TY - JOUR
T1 - Physical basis of the transfort and composition of cosmic rays in the galaxy
AU - Gloeckler, G.
AU - Jokipii, J. R.
PY - 1969
Y1 - 1969
N2 - Consideration of cosmic-ray propagation leads naturally to an equilibrium model for cosmic-ray origin and storage in the galaxy. In this model the relative abundances of nuclei with substantially different charge values are nearly energy independent. We conclude that this simple, one- "component" model is consistent with observations of both the galactic primary (i.e., H1, He4, C, N, O, Fe) and secondary particles (He3, Li, Be, B).
AB - Consideration of cosmic-ray propagation leads naturally to an equilibrium model for cosmic-ray origin and storage in the galaxy. In this model the relative abundances of nuclei with substantially different charge values are nearly energy independent. We conclude that this simple, one- "component" model is consistent with observations of both the galactic primary (i.e., H1, He4, C, N, O, Fe) and secondary particles (He3, Li, Be, B).
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U2 - 10.1103/PhysRevLett.22.1448
DO - 10.1103/PhysRevLett.22.1448
M3 - Article
AN - SCOPUS:4243817016
SN - 0031-9007
VL - 22
SP - 1448
EP - 1453
JO - Physical review letters
JF - Physical review letters
IS - 26
ER -