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Coronal mass ejection — 2026-10-11 09:12 UTC

Outflow first seen to the NW in SOHO LASCO C2 starting around 2026-10-11T09:12Z. This feature is much easier to see later in its propagation into SOHO LASCO C3, GOES CCOR-1, and STEREO A COR2. The source is most likely outflow following CME: 2026-10-10T16:15Z but may be related to field line movement seen near the NW limb in SDO AIA 193 starting as early as 2026-10-11T05:00Z.

Details
Event typeCoronal mass ejection
Date
Peak (UTC)—
End (UTC)—
Flare class—
Source location / observed at—
CME speed (most accurate analysis)374 km/s
Kp index values (as observed)—
CME analyses1
Linked events—
InstrumentsSOHO: LASCO/C2, SOHO: LASCO/C3, STEREO A: SECCHI/COR2, 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)2026-10-11T20:05Z3741749 / 61SSWPC_CAT—

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 identifier874d726a-18f1-5fd4-8962-77dd6ce63a3e

Local observation history

What this site observed; not complete provider history.

  • — Added

About this data