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GEOMAGNETIC STORMS SolarCycle 24: 2013 x 2014 x 2015 x 2016 x 2017
Geomagnetic storms are more frequent during the solar maximum, when frequent CMEs intersect and electrify the planetary field, and in spring and fall around the equinoxes, when north and south poles of the planetary field are equally distant from the sun.
When a CME intersects the planetary field, field lines, draping the CME leading edge, electrify outer planetary field lines grounded in the atmosphere inside the auroral ovals inducing a voltage potential powering high amperage currents of CME electrons, electrifying sectors of the auroral ovals facing the night sky during geomagnetic storms.
The repelling force between electrons, charging sectors of the auroral ovals after geomagnetic storms, powers expansion of the polar air mass, and increases barometric pressure and wind speed along the jet stream interface with the ambient mid latitude air mass deflecting the air mass away from the pole and powering extreme weather, including lightming storms, flash flooding, blizzards and tornadoes.
West to east movement of weather systems is powered by dipole moments captured by the field, induced by rotation of the ionized core, which increases momentum of orbiting ions in the direction of rotation and super-rotation af the atmosphere and high velocity jet streams, ionized by sunlight.
The Coreolis Force powers anticlockwise rotation of storm cells along moving storm fronts and tornadoes transtorm the momentum of moving charges into dipole moments and sum of moments into a field along the rotation axis attracting cloud droplets toward the ground and high amperage currents of ground charge up tornado field lines and draping tornado surfaces which transform momentum of spiralling charges into dipole moments which increase the attractive force of the tornado field. |
Atoms are Electrons and Positrons
