The arrival of solar neutrons from a large zenith angle

Details The arrival of solar neutrons from a large zenith angle The arrival of solar neutrons from a large zenith angle

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....8.3056t&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

Scientific paper

Solar neutrons were detected by the Yangbajing solar neutron telescope located in Tibet(N¡£¢¥¤ , E¦£¢§¤ , 4300 m above sea level) in association with X3.3 solar flare on November 28th 1998. The detection of solar neutrons was possible using a capability of the telescope which can identify the incoming direction of neutrons. In this event, solar neutrons arrived at the top of the the atmosphere with a large zenith angle ¨©¡ ¤ . It has been shown by a Monte Carlo simulation in this paper that even solar neutrons with a large zenith angle can be detected owing to large angle scattering of neutrons by air nuclei. The energy spectrum of neutrons was obtained by assuming that solar neutrons were produced at the start time of BATSE hard X-rays.

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