Scaler mode of the Auger Observatory and Sunspots

Recent data from the Auger Observatory on low energy secondary cosmic ray particles are analyzed to study temporal correlations together with data on the daily sunspot numbers and neutron monitor data. Standard spectral analysis demonstrates that the available data shows 1/f^{\beta} fluctuations wit...

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Published inarXiv.org
Main Authors García Canal, Carlos A, Hojvat, Carlos, Tarutina, Tatiana
Format Paper Journal Article
LanguageEnglish
Published Ithaca Cornell University Library, arXiv.org 06.09.2012
Subjects
Augers
Correlation analysis
Cosmic rays
Data analysis
Frequency ranges
Observatories
Physics - Solar and Stellar Astrophysics
Secondary cosmic rays
Sunspots
Variations
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Abstract Recent data from the Auger Observatory on low energy secondary cosmic ray particles are analyzed to study temporal correlations together with data on the daily sunspot numbers and neutron monitor data. Standard spectral analysis demonstrates that the available data shows 1/f^{\beta} fluctuations with {\beta} approximately 1 in the low frequency range. All data behave like Brownian fluctuations in the high frequency range. The existence of long-range correlations in the data was confirmed by detrended fluctuation analysis. The real data confirmed the correlation between the scaling exponent of the detrended analysis and the exponent of the spectral analysis.
AbstractList Recent data from the Auger Observatory on low energy secondary cosmic ray particles are analyzed to study temporal correlations together with data on the daily sunspot numbers and neutron monitor data. Standard spectral analysis demonstrates that the available data shows 1/f^{\beta} fluctuations with {\beta} approximately 1 in the low frequency range. All data behave like Brownian fluctuations in the high frequency range. The existence of long-range correlations in the data was confirmed by detrended fluctuation analysis. The real data confirmed the correlation between the scaling exponent of the detrended analysis and the exponent of the spectral analysis.
Recent data from the Auger Observatory on low energy secondary cosmic ray particles are analyzed to study temporal correlations together with data on the daily sunspot numbers and neutron monitor data. Standard spectral analysis demonstrates that the available data shows 1/f^{\beta} fluctuations with {\beta} approximately 1 in the low frequency range. All data behave like Brownian fluctuations in the high frequency range. The existence of long-range correlations in the data was confirmed by detrended fluctuation analysis. The real data confirmed the correlation between the scaling exponent of the detrended analysis and the exponent of the spectral analysis.
Author Tarutina, Tatiana
Hojvat, Carlos
García Canal, Carlos A
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BackLink https://doi.org/10.1088/0067-0049/202/2/16$$DView published paper (Access to full text may be restricted)
https://doi.org/10.48550/arXiv.1209.1367$$DView paper in arXiv
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Correlation analysis
Cosmic rays
Data analysis
Frequency ranges
Observatories
Physics - Solar and Stellar Astrophysics
Secondary cosmic rays
Sunspots
Variations
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Title Scaler mode of the Auger Observatory and Sunspots
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