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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4107
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dc.contributor.authorSubramanian, K. R-
dc.contributor.authorKrishan, V-
dc.contributor.authorSastry, Ch. V-
dc.date.accessioned2008-12-17T16:46:59Z-
dc.date.available2008-12-17T16:46:59Z-
dc.date.issued1981-04-
dc.identifier.citationSolar Physics, Vol. 70, No. 2, pp. 375 - 379en
dc.identifier.issn0038-0938-
dc.identifier.urihttp://hdl.handle.net/2248/4107-
dc.description.abstractIt is observed that while there exists a strong correlation between the decay constant and the exciter duration for isolated type III radio bursts, it is absent for those type III radio bursts which are preceded by type IIIb radio bursts. A possible theoretical explanation for the presence of correlation in one case and lack of it in the other is proposeden
dc.language.isoenen
dc.publisherKluwer Academic Publishersen
dc.relation.urihttp://adsabs.harvard.edu/abs/1981SoPh...70..375Sen
dc.relation.urihttp://dx.doi.org/10.1007/BF00151341en
dc.subjectDecametric Wavesen
dc.subjectSolar Physicsen
dc.subjectType 3 Burstsen
dc.subjectCorrelationen
dc.subjectPlasma-Particle Interactionsen
dc.subjectSolar Coronaen
dc.titleOn the correlation between exciter duration and decay constant of solar decameter Type III radio burstsen
dc.typeArticleen
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