{"id":776580,"date":"2024-02-11T09:18:03","date_gmt":"2024-02-11T14:18:03","guid":{"rendered":"http:\/\/spaceweekly.com\/?p=776580"},"modified":"2024-02-11T09:18:03","modified_gmt":"2024-02-11T14:18:03","slug":"m6-7-solar-flare-erupts-from-region-3559-producing-s2-moderate-solar-radiation-storm","status":"publish","type":"post","link":"https:\/\/spaceweekly.com\/?p=776580","title":{"rendered":"M6.7 solar flare erupts from Region 3559, producing S2 – Moderate solar radiation storm"},"content":{"rendered":"


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A moderately strong solar flare measuring M6.7 erupted from Active Region 3559 (beta-gamma) at 04:38 UTC on January 29, 2024. The event started at 03:54 and ended at 05:15 UTC.<\/strong><\/p>\n

A Type II Radio Emission with an estimated velocity of 512 km\/s was associated with the event. Type II emissions occur in association with eruptions on the Sun and typically indicate a coronal mass ejection (CME) is associated with a flare event.<\/p>\n

A 10cm Radio Burst (tenflare) with a peak flux of 2 700 sfu and lasting 36 minutes was also associated with the event. A 10cm radio burst 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 Australia and far SE Asia.<\/p>\n

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