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Coronal mass ejection — 2026-10-10 08:36 UTC

CME observed to the NW in SOHO LASCO C2/C3, GOES CCOR-1, and STEREO A COR2. The source is former AR 14547 (~N15W105) as directly observed by STEREO A around the west limb from SDO. Observed across SDO AIA 131/171/193/211/304 as field line movement and EUV wave, and brightening, starting around 2026-10-10T07:51Z, partially obscured by a rare transit of the moon across the SDO AIA field-of-view. Also seen in STEREO A EUVI 195/304 as brightening, dimming, and field line movement starting around 2026-10-10T07:55Z.

Details
Event typeCoronal mass ejection
Date
Peak (UTC)—
End (UTC)—
Flare class—
Source location / observed atN16W105
CME speed (most accurate analysis)368 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)2026-10-10T18:42Z3684034 / 97SSWPC_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 here12 Oct 2026, 20:02 EDT
Last observed here12 Oct 2026, 22:18 EDT
In latest snapshotYes
Record identifier5082a321-ccde-56f4-8afa-413391697e35

Local observation history

What this site observed; not complete provider history.

  • — Added

About this data