Solar radio flux at 10-cm and Sun's motion.

Details Solar radio flux at 10-cm and Sun's motion. Solar radio flux at 10-cm and Sun's motion.

Jun 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999ppmto..18..176z&link_type=abstract

Publ. Purple Mt. Obs., Vol. 18, No. 2, p. 176 - 178

Physics

Solar Motion: Solar System, Solar Radio Radiation: Solar Patrol

Scientific paper

The solar radio flux at 2800 MHz from Ottawa during 1947 - 1990 has been used to make linear correlation with dL/dt, the rate of change of the angular momentum of the Sun around the center of mass of the solar system. A coefficient of correlation, 0.822 with a confidence level far higher than 99.9% is found, when the time lag τ ≡ 2 - 3 years. In the same period of time the linear coefficient of correlation of the relative sunspot number with dL/dt is 0.829 with a confidence level far higher than 99.9%.

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