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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3894
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dc.contributor.authorCecatto, J. R-
dc.contributor.authorSawant, H. S-
dc.contributor.authorFernandes, F. C. R-
dc.contributor.authorKrishan, V-
dc.contributor.authorNeri, J. A. C. F-
dc.contributor.authorMoraes, J. C-
dc.date.accessioned2008-09-25T12:56:07Z-
dc.date.available2008-09-25T12:56:07Z-
dc.date.issued2003-
dc.identifier.citationAdvances in Space Research, Vol. 32, No. 12, pp. 2533 - 2537en
dc.identifier.issn0273-1177-
dc.identifier.urihttp://hdl.handle.net/2248/3894-
dc.descriptionRestricted Access-
dc.description.abstractType-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 presenteden
dc.language.isoenen
dc.publisherElsevier B. V.en
dc.relation.urihttp://dx.doi.org/10.1016/j.asr.2003.03.010en
dc.rights© Elsevier B.V. All rights reserved.-
dc.subjectBrazilian solar spectroscopeen
dc.subjectElectron-beamsen
dc.subjectRadio-burstsen
dc.subjectEmissionen
dc.subjectBSSen
dc.titleHigh resolution time profile of decimetric type-III burstsen
dc.typeArticleen
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