Abstract
After a solar flare we observe: (a) several bursts of type III; (b) in some cases a burst of type II. These phenomena become understandable when the radiospectrum is recorded: this is done with a cathode-ray tube on a 35 mm film.
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Reference
Kundu, M. R.: 1965, Solar Radio Astronomy, Interscience Publ., New York. See the spectra, notice especially the graphs pp. 297, 324, 325, 342, 357, 374, 376, 378.
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© 1969 D. Reidel Publishing Company, Dordrecht, Holland
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Minnaert, M.G.J. (1969). Radio Bursts after a Solar Flare (L). In: Practical Work in Elementary Astronomy. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-3414-2_48
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DOI: https://doi.org/10.1007/978-94-010-3414-2_48
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