The planetary system and solar-terrestrial phenomena |
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| Authors: | Ivanka Jakubcová Miloš Pick Reviewer J Vondrák |
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| Institution: | (1) Geophysical Institute, Czech. Acad. Sci., Prague |
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| Abstract: | Summary The Sun moves at different distances round the barycentre of the Solar System with different velocities depending on the distribution of the planets. The mean period of the Sun's motion round the barycentre of 11.8627 years and its time variability were observed. A relation between the basic period of 178.4 years and other periods pi in the Sun's motion (pi=178.4/i; i=1, 2, ...) was found. The consistency of the periods in the Sun's motion round the barycentre with the periods of different solar-terrestrial phenomena was studied. It seems that the planetary system governs these phenomena.
         n ¶rt;  ¶rt;u nu¶rt;  a u   a     ama  um (11,8627 m) u auauu. a a¶rt;a  nuua   ¶rt; m¶rt;u nu¶rt;au ¶rt;uu a (pi=178,4/i).  mu nu¶rt;a u nma nu¶rt; n¶rt; a - u.  na¶rt;u nu¶rt; am, m a uma nam mu u.
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