CME
Taken by Rudolf Slošiar on February 4, 2026 @
Slovakia
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Details:
Increased solar activity continues and sunspot AR4366 is only halfway there. So I checked the SID monitor data and it was worth it! CMEs from M 1.72 to X 4.21. The attached graph shows records from two VLF transmitters and the CMEs are very clearly visible. In the blue record of the DHO38 transmitter there is a significant decrease in signal intensity. This is not caused by solar activity but by a regular shutdown of the transmitter between 7:00 and 7:30! This is how the SID monitor RUDY BASE recorded it.
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