Specific yield functions of neutron supermonitors for solar neutrons

Details Specific yield functions of neutron supermonitors for solar neutrons Specific yield functions of neutron supermonitors for solar neutrons

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ge%26ae..28..832e&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 28, Sept.-Oct. 1988, p. 832-835. In Russian.

Physics

3

Elementary Particle Interactions, Energy Spectra, Particle Acceleration, Solar Neutrons, Solar Terrestrial Interactions, Hadrons, Monte Carlo Method, Neutron Counters, Semiempirical Equations

Scientific paper

The Monte Carlo method is used to calculate the specific yield functions
of a neutron supermonitor for solar neutrons. In the calculation, use
was made of semiempirical analytical approximations of double
differential distributions of secondary particles in hadron-nuclear
collisions.

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