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Coronal mass ejection — 2026-10-06 06:23 UTC

Full halo CME in SOHO LASCO C2/C3 and GOES CCOR-1, first seen to the NE in STEREO A COR2 (shock fully to the E, wide). The source is AR 14549, associated with an M1.4 flare (N10E12) peaking at 2026-10-06T06:10Z, observed in SDO AIA 131. Also observed as an EUV wave, field line movement, brightening, filament ejecta, and small post-eruptive arcade in SDO AIA 131/171/193/304. Additionally observed on the NE limb of STEREO A EUVI 195 as field line movement and EUV wave, and EUVI 304 as filament ejecta.

Details
Event typeCoronal mass ejection
Date
Flare class—
CME speed573 km/s
CME analyses2
Linked events2026-10-06T05:38:00-FLR-001, 2026-10-10T01:56:00-IPS-001
InstrumentsSTEREO A: SECCHI/COR2, SOHO: LASCO/C2, SOHO: LASCO/C3, GOES: CCOR-1

Research information from NASA DONKI, not an operational warning. NOAA SWPC is the official US source of space weather forecasts.

CME analyses

Analyses of this coronal mass ejection
AnalysisTime at 21.5 R☉ (UTC)Speed (km/s)Half angle (°)Lat / lon (°)TypeTechniqueModel runs (WSA-ENLIL)
#1 (opens in a new tab) Most accurate (DONKI)2026-10-06T12:42Z5704026 / 6CSWPC_CATShock arrival 2026-10-09T04:16Z; Earth glancing blow: no run (opens in a new tab)
#2 (opens in a new tab) Most accurate (DONKI)2026-10-06T12:19Z573494 / 0CSWPC_CATShock arrival 2026-10-09T02:21Z; Earth glancing blow: no run (opens in a new tab)

Analyses are measurements and modelled predictions submitted to DONKI; the "most accurate" mark is DONKI's own.

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Provenance

SourceNASA DONKI — Space Weather Events
FeedDONKI CME
Provider data as ofnot stated
First observed here12 Oct 2026, 20:02 EDT
Last observed here13 Oct 2026, 20:56 EDT
In latest snapshotYes
Record identifiera43b8550-4ca7-5cfe-9776-7069984e389c

Local observation history

What this site observed; not complete provider history.

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About this data