Possible periodicities of high-speed solar plasma |
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Authors: | J. Xanthakis C. Poulakos B. Petropoulos |
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Affiliation: | 1. Research Center for Astronomy and Applied Mathematics, Academy of Athens, Greece
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Abstract: | We have made a statistical analysis of the monthly numbers of high-velocity solar wind streamers observed by the time period 1964–1978.The following periods have been found:(1) | Eleven years, 6 and 3 months for the solar wind streamers, which have solar flares as sources. | (2) | Fourteen years and 36, 24, 12, 6, 4, 3 months for the number of solar wind streamers, which have coronal holes as sources. | (3) | Sixteen years for the total number of solar wind streamers. |
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