The spectrum features of UHECRs below and surrounding GZK

The energy spectrum of UHECRs is discussed on the basis of the Yakutsk array database analysis. In the region E=0.1 to 30 EeV the showers are detected under trigger-500, while at energies above 30 EeV the whole acceptance area for trigger-1000 is used in order to utilize all the data available in th...

Full description

Bibliographic Details
Main Authors: Egorova, V P, Glushkov, A V, Ivanov, A A, Knurenko, S P, Kolosov, V A, Krasilnikov, A D, Makarov, I T, Mikhailov, A A, Olzoev, V V, Pravdin, M I, Sabourov, A V, Sleptsov, I Ye, Struchkov, G G
Language:English
Published: 2004
Subjects:
Astrophysics and Astronomy
Yakutsk
Online Access:http://cds.cern.ch/record/790453
Description
Summary:The energy spectrum of UHECRs is discussed on the basis of the Yakutsk array database analysis. In the region E=0.1 to 30 EeV the showers are detected under trigger-500, while at energies above 30 EeV the whole acceptance area for trigger-1000 is used in order to utilize all the data available in the region of GZK cutoff.

Similar Items