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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Xanthakis, J., Poulakos, C. & Petropoulos, B. Possible periodicities of high-speed solar plasma. Astrophys Space Sci 141, 233–250 (1988). https://doi.org/10.1007/BF00639491
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DOI: https://doi.org/10.1007/BF00639491