SEARCH FOR THE THIRD HARMONIC OF TYPE III BURSTS RADIO EMISSION AT DECAMETER WAVELENGTHS

Автор(и)

  • A. I. Brazhenko Poltava gravimetrical observatory of Institute of geophysics, National Academy of Sciences of Ukraine, Poltava, Ukraine, Ukraine
  • V. N. Melnik Institute of Radio Astronomy, National Academy of Sciences of Ukraine, Kharkov, Ukraine, Ukraine
  • A. A. Konovalenko Institute of Radio Astronomy, National Academy of Sciences of Ukraine, Kharkov, Ukraine, Ukraine
  • O. S. Pylaev Institute of Radio Astronomy, National Academy of Sciences of Ukraine, Kharkov, Ukraine, Ukraine
  • A. V. Frantsuzenko Poltava gravimetrical observatory of Institute of geophysics, National Academy of Sciences of Ukraine, Poltava, Ukraine, Ukraine
  • V. V. Dorovskyy Institute of Radio Astronomy, National Academy of Sciences of Ukraine, Kharkov, Ukraine, Ukraine
  • R. V. Vashchishin Poltava gravimetrical observatory of Institute of geophysics, National Academy of Sciences of Ukraine, Poltava, Ukraine, Ukraine
  • H. O. Rucker Space Research Institute, Austrian Academy of Sciences, Graz, Austria, Austria

DOI:

https://doi.org/10.18524/1810-4215.2012.25.83355

Ключові слова:

type III bursts, drift rate, duration, polarization, second harmonic, third harmonic, decameter wavelength range.

Анотація

The results of observations of trio bursts consisting of type III bursts are presented in this paper. The instantaneous frequency ratio of trio components is near 1:2:3. We analyze flow, duration, frequency drift rate and polarization of trio components as well as dependencies of these characteristics on frequency.

Посилання

Kundu M.R.: 1965, Solar Radio Astronomy, Interscience Publ., New York.

Benz A. O.: 1973, Nat. Phys. Sci., 242, 39.

Stewart R.T.: 1962, CSIRO Division of Radiophysics Report RPR, 142.

Zheleznyakov V.V., Zlotnik E.Ya.: 1974, Solar Phys., 36, 451.

Takakura T., Yousef S.: 1974,Sol. Phys., 36, 451.

Cairns I. H.: 1988, J. Geophys. Res.,93, 858.

Kliem B., Kruger A., Treumann R. A.: 1992, Sol. Phys., 140, 149.

Yoon P.H., Gaelzer R., Umeda T., Omura Y., Matsumoto H.: 2003, Phys. Plasmas, 10, 364.

Yi S., Yoon P.H., Ryu C.-M.: 2007, Phys. Plasmas, 14, 013301.

Tongnyeol Rhee, Chang-Mo Ryu, Minho Woo, Helen H. Kaang, Sumin Yi, and Peter H. Yoon: 2009, Astro phys. J., 694:618 625.

Zlotnik E.Ya., Klassen A., Klein K.-L., Mann G.: 1998, A&A, 331, 1087.

Dorovskyy V.V., Mel'Nik V.N., Konovalenko A.A., Rucker H.O., Abranin E.P., Stanislavsky A.A., Le-cacheux A.: 2007, European Planetary Science Con-gress, 688.

Wild J.P.: 1950, Aust.J.Sci.Res., 3, 541.

Melnik V.N., Konovalenko A.A., Rucker H.O., Boiko A.I., Dorovskyy V.V., Abranin E.P., Lecacheux A.: 2011, Solar Phys., 269, 2.

Boiko A.I., Mel'nik,V.N., Konovalenko A.A., Rucker H.O., Abranin E.P., Dorovskyy V.V., Lecacheux A.: 2010, PRE VII, 367.

##submission.downloads##

Опубліковано

2012-11-16

Номер

Розділ

Статті