High resolution time profile of decimetric type-III bursts

Cecatto, J. R; Sawant, H. S; Fernandes, F. C. R; Krishan, V; Neri, J. A. C. F; Moraes, J. C

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dc.contributor.author	Cecatto, J. R
dc.contributor.author	Sawant, H. S
dc.contributor.author	Fernandes, F. C. R
dc.contributor.author	Krishan, V
dc.contributor.author	Neri, J. A. C. F
dc.contributor.author	Moraes, J. C
dc.date.accessioned	2008-09-25T12:56:07Z
dc.date.available	2008-09-25T12:56:07Z
dc.date.issued	2003
dc.identifier.citation	Advances in Space Research, Vol. 32, No. 12, pp. 2533 - 2537	en
dc.identifier.issn	0273-1177
dc.identifier.uri	http://hdl.handle.net/2248/3894
dc.description	Restricted Access
dc.description.abstract	Type-III bursts are signatures of the electron beams accelerated during the solar flares, their observation and investigation provide information of the acceleration processes, the characteristics of the exciting agent and the acceleration site. The Brazilian Solar Spectroscope (BSS), in operation at INPE, Brazil, have recorded type-III radio bursts in decimetric range (2050 2250 MHz) with high time resolution of 20 ms. Decimetric reverse drift bursts are possibly generated in a dense loop by electron beams travelling towards the photosphere. Hence their time profiles should carry signatures of the density inhomogenities in the loop. Here the temporal and spectral characteristics of decimetric type-III bursts are presented	en
dc.language.iso	en	en
dc.publisher	Elsevier B. V.	en
dc.relation.uri	http://dx.doi.org/10.1016/j.asr.2003.03.010	en
dc.rights	© Elsevier B.V. All rights reserved.
dc.subject	Brazilian solar spectroscope	en
dc.subject	Electron-beams	en
dc.subject	Radio-bursts	en
dc.subject	Emission	en
dc.subject	BSS	en
dc.title	High resolution time profile of decimetric type-III bursts	en
dc.type	Article	en