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Decameter Type III-Like Bursts

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Abstract

We report the first observations of Type III-like bursts at frequencies 10 – 30 MHz. More than 1000 such bursts during 2002 – 2004 have been analyzed. The frequency drift of these bursts is several times that of decameter Type III bursts. A typical duration of the Type III-like bursts is 1 – 2 s. These bursts are mainly observed when the source active region is located within a few days from the central meridian. The drift rate of the Type III-like bursts can take a large value by considering the velocity of Type III electrons and the group velocity of generated electromagnetic waves.

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Authors and Affiliations

  1. Institute of Radio Astronomy, Ukrainian Academy of Sciences, Kharkov, Ukraine

    V. N. Mel’nik, A. A. Konovalenko, B. P. Rutkevych, V. V. Dorovskyy, E. P. Abranin & A. A. Stanislavskii

  2. Space Research Institute, Austrian Academy of Sciences, Graz, Austria

    H. O. Rucker

  3. Gravimetrical Observatory, Poltava, Ukraine

    A. I. Brazhenko

  4. Departement de Radioastronomie, Observatoire de Paris, Paris, France

    A. Lecacheux

Authors
  1. V. N. Mel’nik
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  2. A. A. Konovalenko
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  3. H. O. Rucker
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  4. B. P. Rutkevych
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  5. V. V. Dorovskyy
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  6. E. P. Abranin
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  7. A. I. Brazhenko
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  8. A. A. Stanislavskii
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  9. A. Lecacheux
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Corresponding author

Correspondence to B. P. Rutkevych.

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Mel’nik, V.N., Konovalenko, A.A., Rucker, H.O. et al. Decameter Type III-Like Bursts. Sol Phys 250, 133–145 (2008). https://doi.org/10.1007/s11207-008-9166-z

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  • DOI: https://doi.org/10.1007/s11207-008-9166-z

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