This paper deals with diffuse cosmic gamma rays in " Single Leaky Box(LB) Model " and in " Double Leaky Box(LB) Model " by means of several typical galactic cosmic ray distribution laws and hydrogen distribution laws. 本文利用几种典型的银河系宇宙线分布律和星际氢分布律计算单漏模式和双漏模式中的弥散宇宙γ射线谱。
In the leaky box model, we give comparisons of calcula - ted ratios of secondary and primary nuclei and primary energy spectra with observed results. 并在漏箱模型中,给出了计算的次级与原初之比和原初能谱与观测结果的比较。