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Cosmic radiation: The primary particles

 

作者: J.G. Wilson,  

 

期刊: Contemporary Physics  （Taylor Available online 1960）
卷期: Volume 1, issue 3  

页码: 204-219

 

ISSN:0010-7514

 

年代: 1960

 

DOI:10.1080/00107516008202612

 

出版商: Taylor & Francis Group

 

数据来源: Taylor

 

摘要:

Observations of primary cosmic-ray particles entering the upper atmosphere show that the solar system is situated in an isotropic flow of protons and of heavier nuclei, and that these particles carry energy which can vary from small values to values so great that we cannot at present define the upper limit of energy carried by a single particle.

 

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