Theoretical and Experimental Aspects of Solar Flares Manifestation in Radiocarbon Abundance in Tree Rings

We describe our method of determining solar cosmic-ray flux and spectrum in the past, based on the comparison of different cosmogenic isotopes. For the period, AD 1781–1950, we have detected several intervals with a high probability of powerful solar flares.

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Veröffentlicht in:Radiocarbon 1992, Vol.34 (2), p.247-253
Hauptverfasser: Kostantinov, A. N., Levchenko, V. A., Kocharov, G. E., Mikheeva, I. B., Cecchini, Stefano, Galli, Menotti, Nanni, Teresa, Povinec, Pavel, Ruggiero, Livio, Salomoni, Agostino
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Sprache:eng
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Zusammenfassung:We describe our method of determining solar cosmic-ray flux and spectrum in the past, based on the comparison of different cosmogenic isotopes. For the period, AD 1781–1950, we have detected several intervals with a high probability of powerful solar flares.
ISSN:0033-8222
1945-5755
DOI:10.1017/S0033822200013692