Set of spectrographic instruments for a global network of cosmic-ray stations

Computer Science

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Cosmic Ray Showers, Instrument Errors, Radiation Measurement, Secondary Cosmic Rays, Spectrometers, Atmospheric Effects, Neutron Counters, Particle Telescopes

Scientific paper

The possibility is considered of separating observed variations in secondary-cosmic-ray intensity into components of thermal and interplanetary origin for a set of instruments that includes neutron monitors with and without lead as well as a vertical telescope for detecting the penetrating and soft cosmic-ray components at the same observational level. It is noted that such a set of instruments can best be implemented in a global network of cosmic-ray stations. A system of four spectrographic equations containing four unknowns is analyzed and solved, and a much simpler solution is obtained by reducing the number of unknowns to three. Errors in determining the three unknowns as functions of the primary-variation spectrum and the amplitude of the observed variations are evaluated for a neutron monitor without lead.

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