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SUMMARY:The PAMELA Experiment: A decade of Cosmic Rays Physics in space
DTSTART;VALUE=DATE-TIME:20161011T060000Z
DTEND;VALUE=DATE-TIME:20161011T063000Z
DTSTAMP;VALUE=DATE-TIME:20260714T035554Z
UID:indico-contribution-527@cern.ch
DESCRIPTION:Speakers: Arkady Galper (NRNU MEPhI)\, Roberta Sparvoli (Unive
 rsity of Rome Tor Vergata)\nIt was the 15th of June of 2006 when the PAMEL
 A satellite-borne experiment  was launched from the Baikonur cosmodrome in
  Kazakstan. Since then\, PAMELA has been making high-precision measurement
 s of the charged component of the cosmic radiation opening a new era of pr
 ecision studies in cosmic  rays. \n\nThe measured antiparticle component o
 f the cosmic radiation shows features that can be interpreted in terms of 
 dark matter annihilation or pulsar contribution. The measurements of the e
 nergy spectra of protons\,  electrons\, helium and light nuclei and their 
 isotopes challenges our basic vision of the mechanisms of production\, acc
 eleration and propagation of cosmic rays in the galaxy. The study of the t
 ime dependence of the various components of the cosmic radiations clearly 
 shows solar modulation effects as well as charge sign dependence. \n\nPAME
 LA measurement of the energy spectra during solar energetic particle event
 s fills the existing energy gap between the highest energy particles measu
 red in space and the ground-based domain. Finally\, by sampling the partic
 le radiation in different regions of the magnetosphere\, PAMELA data provi
 de a detailed study of the Earth magnetosphere. \n\nIn this talk we will r
 eview the PAMELA experiment and its scientific results.\n\nhttps://indico.
 particle.mephi.ru/event/4/contributions/527/
LOCATION:Milan Hotel Rossini
URL:https://indico.particle.mephi.ru/event/4/contributions/527/
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