Solar eclipse effect on VLF transmissions
Taken by Neil Miller on April 8, 2024 @ Aiken, SC
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The signal intensity I detected from four VLF transmitters varied as the Moon's shadow passed over the Earth. The temporary recombination in the ionosphere changed the "skip distance" also seen by Kristina Collins with WWV and WWVH. Note the small variation seen in the NAU signal due to no complete shadow between Puerto Rico And Aiken. I use the SuperSID monitor developed by Standford University for my data collection.
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