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Radio Physics and Radio Astronomy

Publicado 4 números por año

ISSN Imprimir: 2152-274X

ISSN En Línea: 2152-2758

AN UNUSUAL SOLAR BURST AT DECAMETER WAVELENGTHS. 1. OBSERVATIONS

Volumen 3, Edición 4, 2012, pp. 279-284
DOI: 10.1615/RadioPhysicsRadioAstronomy.v3.i4.10
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SINOPSIS

An unusual burst was observed with the UTR-2 (Kharkiv, Ukraine) and URAN-2 (Poltava, Ukraine) radio telescopes on June 3, 2011. It was recorded in the frequency band 16 to 28 MHz. Its frequency drift rate (about 500 kHz/s) was positive at frequencies higher than 22 MHz and negative with drift rate 100 kHz/s at lower frequencies. The halfpower duration of this burst was about the same at all frequencies and made 17−22 s. The fine frequencytime structure was unusual, too. The maximum radio flux of the unusual burst at 24 MHz was about 103 s.f.u., and its polarization was negative making about 10 %. An interpretation of the unusual burst is suggested.

CITADO POR
  1. Stanislavsky A. A., THE ROLE OF RADIO WAVE PROPAGATION EFFECTS IN THE SOLAR CORONA TO INTERPRET THE BEHIND-LIMB BURSTS, Radio physics and radio astronomy, 21, 1, 2016. Crossref

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