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Coronal mass ejection — 2026-10-02 00:53 UTC

CME faintly visible to the NE in STEREO A COR2 and the NW in SOHO LASCO C2/C3 and GOES CCOR-1. The source is likely a gradual eruption with moving field lines best seen in SDO AIA 193 starting around 2026-10-01T17:43Z. Post-eruption arcades are also visible, and best seen after a data gap in STEREO A EUV 195 imagery. The data gap is from 2026-10-01T14:35Z to 2026-10-02T00:55Z.

Details
Event typeCoronal mass ejection
Date
Flare class—
CME speed255 km/s
CME analyses1
Linked events—
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)2026-10-02T12:52Z2552833 / 53SSWPC_CATShock arrival not predicted; Earth glancing blow: no run (opens in a new tab)
Shock 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 here12 Oct 2026, 20:02 EDT
Last observed here14 Oct 2026, 16:02 EDT
In latest snapshotYes
Record identifiera6de4617-0d86-5c31-8003-af3e12a9fb3a

Local observation history

What this site observed; not complete provider history.

  • — Added

About this data