On the 27-day recurrence of phenomena on the sun

Details On the 27-day recurrence of phenomena on the sun On the 27-day recurrence of phenomena on the sun

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ge%26ae..30..663c&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 30, July-Aug. 1990, p. 663-665. In Russian.

Physics

Solar Rotation, Twenty-Seven Day Variation, Solar Activity, Sunspots

Scientific paper

Observational data on the 27-day recurrence of solar phenomena are
examined. It is noted that the 27-day period of solar rotation is
unstable and associated with secular, 22-year, and 11-year activity
cycles, as well as with global torsional oscillations of sunspots with a
period of about one year.

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