AbstractThe 22min long decimetric type IV radio event observed during the decay phase of the June 6, 2000 flare simultaneously by the Brazilian Solar Spectroscope (BSS) and the Ondřejov radiospectrograph in frequency range 1200–4500MHz has been analyzed. We have found that the characteristic periods of about 60s belong to the long-period spectral component of the fast wave trains with a tadpole pattern in their wavelet power spectra. We have detected these trains in the whole frequency range 1200–4500MHz. The behavior of individual wave trains at lower frequencies is different from that at higher frequencies. These individual wave trains have some common as well as different properties. In this paper, we focus on two examples of wave trains in a loop segment and the main statistical parameters in their wavelet power and global spectra are studied and discussed.
Coronal fast wave trains of the decimetric type IV radio event observed during the decay phase of the June 6, 2000 flare
Advances in Space Research ; 43 , 10 ; 1479-1483
2009-01-27
5 pages
Article (Journal)
Electronic Resource
English
Sun , Corona , Flares , Radio radiation , MHD waves
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