xii emission line at 8.42 A have been obtained by the SPectroheliographIc X-Ray Imaging Telescope (SPIRIT) spectroheliograph on the CORONAS-Fsatellite. For a six-month perio