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Stanford University ELF / VLF Receiver

Atmospheric Weather Electromagnetic System for Observation Modelling and Education

Sudden Ionospheric disturbances due to Solar Flares

The ionosphere reacts strongly to the intense x-ray and ultraviolet radiation released by the Sun during a solar flare, solar storm, or coronal mass ejection. By monitoring the signal strength from distant VLF transmitters and noting unusual changes as the waves bounce off the ionosphere, we can monitor and track these disturbances.

© http://solar-center.stanford.edu/SID/science/

VLF Station list :




Stationsverantwortlicher Mag. Klaus Huber Telefon:+43 (0)316 380 - 5276

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