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

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

Jul 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999arep...43..485v&link_type=abstract

Astronomy Reports, Volume 43, Issue 7, July 1999, pp.485-486

Astronomy and Astrophysics

Astronomy

7

Scientific paper

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.

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