Fundamentals of the Thermohydrogravidynamic Theory of the Global Seismotectonic Activity of the Earth

<table>The initial planetary configuration of the outer planet <svg height="12.15" id="M866" style="vertical-align:-3.3907pt" version="1.1" viewbox="0 0 12.2 12.15" width="12.2" xmlns="http://www.w3.org/2000/svg" xmlns:xlink="http://www.w3.org/1999/xlink">
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</svg> (Mars or Jupiter, Saturn, Uranus, Neptune, and Pluto) and the Earth <svg height="12.15" id="M867" style="vertical-align:-3.3907pt" version="1.1" viewbox="0 0 14.675 12.15" width="14.675" xmlns="http://www.w3.org/2000/svg" xmlns:xlink="http://www.w3.org/1999/xlink">
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</svg>.</table>

International Journal of Geophysics

fig6

Figure 6

Figure 6: Fundamentals of the Thermohydrogravidynamic Theory of the Global Seismotectonic Activity of the Earth 