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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4110
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dc.contributor.authorKrishan, V-
dc.contributor.authorSubramanian, K. R-
dc.contributor.authorSastry, Ch. V-
dc.date.accessioned2008-12-18T14:13:56Z-
dc.date.available2008-12-18T14:13:56Z-
dc.date.issued1980-06-
dc.identifier.citationSolar Physics, Vol. 66, No. 2, pp. 347 - 355en
dc.identifier.issn0038-0938-
dc.identifier.urihttp://hdl.handle.net/2248/4110-
dc.description.abstractSolar decameter bursts of Type IIIb are observed with a multichannel radiometer at wavelengths around 12m. The time and frequency resolutions were 10 ms and 100 kHz. Observations on the time structure of these bursts are presented. A theoretical model which accounts for various aspects of these bursts is proposed.en
dc.language.isoenen
dc.publisherKluwer Academic Publishersen
dc.relation.urihttp://dx.doi.org/10.1007/BF00150590en
dc.relation.urihttp://adsabs.harvard.edu/abs/1980SoPh...66..347Ken
dc.subjectAstronomical Modelsen
dc.subjectDecametric Wavesen
dc.subjectPulse Durationen
dc.subjectType 3 Burstsen
dc.subjectAtmosphericsen
dc.subjectElectric Fieldsen
dc.subjectElectromagnetic Radiationen
dc.subjectElectron Beamsen
dc.subjectHigh Resolutionen
dc.subjectMagnetic Fieldsen
dc.subjectPlasma Physicsen
dc.subjectPlasma-Particle Interactionsen
dc.titleObservations and interpretation of solar decameter type IIIb radio burstsen
dc.typeArticleen
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