Periodicities in the occurrence of aurora as indicators of solar variability.

Details Periodicities in the occurrence of aurora as indicators of solar variability. Periodicities in the occurrence of aurora as indicators of solar variability.

Nov 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983nascp2280..349d&link_type=abstract

NASA Conf. Publ., NASA CP-2280, p. 349 - 352

Computer Science

Aurorae:Solar Activity Cycles, Solar Activity Cycles:Aurorae

Scientific paper

A compilation of records of the aurora observed in China from the Time of the Legends (2000 - 3000 B.C.) to the mid-18th century has been used to infer the frequencies and strengths of solar activity prior to modern times. The results show periodicities in solar activity that contain average components with a long period (≡412 years), three middle periods (≡38 years, ≡77 years, and ≡130 years), and the well known short period (≡11 years).

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