Место издания:Tata Institute of Fundamental Research Bombay, India
Первая страница:157
Последняя страница:160
Аннотация:The gamma-radiation detected by the balloon-borne instruments can be divided into three components Iγ = Iγcos + Iγatm + Iγloc where Iγcos is the primary radiation, Iγatm is the secondary radiation in the atmosphere due to cosmic rays, and Iγloc is the secondary radiation in the material of the balloon and gamma-telescope caused by cosmic rays.