Schumann resonances are extremely-low-frequency
Schumann resonances data is provided by the Space Observing System located in Tomsk, Russia https://sosrff.tsu.ru/
The seismic energy released from an earthquake is dependent on the magnitude of the rupture. A one magnitude increase corresponds to a 32x increase in the energy released from the event. The seismic energy released can be calculated in joules (J) or watt-hours (Wh). Because of how the energy released from earthquakes scales, a nearly accurate count of the amount of energy released globally for any given day/time period can be accomplished by calculating the energy released for all earthquakes magnitude 4 and greater and then summing them. Doing this allows us to observe the rhythms in global seismicity, and to categorize each day's "cumulative magnitude". Global Seismic Data provided by Volcano Discovery.
The radiation belts are "clouds" or "populations" or very-high-energy relativistic particles trapped in Earth's magnetosphere that surround the planet from ~ 0.5 Earth Radii (Er) to 9 Er. Generally there are two radiation belts, an inner proton (+) dominant belt from 1-3 Er, and an outer electron (-) dominant belt from 3-9 Er. Radiation belts data is provided by the GFZ Helmholtz Centre for Geosciences
When charged particles precipitate down to Earth as guided by the magnetic field, they interact energetically with elements and molecules in the atmosphere, causing them to reach higher vibratory states through ionization, generating plasma. The dancing colorful lights we sometimes see overhead during a geomagnetic storm from a solar storm impact is that plasma and is known as aurora.
The Auroral Intensity Prediction Model is provided by the GFZ Helmholtz Centre for Geosciences
Solar Imagery is provided by the NASA/ESA Solar Dynamics Observatory
This model of the Solar System with accurate planetary positions and geometry is provided by Solar System Scope.
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