Author/Authors :
Muraki، نويسنده , , Y. and Tsuchiya، نويسنده , , H. and Fujiki، نويسنده , , K. and Masuda، نويسنده , , S. and Matsubara، نويسنده , , Y. and Menjyo، نويسنده , , H. and Sako، نويسنده , , T. and Watanabe، نويسنده , , K. and Ohnishi، نويسنده , , M. and Shiomi، نويسنده , , A. and Takita، نويسنده , , M. and Yuda، نويسنده , , T. and Katayose، نويسنده , , Y. and Hotta، نويسنده , , N. and Ozawa، نويسنده , , S. and Sakurai، نويسنده , , T. and Tan، نويسنده , , Y.H. and Zhang، نويسنده , , J.L.، نويسنده ,
Abstract :
A new solar neutron telescope has been constructed at Yangbajing, Tibet (600 g/cm2) and has been successfully operated for 8 years. During this time several interesting events were observed in coincidence with large solar flares. In this paper the authors discuss a directional count rate enhancement 1998 November 28 as to whether it is related to solar phenomena or not. We use this event to evaluate the sensitivity of the solar neutron telescope and discuss the detection limit for solar neutrons and high energy solar protons of this detector.
Keywords :
Solar neutron telescope , Particle acceleration , Highest energy solar particles , Solar neutrons
