Study of Cosmic Ray fluxes in Low Earth Orbit (LEO) - AMS-02 Perugia
Study of Cosmic Ray fluxes in Low Earth Orbit (LEO) - AMS-02 Perugia
Study of Cosmic Ray fluxes in Low Earth Orbit (LEO) - AMS-02 Perugia
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ÀÈÌÊ ¾º ÇËÅÁ ÊË ÆÊ ÊÌÀ<br />
10<br />
1<br />
0.1<br />
He<br />
Differential flux (m 2 sr s MeV/nucleon) −1<br />
10 −2<br />
10 −3<br />
10 −4<br />
10 −5<br />
10 −6<br />
C<br />
Fe<br />
H<br />
10 −7<br />
10 −8<br />
10 −9<br />
10 10 2 10 3 10 4 10 5 10 6 10 7<br />
K<strong>in</strong>etic energy ( MeV / nucleon )<br />
ÙÖ ¾º½ Ê «ÖÒØÐ ÒÖÝ ×ÔØÖÙÑ ÓÖ «ÖÒØ ÒÙÐ ¿℄<br />
Relative abundance<br />
10 4<br />
10 3<br />
10 2<br />
10<br />
1<br />
10 -1<br />
10 -2<br />
10 -3<br />
10 -4<br />
10 -5<br />
10 -6<br />
10 -7<br />
Li<br />
Be<br />
B<br />
C<br />
N<br />
O<br />
Sc<br />
Ti<br />
V<br />
Fe<br />
10 5 0 5 10 15 20 25 30<br />
Charge number<br />
ÙÖ ¾º¾ ÓÑÔÖ×ÓÒ ØÛÒ Ê ´¬ÐÐ Öе Ò ËÓÐÖ ×Ý×ØÑ ÐÑÒØ ´ÓÔÒ ÖÐ×µ<br />
ÓÑÔÓ×ØÓÒ ¿℄º
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