💾 Archived View for radia.bortzmeyer.org › presto › 2024-05-27.gmi captured on 2024-08-31 at 12:04:26. Gemini links have been rewritten to link to archived content
⬅️ Previous capture (2024-06-16)
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Issued on 2024 May 27 0807 UTC
An X2.8 flare, with peak time 07:08 UTC on May 27, was recorded by GOES-16. This flare originated beyond the south-east limb and is likely associated to a returning active region from the last rotation (NOAA AR 3664). Associated Type II and Type IV radio emissions were observed starting at 06:59 UTC and 07:05 UTC, respectively. The coronagraph data will be analysed when it becomes available, however, due to the location of the flaring region any Coronal Mass Ejection is not likely to have a strong Earth directed component. As this region continues to rotate onto the solar disk, there is an overall heightened risk for strong M and X-class flaring over the next days.
Issued on 2024 May 27 1824 UTC
A halo Coronal Mass Ejection (CME) was detected in SOHO/LASCO-C2 data from 07:24 UTC May 27. This CME has a plane of sky speed of around 800km/s and was predominantly directed to the east. It is associated with the X2.8 flare originating from beyond the east limb, with peak time 07:08 UTC on May 27. Due to the location of the source region, initial modelling suggests that the CME is not expected to impact Earth.