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PoS(ICRC2017)062
35th International Cosmic Ray Conference — ICRC2017 obtain the correction coefficients of these variables. ... corrected (RHc) and temperature.
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PoS(ICRC2017)062
Copyright owned by the author(s) under the terms of the Creative CommonsAttribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0). http://pos.sissa.it/
The Effect of Some Meteorological Parameters on
the Cosmic Ray Muons detected by KACST detector Maghrabi A.H 1 National Centre for Applied Physics, King Abdulaziz City for Science and Technology,Address, P.O.Box 6086Riyadh 11442, Saudi Arabia.
Email: amaghrabi@kacst.edu.sa
Aldosary A.F
National Centre for Applied Physics, King Abdulaziz City for Science and Technology,Address, P.O.Box 6086Riyadh 11442, Saudi Arabia.
Email:aaldosary@kacst.edu.sa
To study the cosmic ray modulation properly, it is important to remove atmospheric effects. In this study cosmic ray data from the KACST detector in Riyadh, Saudi Arabia (Rc = 14.4 GV), for the period 20072009, were used to study the effect of some meteorological parameters on cosmic ray muons. The parameters of interest are the atmospheric pressure, temperature, and relative humidity. We have found that the atmospheric pressure and temperature are inversely correlated with the muon rate. On the other hand, the relative humidity is correlated with the number of cosmic ray muons.1A Maghrabi
35th International Cosmic Ray Conference
ICRC2017
10-20 July, 2017
Bexco, Busan, Korea
PoS(ICRC2017)062The Effect of Some Meteorological Parameters on the Cosmic Ray Muons detected by KACST detector
2 PoS(ICRC2017)062The Effect of Some Meteorological Par 3 1. particle and the cutoff rigidity of the considered 2. cosmic ray variation studies. The details of this detector and its c2009) have
The ୍ିMబ PoS(ICRC2017)062The Effect of Some Meteorological Par 4 157158
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930940950960Rate [Counts/
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where I0 x0 x 3.3.1 Pressure Effect
Figure (1) indicates the daily mean values of the muon rate plotted against the atmosFigure
2009. The straight line
Figure (2) is a scatter plot of the
Figure
PoS(ICRC2017)062The Effect of Some Meteorological Par 5 158159
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Pressure [mb]
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RR Pc P Figure (3) is a time series showing the variations of the monthly averages of the raw muon3.2 Temperature Effect
Figure (4) displays the relationship between the pressure corrected muon rates and the oC with a correlation coefficient of 0.64.Figure .
2009.PoS(ICRC2017)062The Effect of Some Meteorological Par 6 158
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T [ oC]Rate [Counts/
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RR Pc Tc T The oC (about 63 % of the temperature coefficient) with an r 2009.Figure 5.
3.3 Relative Humidity Effect
The effect of relative humidity on cosmic ray secondary particles has been investigated Figure 6. Scatter plot between the daily values of PoS(ICRC2017)062The Effect of Some Meteorological Par 7 159160
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RR Pc Tc RHc 158159
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Rate [Counts/
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Multiple regression analyses have been carried out between the muon rate and both the oC, respectively, and the correlation coefficiFigure (.
4. In this study, the effect of atmospheric pressure, temperature, and relative humidity on PoS(ICRC2017)062The Effect of Some Meteorological Par 8 type of secondary particles and their energies. An acceptable positive correlation was foundAcknowledgments
The authors would like to thank King Abdulaziz City for Science and Technology ReSvensmark H., Friis
Publishers, USA.
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