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Coronal mass ejection — 2026-10-16 06:09 UTC

Faint, wide CME visible to the SW in STEREO A COR2 only. The CME is not clearly seen in SOHO LASCO C2/C3 or GOES CCOR-1 imagery. The potential source is not clearly visible. There is a data gap in STEREO A COR2 and EUV imagery in real-time from 2026-10-15T12:09Z to 2026-10-16T06:09Z. A potential source may be seen in STEREO A EUV imagery anywhere from longitudes W90 to approximately W120 as a gradual, minor dimming may be seen after the data gap starting around 2026-10-16T06:09Z. However, there are not strong post-eruption signatures in imagery, and there is low confidence in this analysis of the source location.

Details
Event typeCoronal mass ejection
Date
Flare class—
CME speed324 km/s
CME analyses1
Linked events—
InstrumentsSTEREO A: SECCHI/COR2

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)2026-10-16T16:20Z32445-31 / —SPlane-of-sky—

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 here16 Oct 2026, 11:52 EDT
Last observed here13 Nov 2026, 19:00 EST
In latest snapshotYes
Record identifiere2c1c5dd-67d7-56c6-9653-cab10aedfa83

Local observation history

What this site observed; not complete provider history.

  • — Added

About this data