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On the correlation between exciter duration and decay constant of solar decameter Type III radio bursts

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dc.contributor.author Subramanian, K. R
dc.contributor.author Krishan, V
dc.contributor.author Sastry, Ch. V
dc.date.accessioned 2008-12-17T16:46:59Z
dc.date.available 2008-12-17T16:46:59Z
dc.date.issued 1981-04
dc.identifier.citation Solar Physics, Vol. 70, No. 2, pp. 375 - 379 en
dc.identifier.issn 0038-0938
dc.identifier.uri http://hdl.handle.net/2248/4107
dc.description.abstract It 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 proposed en
dc.language.iso en en
dc.publisher Kluwer Academic Publishers en
dc.relation.uri http://adsabs.harvard.edu/abs/1981SoPh...70..375S en
dc.relation.uri http://dx.doi.org/10.1007/BF00151341 en
dc.subject Decametric Waves en
dc.subject Solar Physics en
dc.subject Type 3 Bursts en
dc.subject Correlation en
dc.subject Plasma-Particle Interactions en
dc.subject Solar Corona en
dc.title On the correlation between exciter duration and decay constant of solar decameter Type III radio bursts en
dc.type Article en


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