Abstract
Past attempts to link sunspots with the gravitational attraction by planets or with the orbital motion of the Sun have not been successful. In this paper the changes in orbital angular momenta of planets due to gravitational perturbation are considered. Ninety-eight percent of the angular momentum of the solar system is contained in the orbital motion of the four giant planets Jupiter, Saturn, Uranus, and Neptune. The potential relevance of the motion of these giant planets to the sunspot variations is investigated. The perturbation forces between two planets vary periodically over their mutual synodic period and show symmetry about heliocentric conjunction and opposition. Certain pairs and pair groupings in the giant planets have highly commensurable mean motions. Their synodic half periods correspond to the principal sunspot number frequencies. In particular, the 10 yr period appears to be associated with the relative motion of the pair Jupiter — Saturn, the 90 yr period with that of Uranus and Neptune, and the 11 yr period with the motion of the pair Jupiter — Saturn relative to the pair Uranus — Neptune. The physical link between planetary motion and sunspots is seen in the outward transfer of angular momentum from the Sun to the fringe of the solar system. We assume the existence of a basic energy flow from the Sun outward effected by accelerations of outer planets through gravitational perturbation by inner planets rhythmically modulated by the orbital configurations of all the planets. The transmission of gravitational torque in the solar system is assumed to cause changes in the global and local vorticity patterns of low inertia materials such as the solar photosphere and the terrestrial atmosphere; this provides a mechanism of control on the terrestrial atmospheric circulation and climate by extraterrestrial forces either directly or through modulation of solar activity.
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References
C. M. Smythe and J. A. Eddy, Nature, 266, 1977.
R. E. Roy and M. W. Ovenden, Mon. Not. Roy. Astr. Soc., 114, 232, 1954.
L. Schlamminger, Sunspot periods show a synchronization with the resonance periods and the perturbation periods of planets (unpublished), 1977.
T. J. Cohen and P. R. Lintz, Nature, 250, 398, 1974.
K. Sukurai, Nature, 269, 402, 1977.
J. A. Eddy, P. A. Gilman, and D. E. Trotter, Solar Phys., 46, 3, 1976.
W. Gleissberg, Sterne und Weltraum, 7–8, 229, 1977.
1859 Wolf, R,; Compt Rend. Acad. Sci. Paris; Vol. 48, p. 231.
1872 De la Rue, W., Stewart, B., Loewy, B.; Proc. Roy. Soc. London; Vol. 20. pp. 210–218.
1899 Birkeland, Kr.; Recherches sur les taches du soleil et leur origine; Skrift. Vidensk., Vol. 1, Christiania.
1900 Brown, E. W.; A possible explanation of the sunspot period; Monthly Notices, Royal Astron. Society, Vol. 60, p. 599–606.
1911 Schuster, A,; The influence of the planets on the formation of sun- spots; Proc. Roy. Soc. London; Vol. 85, p. 309–323.
1918 Pocock, R. J.; Monthly Notices, Roy. Astr. Soc. London; Vol. 79, p. 54.
1936 Sanford, F.; Smiths. Misc. Coll., Vol. 95, 11 pp.
1937 Stetson, H. T.; Sunspots and their effects; McGraw Hill, 1937.
1946 Johnson, M.; Correlations of cycles in weather, solar activity, geomagnetic values and planetary configurations; Phillips and Van Orden, San Francisco.
1947 Clayton, H. H.; Solar cycles; Smiths. Misc. Coll., Vol. 106, No. 22.
1954 Anderson, C. N.; Geophys. Res.; Vol. 59, p. 455
1954 Nelson, J.; Transactions, Inst. Rad. Eng.; CS-2, p. 19.
1962 Suda, T.; J. Met. Soc. Japan; 40, p. 278.
1965 Jose, P.; Astron. Journ. 70, p. 193–200.
1965 Ward, F. I.; Astrophys. Journ., 141, p. 534.
1965 Wood, K. D., Wood, R. M.; Nature, Vol. 208, p. 129–131.
1966 Trellis, M.; CR Acad. Sci., B, 262, p. 312.
1967 Takahashi, K.; Rad. Res. Lab.; Vol. 14, p. 237.
1967 Bigg, E. K.; Astr. Journal; Vol. 72, p. 463–466.
1968 Bollinger, C. J.; Tellus XX, 3, p. 412–416.
1969 Nickel, G. H.; Rep. Lawrence Radiation Lab., URCL - 502264.
1970 Bureau, R. A., Craine, L. B.; Nature, 228, p. 984
1972 Wood, K. D.; Nature, 240, p. 91–93.
1972 Sleeper, H. P. Jr.; Planetary resonances, bistable oscillation modes and solar activity cycles; NASA Contractor Report 2035, prepared by Northrop Services Inc., Huntsville, Alabama.
1975 Okal, E., Anderson, E. L.; Nature, 255, p. 511.
1977 Smythe, C. M., Eddy, J. A.; Nature, 266, p. 435.
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© 1979 D. Reidel Publishing Company, Dordrecht, Holland
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Mörth, H.T., Schlamminger, L. (1979). Planetary Motion, Sunspots and Climate. In: McCormac, B.M., Seliga, T.A. (eds) Solar-Terrestrial Influences on Weather and Climate. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-9428-7_19
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DOI: https://doi.org/10.1007/978-94-009-9428-7_19
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