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Coronal mass ejection — 2026-11-07 09:36 UTC

First in a pair of far-sided CMEs from a filament eruption, followed by slower CME 2026-11-07T10:24Z. This leading edge is more faint and observed to the NW in SOHO LASCO C2/C3, GOES CCOR-1, and STEREO A COR2. The source for both is a far-sided filament eruption, observed well in GOES SUVI 284/304 over the N limb starting around 2026-11-07T08:04Z, with the filament first lifting off as early as 2026-11-07T06:51Z. Also observed to the NW in STEREO A EUVI 195 as field line movement around 2026-11-07T08:35Z and STEREO A EUVI 304 as filament ejecta around 2026-11-07T06:15Z.

Details
Event typeCoronal mass ejection
Date
Flare class—
CME speed507 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)2026-11-07T17:21Z5072630 / 168CSWPC_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)
Shock 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 here7 Nov 2026, 19:01 EST
Last observed here13 Nov 2026, 19:00 EST
In latest snapshotYes
Record identifiera98c8b88-ea7b-5800-85cf-b405502058d2

Local observation history

What this site observed; not complete provider history.

  • — Changed
  • — Added

About this data