| タイトル | On the Age of Cosmic Rays as Derived from the Abundance of Be-10 |
| 本文（外部サイト） | http://hdl.handle.net/2060/19760012970 |
| 著者（英） | Hagen, F. A. |
| 著者所属（英） | NASA Goddard Space Flight Center |
| 発行日 | 1976-02-01 |
| 言語 | eng |
| 内容記述 | The isotopic composition of cosmic ray Be, B, C, and N was studied using a new range versus total light technique. Special emphasis was placed on the Be isotopes and in particular, on the radioactive isotope Be-10 due to its mean lifetime against decay. The experiment consisted of a thin trigger scintillator, an acrylic plastic Cerenkov detector and a spark chamber, followed by a totally active stack of 14 scintillation detectors. This stack of scintillators made possible the measurement of range, and also permitted the removal of interacting events by continuously monitoring their identities along their trajectories. The experiment was carried by balloon to atmospheric depths ranging from 3.5 to 5.0 g sq cm residual atmosphere for a total exposure time of 23 hr. Results indicate the survival of ( 55 + or -21) % of the Be-10 in the arriving cosmic rays; the data were interpreted using the leaky box model of cosmic ray propagation. |
| NASA分類 | SPACE RADIATION |
| レポートNO | 76N20058
NASA-TM-X-71085
X-660-76-54 |
| 権利 | No Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/186618 |
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