1979
DOI: 10.1086/157504
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Spectral evolution of multiply impulsive solar bursts

Abstract: Hard X-ray and microwave observations of multiply-impulsive solar bursts, identified in the OSO-S data, have been analyzed in a search for the physical basis of the multiplicity of spikes within these events. Spectra in both frequency ranges have been used to determine whether or not the source p roperties change from peak to peak within individual bursts. Two categories of microwave spectral behaviour have been identified: those events during which the microwave turnover frequency and spectral shape remain th… Show more

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Cited by 7 publications
(7 citation statements)
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“…Although a least-squares fitting routine (as was used in the analysis described in Karpen et al, 1979) would provide the most accurate determinations of the spectral index, y, and the normalization constant, A, this procedure is far too time-consuming to be practical for analysis of thousands of spectra. A less precise but adequate technique was implemented, wherein 3' is the weighted mean of the spectral indices determined for each pair of energy channels showing significant flux above the noise level; a pair consists of Channel 2 and one of the higher-energy channels (see Crannell et al, 1978, Table 1).…”
Section: Methods Of Analysis and Test Of The Modelmentioning
confidence: 99%
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“…Although a least-squares fitting routine (as was used in the analysis described in Karpen et al, 1979) would provide the most accurate determinations of the spectral index, y, and the normalization constant, A, this procedure is far too time-consuming to be practical for analysis of thousands of spectra. A less precise but adequate technique was implemented, wherein 3' is the weighted mean of the spectral indices determined for each pair of energy channels showing significant flux above the noise level; a pair consists of Channel 2 and one of the higher-energy channels (see Crannell et al, 1978, Table 1).…”
Section: Methods Of Analysis and Test Of The Modelmentioning
confidence: 99%
“…These events were chosen from the larger set of multiply-impulsive bursts, initially selected according to the criteria outlined by Karpen et al (1979), by requiring sufficient X-ray flux to allow determination of the thick-target parameters F(25) and 3' throughout most, if not all, of the event. Table I lists the bursts and the time periods over which they were tested for the presence of betatron acceleration.…”
Section: Application To the Multiple-spike Burstsmentioning
confidence: 99%
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