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Statistical Evaluation of Solar Neutrino Associated with the Coronal Mass Ejections for Solar Cycle 23 |
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PP: 69-74 |
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doi:10.18576/jrna/060110
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Author(s) |
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I. A. Hussain,
S. S. Salih,
W. H. A. Zaki,
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Abstract |
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Understanding solar neutrino will lead the researchers to understand the Sun. The present study is designed to track the associated solar neutrino with the solar cycle 23 and explore the statistical relations amongst the solar neutrino and solar activity through the correlation and regression.
The major solar energetic events like Coronal Mass Ejection (CME) and Sunspots for cycle (23) in the period of (1996 -2007) were analyzed via the “Large Angle Spectroscopic Coronagraph experiments (LASCO) on board SOHO satellite”. The neutrino events were taken from “the Soviet American Gallium experiment (SAGE)” for the same epoch of time. All the obtained results were statistically analyzed via the statistical program SPSS.
The graphical results revealed the existence of complicated relations between the neutrino candidate events and solar activities as a function of time. Whereas the statistical results indicate that no relation is found between the CME and the neutrino events for the same period of time, while an indicated linear relation was found between the number of CME and the neutrino events within the down phase of the solar activity.
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