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SUMMARY:Time variations of the proton flux in Earth inner radiation belt d
 uring 23/24 solar cycles based on the PAMELA and the ARINA data.
DTSTART;VALUE=DATE-TIME:20161011T114500Z
DTEND;VALUE=DATE-TIME:20161011T120000Z
DTSTAMP;VALUE=DATE-TIME:20260712T093551Z
UID:indico-contribution-703@cern.ch
DESCRIPTION:Speakers: Vitaly Malakhov (NRNU MEPhI)\nThe PAMELA and the ARI
 NA experiments are carried out on the board of satellite RESURS-DK1 since 
 2006. The main goal of the PAMELA instrument is measurements of high energ
 y antiparticles in cosmic rays while the ARINA instrument is intended stud
 ying high energy charged particle bursts in the magnetosphere. Both of the
 se experiments have a possibility to study trapped particles in the inner 
 radiation belt. The complex of these two instruments covers proton energy 
 range from 30 MeV up to trapping limit (E= ∼2 GeV). Continuous measureme
 nts with the PAMELA and the ARINA spectrometers include falling and rising
  phases of 23/24 solar cycles and the maximum of 24th one. In this report 
 we present temporal profiles of proton flux in the inner zone of the radia
 tion belt (1.11 \n\nhttps://indico.particle.mephi.ru/event/4/contributions
 /703/
LOCATION:Milan Hotel Vivaldi-Boccerini
URL:https://indico.particle.mephi.ru/event/4/contributions/703/
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