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Coronal mass ejection — 2026-09-14 11:08 UTC

CME first seen to the E in STEREO A COR2 starting at 2026-09-14T11:08Z. It is also seen to the W in GOES CCOR-1. This CME is covered by a data gap in SOHO LASCO C2/C3 in real time. The source of this CME is an eruption centered around AR 14528 (S11W38) best seen in GOES SUVI 284 beginning around 2026-09-14T10:00Z. Field line movement can be seen accompanied by brightening and ejecta. Post-eruptive arcades can also be seen in SDO AIA 193. There seems to be a northwestward deflection from the location of the source. There are two large coronal holes (a northern and a southern one) nearby, possibly responsible for this deflection.

Details
Event typeCoronal mass ejection
Date
Flare class—
CME speed897 km/s
CME analyses2
Linked events2026-09-17T01:24:00-IPS-001, 2026-09-17T15:10:00-IPS-001
InstrumentsSTEREO 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)2026-09-14T15:34Z744243 / 40CSWPC_CATShock arrival 2026-09-17T09:30Z; Earth glancing blow: yes run (opens in a new tab)
#2 (opens in a new tab) Most accurate (DONKI)2026-09-14T14:28Z897226 / 39CSWPC_CATShock arrival 2026-09-17T06:00Z; Earth glancing blow: yes run (opens in a new tab)

Analyses are measurements and modelled predictions submitted to DONKI; the "most accurate" mark is DONKI's own.

Notifications sent

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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 identifier6aacf98d-6e79-52e1-8252-3c4257b15859

Local observation history

What this site observed; not complete provider history.

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