Kj. Mathew et Svs. Murty, COSMIC-RAY PRODUCED NITROGEN IN EXTRA TERRESTRIAL MATTER, Proceedings of the Indian Academy of Sciences. Earth and planetary sciences, 102(3), 1993, pp. 415-437
Production rates of N-15 by both solar cosmic rays (SCR) and galactic
cosmic rays (GCR) have been calculated for moon, as well as meteorites
of various sizes. Our production rates of N-15 which considered both
the reaction channels O-16(p,pn)O-15 and (O(p,2p)N)-O-16-N-15 separate
ly are about 30% higher than those by Reedy (1981) who considered only
the channel O-16(p,pn)O-15 and used an empirical scaling factor to es
timate the contribution from (O(p,2p)N)-O-16-N-15. Production ratio N-
15/Ne-21 is composition dependent and hence is different for various s
ilicate minerals. Additionally the ratio N-15/Ne-21 is very sensitive
to the energy spectrum of the cosmic rays. This fact can be made use o
f in characterizing as well as in decoupling the SCR and GCR effects i
n extraterrestrial samples.