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Issued on 2022 Mar 30 1542 UTC
A full halo coronal mass ejection was detected by CACTus on March 30th 06:36UT, with an average velocity of 582 km/s. This event is believed to be backsided and is not expected to have an impact on the solar wind conditions.
Issued on 2022 Mar 30 1945 UTC
A class X1.3 solar X-ray flare occurred on 30 March 2022 with peak time 17:37UT. The region of origin was active region NOAA 2975. Additionally, a type II and type IV radio emission were detected at 17:32UT and 17:34UT respectively, indicating an associated CME.
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