Possible periodicities of high-speed solar plasma |
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| Authors: | J Xanthakis C Poulakos B Petropoulos |
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| Institution: | 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.
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Fourteen years and 36, 24, 12, 6, 4, 3 months for the number of solar wind streamers, which have coronal holes as sources.
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Sixteen years for the total number of solar wind streamers.
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