Intensity of the neutron component of cosmic rays and air humidity

IF 0.9 Q4 GEOCHEMISTRY & GEOPHYSICS
Valery Yanchukovsky, Marina Kalyuzhnaya, Rashit Hisamov
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引用次数: 0

Abstract

Neutron monitor data is currently corrected only for the barometric effect. We cannot, however, exclude that changes in air humidity affect the intensity of the cosmic-ray neutron component recorded by neutron monitors. In this regard, we have carried out continuous measurements of air humidity and temperature when observing variations in the cosmic ray intensity with a neutron monitor in Novosibirsk. Analysis of the results of observations of meteorological parameters and cosmic ray intensity in Novosibirsk, as well as data from the global network of neutron monitors, made it possible to identify neutron component intensity variations caused by changes in air humidity. The estimated humidity effect indicates the need to regularly take it into account in the neutron monitor data. To do this, along with atmospheric pressure, regular measurements of humidity and air temperature should be performed.
宇宙射线中子成分的强度与空气湿度
中子监测仪的数据目前只根据气压效应进行校正。但是,我们不能排除空气湿度的变化会影响中子监测仪记录的宇宙射线中子成分的强度。为此,我们在新西伯利亚用中子监测仪观测宇宙射线强度变化时,对空气湿度和温度进行了连续测量。对新西伯利亚气象参数和宇宙射线强度的观测结果以及中子监测仪全球网络的数据进行分析,可以确定空气湿度变化引起的中子成分强度变化。对湿度影响的估计表明,有必要在中子监测器数据中定期考虑湿度影响。为此,除大气压力外,还应定期测量湿度和空气温度。
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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来源期刊
Solar-Terrestrial Physics
Solar-Terrestrial Physics GEOCHEMISTRY & GEOPHYSICS-
CiteScore
1.50
自引率
9.10%
发文量
38
审稿时长
12 weeks
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