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SUMMARY:New Properties of Secondary Cosmic Rays observed by the Alpha Magn
 etic Spectrometer on the International Space Station
DTSTART;VALUE=DATE-TIME:20210902T154500Z
DTEND;VALUE=DATE-TIME:20210902T160000Z
DTSTAMP;VALUE=DATE-TIME:20260612T020214Z
UID:indico-contribution-15754@indico.ific.uv.es
DESCRIPTION:Speakers: Yao Chen (Shandong Institute of Advanced Technology 
 (SDIAT))\nPrecise knowledge of the rigidity dependence of secondary cosmic
  ray fluxes and of secondary-to-primary flux ratios is essential in the un
 derstanding of cosmic ray propagation. We report the properties of light s
 econdary cosmic-ray lithium\, beryllium \, boron nuclei\, and  heavy secon
 dary cosmic ray fluorine nuclei in the rigidity R range 2 GV to 3 TV obser
 ved  by the Alpha Magnetic Spectrometer experiment on the International Sp
 ace Station. The secondary-to-primary ratios fluorine-to-silicon and boron
 -to-oxygen (or boron-to-carbon) will be discussed\, showing that the propa
 gation properties of heavy cosmic rays\, from fluorine to silicon\, are di
 fferent from those of light cosmic rays\, from helium to oxygen.  The prop
 erties of cosmic-ray sodium and aluminum nuclei\, which are partly seconda
 ry and partly primary\, will also be presented.\n\nhttps://indico.ific.uv.
 es/event/6178/contributions/15754/
LOCATION:
URL:https://indico.ific.uv.es/event/6178/contributions/15754/
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