Heliophysicist interested in solar eruptions and their impacts on the heliospherehttps://bsky.app/profile/halocme.bsky.socialhttps://bsky.app/profile/halocme.bsky.social/post/3lizntaertk22On 2025/02/24 a 2nd, larger proton event started ~22 UT, exceeding the S1 level (37.1 pfu). It was caused by the big CME associated with an M3.9 flare, peaking at 23:02UT. As this video shows, the flare was again from behind the limb. It was likely X-class if observed on disk.25 Feb 2025 20:03 +0000at://did:plc:kc6qcer2e7or2txmrcmstb57/app.bsky.feed.post/3lizntaertk22https://bsky.app/profile/halocme.bsky.social/post/3lcblt5feb22kThis is a screenshot of https://solarnews.nso.edu/sdo-iris-outage-2024/ . I will not be able to post AIA near real-time images for some time, but only convey the updates from JSOC.01 Dec 2024 21:52 +0000at://did:plc:kc6qcer2e7or2txmrcmstb57/app.bsky.feed.post/3lcblt5feb22khttps://bsky.app/profile/halocme.bsky.social/post/3lc47zwfyj22kUnfortunately, this platform seems to compress videos more cruelly than others. Perhaps not good for scientific communications at least for now.29 Nov 2024 18:38 +0000at://did:plc:kc6qcer2e7or2txmrcmstb57/app.bsky.feed.post/3lc47zwfyj22khttps://bsky.app/profile/halocme.bsky.social/post/3lc47wrp3p22vTri-color movie of AIA 211Å, 193Å, 171Å running difference images of the far-side (~30° behind-the-limb) eruption on 2024/11/21. It was a big eruption, dominated by the counterclockwise propagation over the limb, which indicates interactions of the wave with coronal structures.29 Nov 2024 18:36 +0000at://did:plc:kc6qcer2e7or2txmrcmstb57/app.bsky.feed.post/3lc47wrp3p22v