12-20 July 2017
BEXCO
Asia/Seoul timezone
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Contribution

BEXCO - Room F(201/202/203/204)

[SH136] Evaluation of long-term stability of the global network of neutron monitors after sixty years of its operation

Speakers

  • L. I. DORMAN

Primary authors

  • L. I. DORMAN (Institute of Terrestrial Magnetism, Ionosphere and Radiowave Propagation RAN of N.V. Pushkov (IZMIRAN), Russia)

Co-authors

  • A.V. BELOV (Institute of Terrestrial Magnetism, Ionosphere and Radiowave Propagation RAN of N.V. Pushkov (IZMIRAN), Russia)
  • R.T. GUSHCHINA (Institute of Terrestrial Magnetism, Ionosphere and Radiowave Propagation RAN of N.V. Pushkov (IZMIRAN), Russia)
  • Eroshenko E.A. EROSHENKO (Institute of Terrestrial Magnetism, Ionosphere and Radiowave Propagation RAN of N.V. Pushkov (IZMIRAN), Russia)
  • M.S. PREOBRAZHENSKY (Institute of Terrestrial Magnetism, Ionosphere and Radiowave Propagation RAN of N.V. Pushkov (IZMIRAN), Russia)
  • V.G. YANKE (Institute of Terrestrial Magnetism, Ionosphere and Radiowave Propagation RAN of N.V. Pushkov (IZMIRAN), Russia)

Description

Results of continuous monitoring of cosmic rays by the neutron monitors network are the experimental basement for a large number of papers studying cosmic rays variations. The problem of long-term stability of neutron monitor detectors is extremely important. In this work two independent methods for estimate of the long-term stability of neutron monitor are used. Quantitative estimates are obtained for detectors operating more than one solar cycle.