Evidence for a common origin of the elec
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S. R. Kane
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Article
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1972
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Springer
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English
β 766 KB
Observations of impulsive solar flare X-rays > 10 keV made with the OGO-5 satellite are compared with ground based measurements of type III solar radio bursts in 10-580 MHz range. It is shown that the times of maxima of these two emissions, when detectable, agree within ~ 18 s. This maximum time dif