Solar cycle variation in energetic parti
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Y. Hakura
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Article
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1974
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Springer
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English
โ 245 KB
Long-term variation in energetic particle emissivity of the sun was examined by the use of PCA, solar proton flux, and geomagnetic data from 1941 to 1973. A solar cycle may be divided into three periods in terms of the Sun's particle emissivity. The first period with a peak of emissivity coinciding