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SUMMARY:Cosmic Ray Nuclei: Results from AMS-02
DTSTART;VALUE=DATE-TIME:20210610T125000Z
DTEND;VALUE=DATE-TIME:20210610T131500Z
DTSTAMP;VALUE=DATE-TIME:20261011T213930Z
UID:indico-contribution-152@indico.nevod.mephi.ru
DESCRIPTION:Speakers: Federico Donnini (INFN Sez. Perugia)\nAMS is a multi
 -purpose high energy particle detector designed to perform high precision 
 direct cosmic ray measurements onboard of the International Space Station.
  AMS can measure and identify cosmic ray nuclei with unprecedented precisi
 on and\, thanks to its large acceptance and the long exposure time\, it is
  able to provide precision studies of cosmic ray nuclei in the GV-TV regio
 n. In 10 years of operation\, AMS has collected more than 170 billion cosm
 ic rays triggers. In this contribution\, the precision measurement of prim
 ary and secondary cosmic rays fluxes from protons to Silicon (Z=14)\, and 
 the primary Iron flux (Z=26)\, in the rigidity range from 2 GV up to 3 TV 
 is presented. These measurements are based on the data collected by AMS fr
 om May 2011 to May 2018\n\nhttps://indico.nevod.mephi.ru/event/6/contribut
 ions/152/
LOCATION:Online Zoom
URL:https://indico.nevod.mephi.ru/event/6/contributions/152/
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