Radionuclides, cosmogenic
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Radionuclides generated by interaction of cosmic radiation with the atomic nuclei of the atmosphere or with extraterrestrial matter coming down to earth as meteors or meteorites.
Nuclide |
Half-life |
Nuclide |
Half-life |
Nuclide |
Half-life |
H-3 |
12,323 a |
Si-32 |
172 a |
Mn-53 |
3,7·106 a |
Be-7 |
53,3 d |
P-32 |
14,3 d |
Mn-54 |
312 d |
Be-10 |
1,6·106 a |
S-35 |
87,5 d |
Fe-55 |
2,73 a |
C-14 |
5730 a |
S-38 |
2,8 h |
Fe-60 |
1,5·106 a |
Na-22 |
2,60 a |
Cl-36 |
3,0·105 a |
Co-60 |
5,27 a |
Na-24 |
15 h |
Ar-39 |
269 a |
Ni-59 |
7,5·104 a |
Al-26 |
7,2·105 a |
Ar-42 |
33 a |
Ni-63 |
100 a |
Mg-28 |
20,9 h |
Ca-41 |
1,0·105 a |
Kr-85 |
10,7 a |
Si-31 |
2,6 h |
Ti-44 |
60,4 a |
I-129 |
1,6 107 a |
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Cosmogenic radionuclides
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ENS conferences |
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TopSafe 2017
12-16 Feb. 2017
Vienna, Austria |
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PIME 2017
19 - 22 March 2017, Middelburg Netherlands |
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RRFM 2017
14 - 18 May 2017 in Rotterdam, Netherlands |
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ETRAP 2017
30 May - 2 June 2017, Valencia, Spain |
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