ON THE HARMONIC COUPLING OF COMPONENTS IN PAIRS OF IIIb–III BURSTS AT DECAMETER WAVELENGTHS

Radio Physics and Radio Astronomy

H. O. Rucker¹  M. Panchenko¹  V. N. Melnik²  V. V. Dorovskyy²  A. V. Frantsuzenko³  A. I. Brazhenko³ 

[1] Institut für Weltraumforschung, Österreichische Akademie der Wissenschaften, Schmiedlstraße 6, Graz, 8042, Österreich, Austria;Institute of Radio Astronomy, National Academy of Sciences of Ukraine, 4, Mystetstv St., Kharkiv, 61002, Ukraine;Poltava Gravimetric Observatory, S. Subbotin Institute of Geophysics, National Academy of Sciences of Ukraine, 27/29, Miasoiedov St., Poltava, 36014, Ukraine;

关键词: sun;    radio emission;    decameter wavelengths;    iiib-iii bursts;    duration;    frequency drift;    polarization;    plasma mechanism of radio emission;   

DOI  :  10.15407/rpra20.02.099

来源: DOAJ

【 摘 要 】

The properties of IIIb–III pairs observed by the URAN-2 radio telescope at frequencies 16-32 MHz are analyzed. Observations of these bursts were hold in April, June and September 2011. Durations, frequency drift rates, simultaneous frequency ratio of pairs components and their polarizations are analyzed. Pro and contra of IIIb–III harmonic connection are discussed.

【 授权许可】

Unknown