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Autor:
E. Riihonen, A. M. Elo, H. Arvela, Eino Valtonen, J. J. Torsti, H. Kananen, E. Vainikka, J. Peltonen, T. Eronen
Publikováno v:
Advances in Space Research. 9:229-232
Neutron monitor measurements using 10-second recording intervals were started at Oulu in September 1987. A special analysis method based on the power spectra was adopted to compensate for the relative low statistics associated with short recording in
Publikováno v:
Journal of Physics G: Nuclear Physics. 10:695-703
The coincidences of cosmic-ray particles in sea-level detectors were investigated theoretically. The object of the work was to clarify the role of accompanied particles in the measurement of the spectrum of hadrons. The calculations were based on a M
Publikováno v:
Journal of Physics G: Nuclear Physics. 10:1465-1471
The energy spectrum of cosmic-ray hadrons between 10 GeV and 10 TeV at sea level was calculated by using a Monte-Carlo method. The results show a strong steepening of the hadron spectrum at about 200 GeV. The change in the spectral slope is interpret
Publikováno v:
Advances in Space Research. 4:101-104
The energy spectra of cosmic-ray neutrons, protons, and pions were determined at sea level in the range 0.1 – 1000 GeV. The results are based on the measurements of the neutron-multiplicity distributions produced by cosmic hadrons in the Turku spec
Autor:
J. Peltonen, J. J. Torsti, M. Lumme, E. Riihonen, E. Vainikka, Eino Valtonen, M. Nieminen, H. Arvela
Publikováno v:
Il Nuovo Cimento C. 10:102-108
The time structure of the ground-level event on February 16, 1984 was studied by using 30 s data of the Turku double neutron monitor. The onset time of the event was found to be (09:06:00±1) min U.T. The time between the injection of protons from th
Publikováno v:
Journal of Physics G: Nuclear Physics. 11:421-437
Energy spectra of neutrons, protons and pions were measured at sea level using a cosmic-ray hadron spectrometer consisting of a double neutron monitor and scintillation counters. All the hadron spectra were determined simultaneously. The analysis of
Publikováno v:
Journal of Physics G: Nuclear Physics. 10:683-694
A Monte-Carlo model has been developed for the calculation of the intensities of hadrons and muons emerging from particle cascades initiated by primary cosmic rays in the atmosphere. Special attenuation is paid to the energy spectra of the particles