Abstract
Abstract The Brazilian Solar Spectroscope (BSS) as well as the radio spectrographs of the Ondřejov Observatory (OO) observed, in decimeter wavelengths, spectra consisting of groups of type III reverse drift (RS) bursts with time resolution of 50 ms and also observed a partial inverted long duration (about 25 s) U-type burst. The speeds of their exciting agents have been determined. The estimated speeds suggest that distinct exciters are responsible for the emissions of the inverted U-type and type-III RS bursts.
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