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SUMMARY:Mass composition of primary cosmic rays by the latest TAIGA-HiSCOR
 E data
DTSTART;VALUE=DATE-TIME:20241025T135700Z
DTEND;VALUE=DATE-TIME:20241025T140900Z
DTSTAMP;VALUE=DATE-TIME:20260314T052853Z
UID:indico-contribution-4095@cern.ch
DESCRIPTION:Speakers: Mark Ternovoy (API ISU)\nThis report presents the la
 test findings on the mass composition of primary cosmic rays based on data
  from the TAIGA-HiSCORE array\, which operated in its full configuration w
 ith four clusters. The TAIGA-HiSCORE stations were reoriented towards the 
 zenith\, and new calibration procedures were introduced to improve the det
 ector array's performance. The study of extensive air showers (EAS) in the
  energy range of 1 to 100 PeV\, using the depth of the shower maximum\, sh
 ows good agreement with results from the LHAASO experiment\, particularly 
 near the "knee" of the cosmic ray energy spectrum. An increase in the mean
  logarithmic mass in the 3-30 PeV energy range was also observed and exami
 ned.\n\nhttps://indico.particle.mephi.ru/event/436/contributions/4095/
LOCATION: Moskvorechye 2
URL:https://indico.particle.mephi.ru/event/436/contributions/4095/
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