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A new investigation of microbursts at meter-decameter wavelengths

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dc.contributor.author Subramanian, K. R
dc.contributor.author Gopalswamy, N
dc.contributor.author Sastry, Ch. V
dc.date.accessioned 2008-07-24T05:16:06Z
dc.date.available 2008-07-24T05:16:06Z
dc.date.issued 1993-02
dc.identifier.citation Solar Physics, Vol. 143, No. 2, pp. 301 - 316 en
dc.identifier.issn 0038-0938
dc.identifier.uri http://hdl.handle.net/2248/2870
dc.description.abstract The results of a new investigation of microbursts at meter-decameter wavelengths are reported. Several properties of microbursts reported earlier are confirmed, and some new properties, such as time profile characteristics, flux density, and energy spectra are studied in order to compare the properties of microbursts with those of normal type III bursts. Electron beams of similar characteristics are found to generate both microbursts and type III bursts. Plasma waves generated by the electron beams due to beam-plasma instability are quickly isotropized as they scatter on the density fluctuations in the corona, leading to the low brightness temperature of microbursts. The resulting low levels of plasma waves produce transverse radiation of low brightness temperature. As a result of the isotropization, the second harmonic plasma emission dominates the fundamental, so that microbursts are expected to be primarily a harmonic plasma emission. en
dc.format.extent 1336983 bytes
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher Kluwer Academic Publishers en
dc.relation.uri http://adsabs.harvard.edu/abs/1993SoPh..143..301S en
dc.subject Solar physics en
dc.subject Solar radio bursts en
dc.subject Brightness temperature en
dc.subject Electron beams en
dc.subject Solar electrons en
dc.subject Type 3 bursts en
dc.title A new investigation of microbursts at meter-decameter wavelengths en
dc.type Article en


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