ueb5e - Astroparticle Physics, 2011 Problem 5 Problem 5:...

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Unformatted text preview: Astroparticle Physics, 2011 Problem 5 Problem 5: Neutron monitors The flux of cosmic rays can be measured with neutron monitors because secondary neutrons produced in the atmosphere are a good measure of the incident cosmic-ray flux in the GeV band. How would you construct a gound-based detector for neutrons? ...
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This note was uploaded on 02/29/2012 for the course PHYS 227 taught by Professor Rabe during the Fall '08 term at Rutgers.

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