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Decimetric fine structures associated with the 6th June, 2000 solar flare

Published online by Cambridge University Press:  01 November 2006

Francisco C. R. Fernandes ,
José R. Cecatto ,
Maria C. Andrade ,
Reinaldo R. Rosa  and
Hanumant S. Sawant
Francisco C. R. Fernandes
Affiliation:
INPE – National Institute for Space Research, São José dos Campos, SP, Brazil email: guga@das.inpe.br. Present address: INPE/DAS, C.P. 515 12201-970, São José dos Campos, SP, Brazil.
José R. Cecatto
Affiliation:
INPE – National Institute for Space Research, São José dos Campos, SP, Brazil email: guga@das.inpe.br.
Maria C. Andrade
Affiliation:
INPE – National Institute for Space Research, São José dos Campos, SP, Brazil email: guga@das.inpe.br.
Reinaldo R. Rosa
Affiliation:
INPE – National Institute for Space Research, São José dos Campos, SP, Brazil email: guga@das.inpe.br.
Hanumant S. Sawant
Affiliation:
INPE – National Institute for Space Research, São José dos Campos, SP, Brazil email: guga@das.inpe.br.
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Abstract

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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 harmonic “zebra” 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.

Keywords

Sun: activitysolar flaresradio radiationdecimetric fine structures
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S233: Solar Activity and its Magnetic Origin , March 2006 , pp. 391 - 392
Copyright
© 2006 International Astronomical Union