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Coronal mass ejection — 2026-10-06 09:53 UTC

CME observed to the NE in STEREO A COR2, also faintly observed to the N in SOHO LASCO C2/C3 and GOES CCOR-1. The source is AR 14549, associated with an M1.8 class flare (N08E07) peaking at 2026-10-06T08:05Z, observed in SDO AIA 131. Also observed as field line movement, EUV wave, dimming, and brightening in SDO AIA 171/193 starting around 2026-10-06T07:52Z, with brightening and filament ejecta in SDO AIA 304. Also observed well in STEREO A EUVI 195/304 starting around 2026-10-06T08:05Z as field line movement and filament ejecta on the NE limb, with some northward deflection.

Details
Event typeCoronal mass ejection
Date
Peak (UTC)—
End (UTC)—
Flare class—
Source location / observed atN08E07
CME speed (most accurate analysis)424 km/s
Kp index values (as observed)—
CME analyses1
Linked events2026-10-06T07:47:00-FLR-001, 2026-10-10T14:33:00-IPS-001, 2026-10-10T14:35:00-RBE-001, 2026-10-10T15:00:00-GST-001, 2026-10-10T15:33:00-MPC-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)2026-10-06T18:49Z4242428 / -1SSWPC_CATShock arrival 2026-10-09T20:00Z; 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.

View at the source

Provenance

SourceNASA DONKI — Space Weather Events
FeedDONKI CME
Provider data as ofnot stated
First observed here12 Oct 2026, 20:02 EDT
Last observed here12 Oct 2026, 22:18 EDT
In latest snapshotYes
Record identifier713fb39d-1cb3-5bba-bfea-f8b38c5f9811

Local observation history

What this site observed; not complete provider history.

  • — Added

About this data