Search Results - "Marchenko, G P"

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  1. 1

    Flare on 2011 September 22 and coronal mass ejection from observations in the He i 10830-Å line by Akimov, L. A., Belkina, I. L., Marchenko, G. P.

    “…In this paper, we present the results from a study of the X1.4/2N flare and the accompanying coronal mass ejection (CME) on 2011 September 22 from observations…”
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    Journal Article
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    Quasi-periodicity of MgXII X-ray bursts revealed by CORONAS-F SPIRIT data for solar active regions by Akimov, L A, Beletskii, S A, Belkina, I L, Bugaenko, O I, Velikodskii, Yu I, Zhitnik, I A, Ignat'ev, A P, Korokhin, V V, Kuzin, S V, Marchenko, G P, Pertsov, A A

    Published in Astronomy reports (01-07-2005)
    “…A spectral analysis of a series of integrated MgXII 8.42 X-ray intensities recorded by the CORONAS-F SPIRIT spectroheliometer is presented. Statistically…”
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    Journal Article
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    Characterizing dark mantle deposits in the lunar crater Alphonsus by Shkuratov, Y.G., Ivanov, M.A., Korokhin, V.V., Kaydash, V.G., Basilevsky, A.T., Videen, G., Hradyska, L.V., Velikodsky, Y.I., Marchenko, G.P.

    Published in Planetary and space science (01-04-2018)
    “…We analyze available remote-sensing data of the crater Alphonsus, focusing on the analysis of the crater's dark mantle deposits (DMDs), which includes images…”
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    Journal Article
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    Solar chromosphere in the D3 helium line from spectra of the eclipse of March 29, 2006 by Marchenko, G. P., Akimov, L. A., Belkina, I. L., Velikodsky, Yu. I.

    Published in Kinematics and physics of celestial bodies (01-08-2011)
    “…We present the processing results of slitless chromospheric spectra in a D 3 helium line obtained during the solar eclipse of March 29, 2006. A…”
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  5. 5

    Solar chromosphere in the D^sub 3^ helium line from spectra of the eclipse of March 29, 2006 by Marchenko, G P, Akimov, L A, Belkina, I L, Velikodsky, Yu I

    Published in Kinematics and physics of celestial bodies (01-08-2011)
    “…We present the processing results of slitless chromospheric spectra in a D^sub 3^ helium line obtained during the solar eclipse of March 29, 2006. A…”
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    Journal Article
  6. 6

    Solar chromosphere in the D sub(3) helium line from spectra of the eclipse of March 29, 2006 by Marchenko, G P, Akimov, LA, Belkina, IL, Velikodsky, YuI

    Published in Kinematics and physics of celestial bodies (01-08-2011)
    “…We present the processing results of slitless chromospheric spectra in a D sub(3) helium line obtained during the solar eclipse of March 29, 2006. A…”
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    Journal Article
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    The north-south asymmetry of polarization of Jupiter: The causes of seasonal variations by Shalygina, O. S., Korokhin, V. V., Starukhina, L. V., Shalygin, E. V., Marchenko, G. P., Velikodsky, Yu. I., Starodubtseva, O. M., Akimov, L. A.

    Published in Solar system research (01-02-2008)
    “…We present new results obtained from the analysis of the seasonal variations in the asymmetry of polarization of light reflected by Jupiter. From the 23-year…”
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    The north-south asymmetry of polarization of Jupiter: The causes of seasonal variations by Shalygina, O S, Korokhin, V V, Starukhina, L V, Shalygin, E V, Marchenko, G P, Velikodsky, Yu I, Starodubtseva, O M, Akimov, L A

    Published in Solar system research (01-02-2008)
    “…We present new results obtained from the analysis of the seasonal variations in the asymmetry of polarization of light reflected by Jupiter. From the 23-year…”
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    Journal Article
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    New functional properties of albumin by Pentiuk, A A, Musin, R A, Marchenko, G P

    Published in Voprosy meditsinskoi khimii (01-05-1995)
    “…Effects of albumin on N-demethylation reactions of substrates in rat liver microsomes were studied in vitro. Albumin was found both to accelerate and to…”
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    Causes of Observed Long-Periodic Variations of the Polarization at Polar Regions of Jupiter by Shalygina, O. S, Korokhin, V. V, Shalygin, E. V, Marchenko, G. P, Velikodsky, Yu. I, Akimov, L. A, Starodubtseva, O. M

    Published 10-07-2006
    “…Data of 23-years of Jupiter polarimetric observations (1981- 2004) have been reprocessed using new improved technique. The data from other observers have been…”
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