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Neutron Monitor Response Functions

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Abstract

The neutron monitor provides continuous ground-based recording of the hadronic component in atmospheric secondary radiation which is related to primary cosmic rays. Simpson (1948) discovered that the latitude variation of the secondary hadronic component was considerably larger than the muon component suggesting the response of a neutron monitor is more sensitive to lower energies in the primary spectrum. The different methods of determining the neutron monitor response function of primary cosmic rays are reviewed and discussed including early and recent results. The authors also provide results from a new calculation (Clem, 1999) including angle dependent yield functions for different neutron monitor types which are calculated using a simulation of cosmic ray air showers combined with a detection efficiency simulation for different secondary particle species. Results are shown for IGY and NM64 configurations using the standard 10BF3 detectors and the new 3He detectors to be used in the Spaceship Earth Project (Bieber et al., 1995). The method of calculation is described in detail and the results are compared with measurements and previous calculations. A summary of future goals is discussed.

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Authors and Affiliations

  1. Bartol Research Institute, University of Delaware, Newark, DE, 19716, U.S.A.

    John M. Clem

  2. IZMIRAN, Moscow, Russia

    Lev I. Dorman

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  1. John M. Clem
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  2. Lev I. Dorman
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Clem, J.M., Dorman, L.I. Neutron Monitor Response Functions. Space Science Reviews 93, 335–359 (2000). https://doi.org/10.1023/A:1026508915269

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