Abstract

We report the temporal evolution of the long lasting solar flare observed on June 6, 2000 (15:00 - 17:00 UT) by the Brazilian Solar Spectroscope (BSS) at INPE. We emphasize the identification of the decimetric fine structures, such as fiber and zebra emissions, including the unique case of harmoniczebra emissions in the decimetric band reported, radio pulsations, type III bursts and variants, recorded during this event in the frequency range of (1.2 - 1.7 GHz). The main characteristics of fine structures recorded are presented.

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