The abundance of the radioactive isotope Al-26 in galactic cosmic rays

Details The abundance of the radioactive isotope Al-26 in galactic cosmic rays The abundance of the radioactive isotope Al-26 in galactic cosmic rays

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....9..147w&link_type=abstract

IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Late Papers. Volume 9 (A85-22801 0

Computer Science

Abundance, Aluminum 26, Galactic Cosmic Rays, Beryllium 10, Chronology, Radioactive Isotopes, Satellite Observation

Scientific paper

Satellite observations of the isotopic composition of aluminum in low energy cosmic rays (E/M = 200 MeV/amu) have been used to determine the abundance of the unstable isotope Al-26 (T1/2 = 0.87 Myr). The observed abundance ratio, Al-26/Al-27 = 0.036 (+0.037, -0.022), is in good agreement with previous balloon observations and yields a cosmic ray confinement time consistent with values based on the abundance of Be-10.

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