Solar cycles in the energy and mass outputs of the heliospheric plasma

I. S. Veselovskii, A. V. Dmitriev, O. A. Panasenko, A. V. Suvorova

研究成果: 雜誌貢獻期刊論文同行評審

8 引文 斯高帕斯(Scopus)

摘要

The variability of the Sun as a star is traced in its integrated solar-wind mass and energy fluxes. Direct plasma measurements in the heliosphere over more than the last thirty years indicate that these quantities have experienced relative variations by factors of 1.5 - 2, approximately in antiphase with the last three eleven-year solar cycles. A rising trend is noted over this time, with a similar relative-variation scale. This trend may be a manifestation of a "secular" cycle with a duration of 60 - 70 years or longer.

原文???core.languages.en_GB???
頁(從 - 到)485-486
頁數2
期刊Astronomy Reports
43
發行號7
出版狀態已出版 - 7月 1999

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