作者: R. Michel , P. Dragovitsch , P. Cloth , G. Dagge , D. Filges
DOI: 10.1111/J.1945-5100.1991.TB01043.X
关键词:
摘要: A purely physical model is presented describing the depth‐ and size‐dependence of the production of cosmogenic nuclides in meteoroids with radii up to 85 cm and in planetary …