Author:
Castagnoli Giuliana,Lal Devendra
Abstract
This paper is concerned with the expected deviations in the production rate of natural 14C on the earth due to changes in solar activity. We review the published estimates of the global production rates of 14C due to galactic and solar cosmic ray particles, and present new estimates of the expected secular variations in 14C production, taking into account the latest information available on galactic cosmic ray modulation and long-term variations in solar activity.
Publisher
Cambridge University Press (CUP)
Subject
General Earth and Planetary Sciences,Archeology
Reference82 articles.
1. Reedy R C , 1977, Solar proton fluxes since 1956; Lunar sci conf, 8th, Proc, p 825–839.
2. Agrawal S P , Ananth A G , Bemalkhedkar M M , Kargathra L V , and Rao U R , 1974, High energy cosmic ray intensity increases of non-solar origin and the unusual forbush decrease of August 1972: Jour Geophys Research, v 79, no. 16, p 2269–2280.
3. Lassus de , St-Genies C , and Tobailem J , 1972, Sections efficaces des reactions nucléaires induites par protons, deutons, particules alpha. II. Fluor, neon, sodium and magnesium: Centre d'Etudes Nucléaires de Saclay Rept CEA-N-1466 (2).
4. Ramaty R , Kozlovsky B , and Lingenfelter R E , 1975, Solar gamma rays: Space Sci Rev, v 18, p 341–388.
Cited by
226 articles.
订阅此论文施引文献
订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献