{"id":793210,"date":"2025-01-31T12:00:08","date_gmt":"2025-01-31T17:00:08","guid":{"rendered":"http:\/\/spaceweekly.com\/?p=793210"},"modified":"2025-01-31T12:00:08","modified_gmt":"2025-01-31T17:00:08","slug":"strong-m6-7-solar-flare-erupts-from-region-3978-cme-produced","status":"publish","type":"post","link":"https:\/\/spaceweekly.com\/?p=793210","title":{"rendered":"Strong M6.7 solar flare erupts from Region 3978, CME produced"},"content":{"rendered":"


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A Type II Radio Emission with an estimated velocity of 673 km\/s was associated with the flare event, suggesting a coronal mass ejection (CME) was associated with the event.<\/p>\n

A 10cm Radio Burst (TenFlare) lasting 14 minutes and with a peak flux of 280 sfu. This indicates that the electromagnetic burst associated with a solar flare at the 10cm wavelength was double or greater than the initial 10cm radio background. This can be indicative of significant radio noise in association with a solar flare. This noise is generally short-lived but can cause interference for sensitive receivers including radar, GPS, and satellite communications.<\/p>\n

Radio frequencies were forecast to be most degraded over South America, the South Atlantic Ocean, and parts of Africa.<\/p>\n

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