Be-7 nuclei produced by galactic cosmic rays and solar energetic particles, in the Earth's atmosphere

被引:19
|
作者
Yoshimori, M
Hirayama, H
Mori, S
Sasaki, K
Sakurai, H
机构
[1] Rikkyo Univ, Sch Sci, Toshima Ku, Tokyo 1718501, Japan
[2] Yamagata Univ, Sch Sci, Yamagata 9908560, Japan
关键词
D O I
10.1016/j.asr.2003.07.006
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
Be-7 radioactive nuclei with a half-life of 53.3 days result from spallation reactions of galactic cosmic rays (GCR) and solar energetic particles (SEP) with N and 0 nuclei in the Earth's atmosphere. We calculate the average global production of Be-7 in the atmosphere by GCR and SEP. The result indicates that an intense SEP event produces a large amount of Be-7 in the polar stratosphere and part of them could be transported to the surface at lower latitudes. The ground-level measurement of Be-7 in Japan exhibits the possibility of enhancement in the Be-7 radioactivity associated with the intense SEP event on July 14, 2000. In addition, the present experiment shows seasonal variations in the surface Be-7 concentration which peaks in spring and autumn. We discuss the possible air mass mixing between the stratosphere and troposphere to explain the measured seasonal variations. The surface concentration of Pb-210 nuclei indicates a similar trend to that of Be-7 and we suggest two possible explanations. (C) 2003 COSPAR. Published by Elsevier Ltd. All rights reserved.
引用
收藏
页码:2691 / 2696
页数:6
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