The muon flux of cosmic rays at sea level

A. K. De, P. Ghosh, S. Mitra, P. Bhattacharya, A. Das
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引用次数: 14

Abstract

The sea-level absolute vertical integral cosmic ray muon intensities for three momenta near 1 GeV/c at 12 degrees N were measured with a range spectrometer. The results obtained from this measurement are used to derive the intensities at a latitude of 50 degrees N by applying the latitude correction suggested by Olbert (1954). The integral muon intensities are found to be on the average 3.5% lower and 21.6% higher than the values obtained by Allkofer et al. and Rossi respectively. The differential intensities derived from the integral ones are 20% higher than those calculated from Olbert at the same latitude. The results of the other recent measurements on the differential muon intensities in the low energy region in relation to a form spectrum are also discussed.
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海平面上宇宙射线的介子通量
用距离谱仪测量了12°N条件下海平面接近1 GeV/c的三个动量的绝对垂直积分宇宙射线μ子强度。采用奥尔伯特(Olbert, 1954)提出的纬度校正法,利用这一测量结果推导出北纬50度处的强度。发现积分μ子强度比Allkofer等和Rossi得到的值分别平均低3.5%和高21.6%。在同一纬度,由积分得到的微分强度比由奥尔伯特计算得到的高20%。本文还讨论了最近对低能区的微分μ子强度与形式谱的关系的测量结果。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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