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Verifying the Relationship between Solar Neutrinos and Solar Wind for Solar Cycle 23 |
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PP: 65-72 |
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doi:10.18576/jrna/040109
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Author(s) |
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Imad A. H. Al-Hayali,
Wafaa H. A. Zaki,
Shadan S. Salih,
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Abstract |
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| The major solar energetic events of solar cycle (23) for the years (1996 -2007) are analysed by using the Energetic and Relativistic Nucleus and Electrons (ERNE) detectors, the Large Angle Spectroscopic Coronagraph experiments (LASCO) on board SOHO and the Geostationary Operational Environmental Satellite system (GOES) that is operated by the U.S. National Oceanic and Atmospheric Administration (NOAA). The number of Coronal Mass Ejection (CME) which satisfies the required conditions by testing their intensity – time profile provided by ERNE detector is 212 events, as well as the 100 solar energetic particle (SEP) events that are detected by GOES and 23176 flares has been held in this study. The captured flare by GOES are classified according to their strength include only 1339 flares of class M and X. 2313 neutrino events of energy (Eѵ=233 keV to 15 MeV) are taken from the Soviet American Gallium Experiment (SAGE) for the same period of time of the investigated solar wind. All the extracted results are statistically analysed using the statistical program SPSS (version 20), these results indicate to a linear relationship between CME and the neutrino events for the down phase of the solar cycle 23. |
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