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Перегляд Відділення фізики і астрономії за автором "Abranin, E.P."

Репозиторій DSpace/Manakin

Перегляд Відділення фізики і астрономії за автором "Abranin, E.P."

Сортувати за: Порядок: Результатів:

  • Konovalenko, A.A.; Stanislavsky, A.A.; Abranin, E.P.; Dorovsky, V.V.; Mel'nik, V.N. (Кинематика и физика небесных тел, 2005)
    We report the results of UTR-2 radio telescope observations of an absorption burst at the decameter range. This event is associated with two consecutive M-class flares and happened after the second M-flare. The latter flare ...
  • Boiko, A.I.; Melnik, V.N.; Konovalenko, A.A.; Abranin, E.P.; Dorovskyy, V.V.; Rucker, H.O. (Advances in Astronomy and Space Physics, 2012)
    We report on the observations of solar type IV burst and its precursors on the 13 of July 2004 at frequencies 10 − 30 MHz. The radio telescope UTR-2 observational data compiled from SOHO, WIND, NDA, RHESSI, GOES data were ...
  • Boiko, A.I.; Mel'nik, V.N.; Konovalenko, A.A.; Rucker, H.O.; Abranin, E.P.; Dorovskyy, V.V.; Lecacheux, A. (Advances in Astronomy and Space Physics, 2011)
    We report on the observations of powerful (fluxes are larger than 10⁻¹⁹ W m⁻² Hz⁻¹) solar Type III bursts at frequencies 10 − 30 MHz. Recordings of 163 bursts, observed in July 2002 and of 231 bursts observed in August ...
  • Brazhenko, A.I.; Bulatsen, V.G.; Vashchishin, R.V.; Frantsuzenko, A.V.; Konovalenko, A.A.; Falkovich, I.S.; Abranin, E.P.; Ulyanov, O.M.; Zakharenko, V.V.; Lecacheux, A.; Rucker, H. (Кинематика и физика небесных тел, 2005)
    The description of the new decameter radiopolarimeter is submitted. It is created based on the phased array URAN-2, which is the greatest decameter array in the world after UTR-2, having the effective area about 30 000 m2, ...
  • Mel'nik, V.N.; Konovalenko, A.A.; Abranin, E.P.; Dorovsky, V.V.; Lisachenko, V.N.; Stanislavsky, A.A.; Rucker, H.O.; Lecacheux, A. (Кинематика и физика небесных тел, 2005)
    Results of observations of the solar sporadic radio emission in decameter range are presented. These observations were carried out at UTR-2 radio telescope with 60-channel spectrometer and DSP (Digital Spectral Polarimeter) ...

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