DONKI Header

CCMC DONKI

DONKI: Menu Page

Go to:

DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2026-07-09T07:53Z ( STEREO A: SECCHI/COR2 )
All Detecting Spacecrafts:
STEREO A: SECCHI/COR2
GOES: CCOR-1
Activity ID: 2026-07-09T07:53:00-CME-001 (version 1)
Source Location: S10W34
Active Region Number: 14485
Note Keyword:
OVR: Event partially overlaps with another CME
Source Signature Keyword:
FLR: Flare
PEA: Post eruption arcade
BR: Brightening
DIM: Dimming
EUVW: EUV Wave
Morphology Keyword:
Note: Possibly two overlapping CMEs visible to the E in STEREO A COR2 imagery and to the S/SW in GOES CCOR-1 imagery starting at 2026-07-09T07:53Z and 2026-07-09T08:23Z based on STEREO A COR2 imagery. The source of this CME(s) is an eruption from the area of Active Region 14485 (S10W34) starting around 2026-07-09T06:56Z to the SW in GOES SUVI 195 with additional eruption signatures to the NW of AR 14485 (S10W34) in GOES SUVI 195 starting around 2026-07-09T07:08Z. There is a following eruption starting around 2026-07-09T07:48Z with associated brightening and dimming to the N/NW of the Active Region spanning roughly from W25 to W10 and S00 to S12. An EUV wave is visible in GOES SUVI 284 following the main eruption with post-eruptive arcades starting around 2026-07-09T08:53Z as seen in GOES SUVI 195 and 284. These eruptions are also visible in STEREO A EUV 195 and 304 as well as in SDO/AIA wavelengths following an eclipse.
Version 1 submitted on 2026-07-09T13:34Z by Carina Alden
	
A Notification with ID 20260709-AL-001 was sent on 2026-07-09T14:09Z
A Notification with ID 20260709-AL-003 was sent on 2026-07-09T22:13Z

The List of CME Analysis already entered:
Event Type Catalog
Measurement TypeCME measurement type: Leading Edge (LE), Shock Front (SH), Right Hand Boundary (RHB), Left Hand Boundary (LHB), Black/White Boundary (BW), Prominence Core (COR), Disconnection Front (DIS), Trailing Edge (TE).
Prime?"primary flag" which is either True or False. If there are multiple CME analysis entries for a single CME, this flag would indicate which analysis is considered most accurate per measurement type. This is a helpful flag if you would like to download only one most accurate CME analysis per CME per Measurement Type
Technique Long Lat Speed Type Half Width Time 21.5 Note WSA-ENLIL+Cone Result(s) Measured On Submitted By
CME Analysis M2M_CATALOG LE true SWPC_CAT 20.0 -8.0 749.0 C 31.0 2026-07-09T11:57Z Parameters based on best fit using STEREO A COR2 and GOES CCOR-1 imagery including both fronts or lobes of the CME(s) visible more clearly in STEREO A COR2 imagery. 1: Result 1 (2.0 AU)
Earth = 2026-07-12T01:38Z
BepiColombo = 2026-07-10T08:40Z
Juice = 2026-07-13T18:59Z
OSIRIS-APEX = 2026-07-13T01:26Z
Parker Solar Probe = 2026-07-11T05:35Z
Europa Clipper = 2026-07-13T10:00Z
STEREO A = 2026-07-12T20:00Z
2026-07-09T13:21Z Carina Alden on 2026-07-09T13:36Z



All directly linked activities:
2026-07-09T06:51:00-FLR-001
FLR Type: C2.7


Comments by users:
0 comment received.
Insert title here

The Moon to Mars Space Weather Analysis Office and other entities provide data to DONKI as a courtesy to the community.
By visiting this site, you acknowledge that you understand and agree to the Important Disclaimer Notice

If you are looking for the official U.S. Government forecast for space weather, please go to NOAA's Space Weather Prediction Center (https://swpc.noaa.gov). This "Experimental Research Information" consists of preliminary NASA research products and should be interpreted and used accordingly.

Curator: Chiu Wiegand | NASA Official: Dr. Masha Kuznetsova | Privacy and Security Notices | Accessibility | CCMC Data Policy