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SUMMARY:Astropalticle Physics at Chacaltaya 5230 m a.s.l.
DTSTART;VALUE=DATE-TIME:20151008T080000Z
DTEND;VALUE=DATE-TIME:20151008T083000Z
DTSTAMP;VALUE=DATE-TIME:20261014T232519Z
UID:indico-contribution-34-468@cern.ch
DESCRIPTION:Speakers: Oscar Saavedra San Martin (Torino University)\nAfter
  a brief description of the main scientific findings at Chacaltaya\, we pr
 esented  the possibility of a network to search for Extensive Air Showers 
 originated from primary cosmic rays at energies greater than 10^^15 eV. Su
 ch EAS could be measured in the existing high altitude laboratories deploy
 ed in the region of Latin America.\nThe Chacaltaya EAS array\, located at 
 5230 m a.s.l. could be take as\nthe centre of the network from where the d
 istances of the others could be at\nEl Alto (4000 m a.s.l.) and Cota Cota 
 (3600 m a.s.l.) in Bolivia\, at the\ndistances of 15 and 25 Km from Chacal
 taya respectively while the\nlaboratory of Putre (3600 m a.s.l.) in Chile 
 and Huancayo (3500 m\na.s.l.) in Peru\, are at the distances about 250 and
  700 km respectively from\nChacaltaya.\nSearching for simultaneous and par
 allel EAS events at multiple observatories is very important to look for n
 on random cosmic rays.\nOne of main aim of this network could be to search
  for simultaneous and\nparallel EAS events at multiple EAS observatories f
 or example due to Gerasimova-Zatsepin effect at high altitude laboratories
 . Besides this\, study other astrophysical phenomena\, like high energy ga
 mma rays from GRBs could be possible with the same array.\n\nhttps://indic
 o.particle.mephi.ru/event/2/contributions/468/
LOCATION:Milan Hotel 4* Verdi&Bellini
URL:https://indico.particle.mephi.ru/event/2/contributions/468/
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BEGIN:VEVENT
SUMMARY:Cosmic Ray Physics with TeV Muons in Large Volume Detectors
DTSTART;VALUE=DATE-TIME:20151008T073000Z
DTEND;VALUE=DATE-TIME:20151008T080000Z
DTSTAMP;VALUE=DATE-TIME:20261014T232519Z
UID:indico-contribution-34-324@cern.ch
DESCRIPTION:Speakers: Patrick Berghaus (DESY Zeuthen)\nLarge volume detect
 ors designed for the detection of astrophysical neutrinos such as IceCube 
 register cosmic ray-induced atmospheric muon bundles at a rate of several 
 thousand events per second. Due to the large amount of surrounding materia
 l\, the effective energy threshold for muons reaching the detector lies at
  approximately one TeV. By careful evaluation of event profiles it is poss
 ible to address cosmic ray and particle physics issues in an unprecedented
  energy range. First results from the analysis of one year of IceCube data
  will be presented and their implications discussed.\n\nhttps://indico.par
 ticle.mephi.ru/event/2/contributions/324/
LOCATION:Milan Hotel 4* Verdi&Bellini
URL:https://indico.particle.mephi.ru/event/2/contributions/324/
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BEGIN:VEVENT
SUMMARY:Taiga project
DTSTART;VALUE=DATE-TIME:20151008T083000Z
DTEND;VALUE=DATE-TIME:20151008T090000Z
DTSTAMP;VALUE=DATE-TIME:20261014T232519Z
UID:indico-contribution-34-288@cern.ch
DESCRIPTION:Speakers: Igor Yashin (National Research Nuclear University ME
 PHI)\nThe TAIGA project is aimed at solving the fundamental problems of ga
 mma-ray astronomy and physics of ultrahigh energy cosmic rays with the hel
 p of the complex of detectors\, located in the Tunka valley (Siberia\, Rus
 sia). TAIGA includes a wide-angle large area Tunka-HiSCORE array\, designe
 d to detect gamma-rays of ultrahigh energies in the range 20 - 1000 TeV an
 d charged cosmic rays with energies of 100 TeV - 100 PeV\, large area muon
  detector to improve the rejection of background EAS protons and nuclei an
 d a network of imaging atmospheric Cherenkov telescopes for gamma radiatio
 n detection. We discuss the goals and objectives of the complex features o
 f each detector and the results obtained in the first stage of the HiSCORE
  installation.\n\nhttps://indico.particle.mephi.ru/event/2/contributions/2
 88/
LOCATION:Milan Hotel 4* Verdi&Bellini
URL:https://indico.particle.mephi.ru/event/2/contributions/288/
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BEGIN:VEVENT
SUMMARY:Results from the KASCADE-Grande experiment
DTSTART;VALUE=DATE-TIME:20151008T070000Z
DTEND;VALUE=DATE-TIME:20151008T073000Z
DTSTAMP;VALUE=DATE-TIME:20261014T232519Z
UID:indico-contribution-34-249@cern.ch
DESCRIPTION:Speakers: Andrea Chiavassa (Università agli studi di Torino)\
 nIn this talk I will review and disucss the results obtained with the KASC
 ADE-Grande in the study of the spectrum\, chemical composition and anistro
 py of primary cosmic rays in the 10^16-10^18 eV energy range\n\nhttps://in
 dico.particle.mephi.ru/event/2/contributions/249/
LOCATION:Milan Hotel 4* Verdi&Bellini
URL:https://indico.particle.mephi.ru/event/2/contributions/249/
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