Proceedings of the 34th International Cosmic Ray Conference — PoS(ICRC2015) 2016
DOI: 10.22323/1.236.0040
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Atmospheric- Weighted Temperature and its influence on Cosmic Ray muons

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Cited by 5 publications
(5 citation statements)
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“…[19] and [20] have shown there is a direct link between SSW and cosmic-ray Muon flux (CMF) via the atmospheric effective temperature. The effective temperature is the weighted-atmospheric temperature that acts as a proxy for the temperature of the real atmosphere when the various conditions from the point of observa- [21] and [22]. [23] strengthens our argument of the link between cosmic-ray Muon flux (CMF)-Sudden Stratospheric Warming (SSW) and the primary dry season (PDS) by pointing to a strong statistical correlation between cosmic-ray flux, large-scale precipitation and precipitation efficiency.…”
Section: Introductionsupporting
confidence: 55%
“…[19] and [20] have shown there is a direct link between SSW and cosmic-ray Muon flux (CMF) via the atmospheric effective temperature. The effective temperature is the weighted-atmospheric temperature that acts as a proxy for the temperature of the real atmosphere when the various conditions from the point of observa- [21] and [22]. [23] strengthens our argument of the link between cosmic-ray Muon flux (CMF)-Sudden Stratospheric Warming (SSW) and the primary dry season (PDS) by pointing to a strong statistical correlation between cosmic-ray flux, large-scale precipitation and precipitation efficiency.…”
Section: Introductionsupporting
confidence: 55%
“…The calculation procedures were conducted on the basis of (1). Multiple regression analyses were conducted between (i) raw muon rate and both pressure and temperature at the production level; (ii) raw muon rate and both pressure and level of pion production; (iii) raw muon rate and the three parameters; and (iv) pressure-corrected muon rate, using the method discussed in Maghrabi et al [23] and Maghrabi et al [12,13], which was correlated with both height and the temperature at the production level. 12 h data for each Advances in Astronomy 3 day during the specific month were used in the calculations.…”
Section: Resultsmentioning
confidence: 99%
“…According to theoretical and experimental investigations, atmospheric pressure is the most important factor affecting both cosmic ray muons and neutrons. It is a measure of the total atmospheric absorption above the detector (e.g., [8,[11][12][13]).…”
Section: Introductionmentioning
confidence: 99%
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“…On the other hand, the temperature corrections are slightly more complicated and several methods have been suggested to account for them [e.g., 1 and 3]. These include correlation of the muon rates with one of the following parameters: the atmospheric weighted temperature [4][5], the temperature at ground level [3 and 6], or with the temperature at the level of pion production [7][8][9][10][11].…”
mentioning
confidence: 99%