Current Status of the High-Energy Ray Observatory


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Resumo

The aims and scientific tasks of the space High-Energy Ray Observatory experiment are determined. The design of the scientific equipment is described. It is characterized by an unprecedently high geometric factor (~20 m2 sr) and fairly high accuracy of measurement. The performance of the equipment allows precise study of cosmic rays in a wide range of energies, including the completely unstudied region of 1015–1016 eV. The current status of the space experiment is determined.

Sobre autores

D. Podorozhny

Skobeltsyn Institute of Nuclear Physics, Moscow State University

Autor responsável pela correspondência
Email: dmp@eas.sinp.msu.ru
Rússia, Moscow, 119991

D. Karmanov

Skobeltsyn Institute of Nuclear Physics, Moscow State University

Email: dmp@eas.sinp.msu.ru
Rússia, Moscow, 119991

A. Panov

Skobeltsyn Institute of Nuclear Physics, Moscow State University

Email: dmp@eas.sinp.msu.ru
Rússia, Moscow, 119991

L. Tkachev

Joint Institute for Nuclear Research

Email: dmp@eas.sinp.msu.ru
Rússia, Dubna, 141980

A. Turundaevskiy

Skobeltsyn Institute of Nuclear Physics, Moscow State University

Email: dmp@eas.sinp.msu.ru
Rússia, Moscow, 119991

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