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SUMMARY:Orbital High Energy  Cosmic Rays Observatory - stages of developme
 nt
DTSTART;VALUE=DATE-TIME:20210610T134000Z
DTEND;VALUE=DATE-TIME:20210610T135500Z
DTSTAMP;VALUE=DATE-TIME:20260314T021747Z
UID:indico-contribution-155@indico.nevod.mephi.ru
DESCRIPTION:Speakers: Dmitry Podorozhny (M.V.Lomonosov Moscow State Univer
 sity\, Skobeltsyn Institute of Nuclear PhysicsM.V.Lomonosov Moscow State U
 niversity\, Skobeltsyn Institute of Nuclear Physics)\nCurrent status and p
 reliminary design of the High-Energy Ray Observatory (HERO) are presented.
  The HERO is planned to be launched onboard a heavy satellite. This experi
 ment is based on the application of a deep and wide aperture ionization ca
 lorimeter with mass from 10 to 70 tonns. The effective geometrical factor 
 of the observatory varies from 12 to 62 m2sr respectively\, depending on t
 he mass of the calorimeter. Under the 5-7 years exposure\, this mission wi
 ll allow to measure the cosmic ray composition and energy spectra of nucle
 i around the knee and up to 10^17 eV with high precision and to solve the 
 most actual problems of high energy astrophysics. Stages of development ar
 e presented\; details of technical realization are discussed.\n\nhttps://i
 ndico.nevod.mephi.ru/event/6/contributions/155/
LOCATION:Online Zoom
URL:https://indico.nevod.mephi.ru/event/6/contributions/155/
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