An Investigation for the Cause of Formation of the Major Period of the Relative Sunspot Numbers with Bipolarity

Details An Investigation for the Cause of Formation of the Major Period of the Relative Sunspot Numbers with Bipolarity An Investigation for the Cause of Formation of the Major Period of the Relative Sunspot Numbers with Bipolarity

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988acasn..29..297y&link_type=abstract

Acta Astronomica Sinica, Vol.29:3, P. 304, 1988

Astronomy and Astrophysics

Astronomy

Scientific paper

In this paper, the latest mean orbit elements of the major planets have been used to calculate the orbital motion of the Sun's center in the ecliptic coordinates of barycenter of the solar system with reference to the epoch JD = 2451545.0. The coefficients of crosscorrelation between the orbital motion of Sun's center and the relative sunspot numbers for the period 1700 to 1985 have been calculated, also the power spectra have been analysed. It is found that the major period term of the relative sunspot numbers with bipolarity is not 22 yr but 19.9 yr.

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