Production of cosmogenic Cl-36 on atmospheric argon

被引：25
|
作者：
Huggle, D
Blinov, A
StanSion, C
Korschinek, G
Scheffel, C
Massonet, S
Zerle, L
Beer, J
Parrat, Y
Gaeggeler, H
Hajdas, W
Nolte, E
机构：
[1] TECH UNIV MUNICH,FAC PHYS,D-85747 GARCHING,GERMANY
[2] TECH UNIV ST PETERSBURG,DEPT COSM RES,ST PETERSBURG 195251,RUSSIA
[3] INST NUCL PHYS & ENGN,BUCHAREST,ROMANIA
[4] SWISS FED INST ENVIRONM SCI & TECHNOL EAWAG,CH-8600 DUBENDORF,SWITZERLAND
[5] PAUL SCHERRER INST WURENLINGEN & VILLIGEN,CH-5232 VILLIGEN PSI,SWITZERLAND
来源：
PLANETARY AND SPACE SCIENCE | 1996年 / 44卷 / 02期
关键词：
D O I：
10.1016/0032-0633(95)00085-2
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Spallation cross sections for the reaction Ar-40(p, 2p3n)Cl-36 are measured in the energy range 47-1000 MeV. The results are used to calculate the production of cosmogenic Cl-36 on atmospheric argon by solar protons and by galactic cosmic rays. The dependence of the fall-out rate of atmospheric cosmogenic Cl-36 on geomagnetic latitude and solar activity is calculated.
引用
收藏
页码：147 / 151
页数：5
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