Study of the Effects of Atmospheric Pressure in the Time Series of Muon Detector Using the Method of Spectral Analysis


This paper presented a study of the effects of atmospheric pressure in the time series of muon detector using the method of spectral analysis of iterative regression. In which it observed that the periods of 4.8, 5.7, 7.0, 8.7, 10.7, 14.1, 16.2, 21.0, 31.2 and 356.7 days present in the amplitude spectrum of atmospheric pressure are also present in the amplitude spectra of muons data. Also it observed that the standardization of muons data to eliminate the effects of atmospheric pressure is efficient for periods under 7 days.

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Rigozo, N. (2014) Study of the Effects of Atmospheric Pressure in the Time Series of Muon Detector Using the Method of Spectral Analysis. International Journal of Geosciences, 5, 239-246. doi: 10.4236/ijg.2014.53025.

Conflicts of Interest

The authors declare no conflicts of interest.


[1] Gosling, J.T., Bame, S.J., McComas, D.J. and Phillips, J.L. (1990) Coronal Mass Ejections and Large Geomagnetic Storms. Geophysical Research Letters, 17, 901-904.
[2] Gosling, J.T., McComas, D.J., Phillips, J.L. andBame, S.J. (1991) Geomagnetic Activity Associated with Earth Passage of Interplanetary Shock Disturbances and Coronal Mass Ejections. Journal of Geophysical Research, 96, 7831-7838.
[3] Cane, H.V. (2000) Coronalmass Ejections and Forbush Decreases. Space Science Reviews, 93, 55-77.
[4] Pomerantz, M.A. and Duggal, S.P. (1971) The Cosmic Ray Solar Diurnal Anisotropy. Space Science Reviews, 12, 75-130.
[5] Simpson, J.A., Fonger, W. and Treimant, S.B. (1953) Cosmic Radiation Intensity-Time Variations and Their Origin. I. Neutron Intensity Variation Method and Meteorological Factors. Physical Review, 90, 934-950.
[6] Dorman, L.I.I. and Yanke, V.G. (1975) Development of the Theory of Meteorological Effects in Cosmic Rays. Proceedings from the 14th International Cosmic Ray Conference, Munchen, 15-29 August 1975, 1385.
[7] Kurguzova, A.I. and Charakhchian, T.N. (1979) Temperature Effect of the Muon Component of Cosmic Rays in the Atmosphere. Geomagnetism and Agronomy, 18, 403-407.
[8] Bercovitch, M. (1967) Atmospheric Effects on Cosmic Ray Monitors. Proceedings of the 10th International Cosmic Ray Conference, Calgary, 19-30 June 1967, 269.
[9] Wolberg, J.R. (1967) Prediction Analysis. D. Van Nostrand, Princeton.
[10] Rigozo, N.R., Echer, E., Nordemann, D.J.R., Vieira, L.E.A. and Faria, H.H. (2005) Comparative Study between Four Classical Spectral Analysis Methods. Applied Mathematics and Computation, 168, 411-430.
[11] Dragic, A., Banjanac, R., Udovicic, V., Jokovic, D., Puzovic, J. and Anicin, I. (2005) Variations of CR-Muon Intensity in the Declining Phase of the 23rd Solar Cycle in Ground and Shallow Underground Data. Proceedings of the 29th International Cosmic Ray Conference, Pune, 3-10 August 2005, 101-104.
[12] Kirkby, J., Mangini, A. and Muller, R.A. (2004) The Glacial Cycles and Cosmic Rays. European Organization for Nuclear Research, CERN-PH-EP/2004-027, 1-16.
[13] Da Silva, M.R., Gonzalez, W.D., Echer, E., Dal Lago, A., Vieira, L.E.A., Guarnieri, F.L., Lucas, A., Schuch, N.J. and Munakata, K. (2007) Multitaper Spectral Analysis of Cosmic Rays Sao Martinho da Serra’s Muon Telescope and Newark’s Neutron Monitor Data. Revista Brasileira de Geofísica, 25, 163-167.
[14] Dorman, L. (2004) Cosmic Rays in the Earth’s Atmosphere and Underground. Kluwer Academic Publisher, Dordrecht.
[15] Vieira, L.R., Dal Lago, A., Rigozo, N.R., Da Silva, M.R., Braga, C.R., Petry, A. and Schuch, N.J. (2012) Near 13.5-Day Periodicity in Muon Detector Data during Late 2001 and Early 2002. Advances in Space Research, 49, 1615-1622.

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