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Coronal mass ejection — 2026-10-28 11:12 UTC

Faint CME observed to the SW in SOHO LASCO C2/C3 and GOES CCOR-1, also very faintly observed to the SW in STEREO A COR2, becoming more defined as it travels further into each coronagraph's field-of-view. The source is likely former AR 14561, located around S10W95 at this time. There is no distinct, clean eruption associated with this CME, but rather slow field line movement and brightening from this region of the disk in GOES SUVI 284 starting around 2026-10-28T09:46Z, also observed as some field line movement and brightening near AR 14561 in STEREO A EUVI 195.

Details
Event typeCoronal mass ejection
Date
Flare class—
CME speed329 km/s
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)2026-10-28T21:34Z32910-14 / 95SSWPC_CATShock arrival not predicted; 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 here28 Oct 2026, 20:01 EDT
Last observed here12 Nov 2026, 19:01 EST
In latest snapshotYes
Record identifiere5fbd777-7f06-5ccc-9798-a62d7e91f3af

Local observation history

What this site observed; not complete provider history.

  • — Changed
  • — Added

About this data