Abstract
A STACK of track-recording plastic detectors was exposed outside the Apollo 16 lunar module so that we could study the chemical Composition, energy spectra and origin of interplanetary heavy ions with 0.2≲E≲150 MeV/nucleon. The relative abundances of secondary nuclei such as LiBeB and the elements 17≤Z≤25 as a function of energy should be directly related to the galactic cosmic ray contribution because they are extremely rare in the Sun and in solar flare particles.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Paper version not known
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
