摘要
建立了宇宙线广延大气簇的MonteCarlo模拟的模型，应用该模型模拟出一定能量的初级粒子在观测平面产生的次级电子数．与郑州阵列的实验数据相比较，模拟值与实验结果相符合．该模型可靠，可以用来进一步分析阵列的实验数据．
A Cosmic Ray Extensive Air Shower(EAS) simulation model is presented. The model is used to simulate the size of second particles which is produced through EAS by a primary particle with a defined energy. The simulation result accords with the experimental data. Therefore,the model is reliable and is used to further analyze the experimental data of array.
出处
《湘潭大学自然科学学报》
CAS
CSCD
1997年第3期43-45,共3页
Natural Science Journal of Xiangtan University
