Earth Analytics

Schumann Resonances 0-40 Hz (E_z) Spectrogram UTC+7

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Schumann resonances are extremely-low-frequency
Schumann resonances data is provided by the Space Observing System located in Tomsk, Russia https://sosrff.tsu.ru/

Real-Time Radiation Belts (past 7 days)

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 (E_r) to 9 E_r. Generally there are two radiation belts, an inner proton (+) dominant belt from 1-3 E_r, and an outer electron (-) dominant belt from 3-9 E_r. Radiation belts data is provided by the GFZ Helmholtz Centre for Geosciences

Northern Hemisphere Aurora Prediction Model

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