پديد آورندگان :
دهقاني، محمد نويسنده دانشگاه صنعتي شريف,; Dehghani, M , انواري، عباس نويسنده دانشگاه صنعتي شريف,دانشكده فيزيك; Anvari, A , بهمن آبادي، محمود نويسنده دانشگاه صنعتي شريف,; Bahmanabadi, M , هدايتي، هادي نويسنده دانشگاه صنعتي شريف,; Hedayati, H , ميركاظمي، مهدي نويسنده دانشگاه صنعتي شريف,; Mirkazemi, M , خاكيان، مهدي نويسنده دانشگاه صنعتي شريف,; , , صميمي، جلال نويسنده دانشگاه صنعتي شريف,دانشكده فيزيك; ,
چكيده لاتين :
A cosmic ray tracking telescope has been made for the measurement of cosmic rays from different directions, especially those received from the sun direction. Our observations by the telescope shows a noticeable deficiency in the detected number of cosmic rays entering the telescope when its axis was pointing to the sun compared to that entering the telescope with no sun in its field of view. The statistical significance of this deficit with the Li and Ma method stands near 2 cr for all of our observations.
